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description Publicationkeyboard_double_arrow_right Article , Other literature type 2021Publisher:Springer Science and Business Media LLC Lucy Allington; Carla Cannone; Ioannis Pappis; Karla Cervantes Barron; Will Usher; Steve Pye; Edward Brown; Mark Howells; Constantinos Taliotis; Caroline Sundin; Vignesh Sridha; Eunice Ramos; Maarten Brinkerink; Paul Deane; Andrii Gritsevskyi; Gustavo Moura; Arnaud Rouget; David Wogan; Edito Barcelona; Holger Rogner; Stephanie Hirmer;Abstract Energy system modelling can be used to assess the implications of different scenarios and support improved policymaking. However, access to data is often a barrier to starting energy system modelling in developing countries, thereby causing delays. This article therefore provides data that can be used to create a simple zero order energy system model for Mauritania, which can act as a starting point for further model development and scenario analysis. The data are collected entirely from publicly available and accessible sources, including the websites and databases of international organizations, journal articles, and existing modelling studies. This means that the dataset can be easily updated based on the latest available information or more detailed and accurate local data. These data were also used to calibrate a simple energy system model using the Open Source Energy Modelling System (OSeMOSYS) and two stylized scenarios (Fossil Future and Least Cost ) for 2020-2050. The assumptions used and results of these scenarios are presented in the appendix as an illustrative example of what can be done with these data. This simple model can be adapted and further developed by in-country analysts and academics, providing a platform for future work.
https://doi.org/10.2... arrow_drop_down https://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefhttps://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.21203/rs.3.rs-479591/v2&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert https://doi.org/10.2... arrow_drop_down https://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefhttps://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.21203/rs.3.rs-479591/v2&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2024Publisher:Springer Science and Business Media LLC Amel Kasri; Kamel Ouari; Youcef Belkhier; Mohit Bajaj; Ievgen Zaitsev;AbstractEnhancing the efficiency of the electric vehicle’s powertrain becomes a crucial focus, wherein the control system for the traction motor plays a significant role. This paper presents a novel electric vehicle traction motor control system based on a robust predictive direct torque control approach, an improved version of the conventional DTC, where the traditional switching table and the hysteresis regulators are substituted with a predictive block based on an optimization algorithm. Additionally, a robust predictive speed loop regulator is employed instead of the proportional-integral regulator, which integrates a new cost function with a finite horizon, incorporating integral action into the control law based on a Taylor series expansion. This technique’s primary benefit is its independence from the necessity to measure and observe external disturbances, as well as uncertainties related to parameters. The effectiveness of the suggested system was confirmed through simulation and experimental results under the OPAL-RT platform. The findings indicate that the proposed approach outperforms the conventional method in terms of rejecting disturbances, exhibiting robustness to variations in parameters, and minimizing torque ripple.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1038/s41598-024-65988-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 6 citations 6 popularity Average influence Average impulse Top 10% Powered by BIP!
more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1038/s41598-024-65988-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2014 FrancePublisher:Springer Science and Business Media LLC Authors: Arnoult, Stéphanie; Brancourt-Hulmel, Maryse;The lignocellulosic C4 perennial crop miscanthus and, more particularly, one of its species, Miscanthus × giganteus, are especially interesting for bioenergy production because they combine high biomass production with a low environmental impact. However, few varieties are available, which is risky due to disease susceptibility. Gathering worldwide references, this review shows a high genotypic and environmental variability for traits of interest related to miscanthus biomass production and composition, which may be useful in breeding programs for enhancing the availability of suitable clones for bioenergy production. The M. × giganteus species and certain clones in the Miscanthus sinensis species seem particularly interesting due to high biomass production per hectare. Although the industrial requirements for biomass composition have not been fully defined for the different bioenergy conversion processes, the M. × giganteus and Miscanthus sacchariflorus species, which show high lignin contents, appear more suitable for thermochemical conversion processes. In contrast, the M. sinensis species and certain M. × giganteus clones with low lignin contents were interesting for biochemical conversion processes. The M. sacchariflorus species is also interesting as a progenitor for breeding programs, due to its low ash content, which is suitable for the different bioenergy conversion processes. Moreover, mature miscanthus crops harvested in winter seem preferred by industry to enhance efficiency and reduce the expense of the processes. This investigation on miscanthus can be extrapolated to other monocotyledons and perennial crops, which may be proposed as feedstocks in addition to miscanthus.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1007/s12155-014-9524-7&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routeshybrid 82 citations 82 popularity Top 1% influence Top 10% impulse Top 10% Powered by BIP!
more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1007/s12155-014-9524-7&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article 2015 FrancePublisher:IEEE Authors: Cany, Camille; Mansilla, Christine; Mathonnière, Gilles; da Costa, Pascal;n the French context of increasing renewable penetration and significant nuclear power, the optimal contribution of this energy source is discussed from two viewpoints. On the one hand, from the social planner viewpoint, the nuclear optimum contribution is the one that minimizes the overall electric price, whatever the resulting load factor. The use of screening curves, often implemented to design the optimal power mix is questioned, being highly sensitive to the assumptions. On the other hand, from the plant operator viewpoint, the nuclear power plants need to amortize the capital expenses, hence achieve the longest operating time. With a view to make the two viewpoints meet, we propose to operate nuclear power plants as baseloads and consider modulation through the power use, i.e. supply electricity to the electric system when requested and use the remaining power to produce other valuable products, such as heat or hydrogen.
Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverConference object . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationConference object . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/eem.2015.7216627&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverConference object . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationConference object . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/eem.2015.7216627&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint , Journal 2012Embargo end date: 01 Jan 2012 Italy, France, Spain, Italy, France, Italy, France, Italy, Netherlands, United Kingdom, Spain, Italy, Italy, Italy, Spain, United Kingdom, Italy, Switzerland, Spain, France, United Kingdom, United Kingdom, United Kingdom, France, France, Italy, Spain, Netherlands, France, France, France, Italy, Netherlands, FrancePublisher:Springer Science and Business Media LLC Publicly fundedFunded by:SNSF | Search for New Physics in..., SNSF | High Precision CP Violati..., SNSF | Particle Physics in the L...SNSF| Search for New Physics in Electroweak Penguin Transitions at LHCb ,SNSF| High Precision CP Violation Physics at LHCb ,SNSF| Particle Physics in the LHC EraAlexey Novoselov; J. Magnin; V. N. La Thi; Naylya Sagidova; Antonio Falabella; Albert Bursche; M. Matveev; Evelina Gersabeck; V. Tisserand; Maximilian Schlupp; C. Potterat; Cristina Lazzeroni; U. Kerzel; Marie Helene Schune; B. Schmidt; C. J. Parkinson; B. Sciascia; F. Xing; G. N. Patrick; Massimiliano Ferro-Luzzi; R. Vazquez Gomez; P. M. Bjørnstad; O. Francisco; J. Dickens; B. Pietrzyk; Jessica Prisciandaro; J. Buytaert; Nazim Hussain; Marcin Kucharczyk; Marcin Kucharczyk; Marcin Kucharczyk; T. E. Latham; I. R. Kenyon; H. Ruiz; D. Souza; F. Eisele; Th. S. Bauer; E. van Herwijnen; A. Bates; N. A. Smith; R. Silva Coutinho; Marc-Olivier Bettler; Alessia Satta; J. Anderson; Leonid Kravchuk; C. D'Ambrosio; D. Savrina; J. Panman; Manuel Schiller; Z. Mathe; Alexey Zhelezov; E. Grauges; Timothy Gershon; Timothy Gershon; S. C. Haines; David Ward; A. Puig Navarro; D. Wiedner; T. Huse; K. Hennessy; P. Rodriguez Perez; Andrey Vorobyev; Po-Hsun Chen; Po-Hsun Chen; Evgeny Gushchin; Jack Benton; Sebastian Bachmann; R. S. Huston; H. Dijkstra; A. D. Nguyen; Gregory Ciezarek; N. Chiapolini; A. Borgia; Adriano Lai; S. Eidelman; Ronan McNulty; Daniel Lacarrere; J. Rouvinet; Krzysztof Grzegorz Sobczak; Minh Tâm Tran; A. D. Webber; T. Lesiak; Y.Y. Li; Mikhail Zavertyaev; Ph. Charpentier; Ronan Wallace; Giulia Manca; Marcin Chrzaszcz; P. Diniz Batista; Dmitry Popov; C. Voß; V. V. Gligorov; Ivan Belyaev; Andrey Golutvin; Andrey Golutvin; Andrey Golutvin; W. Witzeling; Alessandro Petrolini; J. van Tilburg; Thomas Blake; A. Nomerotski; A. Nomerotski; R. Lefèvre; V.G. Shevchenko; Jing Wang; Robert Currie; S. Roiser; Rustem Dzhelyadin; Edwige Tournefier; Edwige Tournefier; K. De Bruyn; A. Gomes; Giacomo Graziani; A. Richards; Marc S. Williams; Patrick Owen; A. Palano; Piotr Morawski; J. P. Lees; P. Shatalov; T. Brambach; M. Seco; Nikolay Bondar; Marco Clemencic; K. Ciba; E. Lanciotti; Iurii Raniuk; P. Henrard; G. Raven; C. Langenbruch; V. Fave; Andrew Cook; G. D. Patel; Miriam Gandelman; S. Belogurov; Harry Cliff; Sandra Amato; David Websdale; F. Dupertuis; O. Kochebina; V. A. Kudryavtsev; Neville Harnew; E. Ben-Haim; Olaf Steinkamp; Oleg Yushchenko; Haonan Lu; Chung Nguyen-Mau; A. Camboni; Oliver Grünberg; Ilya Komarov; J. A. Hernando Morata; Roberta Santacesaria; Carla Göbel; Francesca Dordei; Daniel Charles Craik; J. J. Saborido Silva; D. A. Milanes; S. Schleich; A. Sparkes; Rolf Lindner; Vitaly Vorobyev; T. M. Karbach; A. Dosil Suárez; Hamish Gordon; M. Whitehead; Giampiero Mancinelli; L. A. Granado Cardoso; Biagio Saitta; Mehul Patel; A. N. Solomin; D. Gascon; D. Voong; X. Cid Vidal; Lain-Jong Li; Thierry Gys; R. Muresan; E. Teodorescu; Tjeerd Ketel; T. Pilař; Guy Wilkinson; Thomas Ruf; V. Obraztsov; Vincenzo Vagnoni; B. Gui; J. Mylroie-Smith; Oleg Maev; Oleg Maev; M. Calvi; A. Martens; Paolo Gandini; Pierluigi Campana; Raymond Mountain; A. Mac Raighne; Konstantin Belous; Mikhail Shapkin; A. A. Alves; D. Elsby; G. D. Lafferty; D. van Eijk; C. Hadjivasiliou;arXiv: http://arxiv.org/abs/1206.5160 , 1206.5160
The charged-particle production ratios $\bar{p}/p$, $K^-/K^+$, $��^-/��^+$, $(p + \bar{p})/(��^+ + ��^-)$, $(K^+ + K^-)/(��^+ + ��^-)$ and $(p + \bar{p})/(K^+ + K^-)$ are measured with the LHCb detector using $0.3 {\rm nb^{-1}}$ of $pp$ collisions delivered by the LHC at $\sqrt{s} = 0.9$ TeV and $1.8 {\rm nb^{-1}}$ at $\sqrt{s} = 7$ TeV. The measurements are performed as a function of transverse momentum $p_{\rm T}$ and pseudorapidity $��$. The production ratios are compared to the predictions of several Monte Carlo generator settings, none of which are able to describe adequately all observables. The ratio $\bar{p}/p$ is also considered as a function of rapidity loss, $��y \equiv y_{\rm beam} - y$, and is used to constrain models of baryon transport. Incorrect entries in Table 2 corrected. No consequences for rest of paper
CORE arrow_drop_down COREArticle . 2012License: CC BYFull-Text: https://eprints.gla.ac.uk/80224/1/80224.pdfData sources: COREWarwick Research Archives Portal RepositoryArticle . 2012License: CC BY NDData sources: CORE (RIOXX-UK Aggregator)EnlightenArticle . 2012License: CC BYFull-Text: http://eprints.gla.ac.uk/80224/1/80224.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2012 . Peer-reviewedData sources: CrossrefEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: DANS (Data Archiving and Networked Services)Recolector de Ciencia Abierta, RECOLECTAArticle . 2012License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2012European Physical Journal C: Particles and FieldsArticle . 2012License: CC BYData sources: Maastricht University | MUMC+ Research InformationSpiral - Imperial College Digital RepositoryArticle . 2012Data sources: Spiral - Imperial College Digital RepositoryEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: Oxford University Research ArchiveINRIA a CCSD electronic archive serverArticle . 2012Data sources: INRIA a CCSD electronic archive serverZurich Open Repository and ArchiveArticle . 2012 . Peer-reviewedData sources: Zurich Open Repository and ArchiveDiposit Digital de la Universitat de BarcelonaArticle . 2012License: CC BYData sources: Diposit Digital de la Universitat de BarcelonaRecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTAArchivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della ricerca- Università di Roma La SapienzaArticle . 2012Data sources: Archivio della ricerca- Università di Roma La SapienzaThe University of Manchester - Institutional RepositoryArticle . 2012Data sources: The University of Manchester - Institutional RepositoryDAU - Arxiu Digital de la URLArticle . 2021License: CC BYData sources: DAU - Arxiu Digital de la URLUniversità degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi della Basilicata: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-012-2168-x&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 31 citations 31 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
visibility 248visibility views 248 download downloads 237 Powered bymore_vert CORE arrow_drop_down COREArticle . 2012License: CC BYFull-Text: https://eprints.gla.ac.uk/80224/1/80224.pdfData sources: COREWarwick Research Archives Portal RepositoryArticle . 2012License: CC BY NDData sources: CORE (RIOXX-UK Aggregator)EnlightenArticle . 2012License: CC BYFull-Text: http://eprints.gla.ac.uk/80224/1/80224.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2012 . Peer-reviewedData sources: CrossrefEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: DANS (Data Archiving and Networked Services)Recolector de Ciencia Abierta, RECOLECTAArticle . 2012License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2012European Physical Journal C: Particles and FieldsArticle . 2012License: CC BYData sources: Maastricht University | MUMC+ Research InformationSpiral - Imperial College Digital RepositoryArticle . 2012Data sources: Spiral - Imperial College Digital RepositoryEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: Oxford University Research ArchiveINRIA a CCSD electronic archive serverArticle . 2012Data sources: INRIA a CCSD electronic archive serverZurich Open Repository and ArchiveArticle . 2012 . Peer-reviewedData sources: Zurich Open Repository and ArchiveDiposit Digital de la Universitat de BarcelonaArticle . 2012License: CC BYData sources: Diposit Digital de la Universitat de BarcelonaRecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTAArchivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della ricerca- Università di Roma La SapienzaArticle . 2012Data sources: Archivio della ricerca- Università di Roma La SapienzaThe University of Manchester - Institutional RepositoryArticle . 2012Data sources: The University of Manchester - Institutional RepositoryDAU - Arxiu Digital de la URLArticle . 2021License: CC BYData sources: DAU - Arxiu Digital de la URLUniversità degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi della Basilicata: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-012-2168-x&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2024Embargo end date: 01 Jan 2024 France, SwitzerlandPublisher:California Digital Library (CDL) Funded by:EC | TRIATLASEC| TRIATLASArtana, Camila; Capitani, Leonardo; Santos Garcia, Gabriel; Angelini, Ronaldo; Coll, Marta;pmid: 38790092
1. Marine Heat Waves (MHWs) are episodes of anomalous warming in the ocean that can last from a few days to months. MHWs have different characteristics in terms of intensity, duration, and frequency and generate thermal stress on marine ecosystems. In reef ecosystems, they are one of the main causes of decreased presence and abundance of corals, invertebrates, and fish. The deleterious capacity of thermal stress often depends upon biotic factors such as resource availability (bottom-up control on predators) and predation (top-down control on prey). Despite the evidence of thermal stress and biotic factors affecting individual species, the combined effects of both stressors on the entire reef ecosystems are far less studied. 2. Here, using a food-web modeling approach, we estimated the rate of change in species’ biomass due to different MHW scenarios based on their physical characteristics. Specifically, we modeled the mechanistic link between species’ consumption rate and seawater temperature (thermal stressor), simulating species’ biomass dynamics for different MHW scenarios under different trophic control assumptions (biotic factor). 3. We find that total reef ecosystem biomass declined by 10% ± 5% under MHWs with severe intensity and top-down control assumption. The bottom-up control assumption moderates the total ecosystem biomass reduction by 5% ± 5%. Irrespective of the MHW scenario and the trophic control assumption, the most substantial biomass changes occur among top, meso-predators, and corals (5% to 20% ± 10%).4. Since habitat degradation may lead to reef ecosystems governed by top-down control on prey, our findings point to the critical importance of protecting reef ecosystems as a pivotal strategy to alleviate the impacts of thermal stress induced by MHWs. Overall, our results provide a unified understanding of the interplay between abiotic stressors and biotic factors in reef ecosystems under extreme thermal events, offering insights into present baselines and future ecological states for reef ecosystems.
Journal of Animal Ec... arrow_drop_down École Polytechnique, Université Paris-Saclay: HALArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.32942/x2gk63&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert Journal of Animal Ec... arrow_drop_down École Polytechnique, Université Paris-Saclay: HALArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2017 FrancePublisher:HAL CCSD Authors: Vimeux, Françoise;Reconstruire les variations passées de notre climat permet de mieux appréhender le fonctionnement de notre système climatique.Les carottes de glace issues des calottes polaires et des glaciers montagneux de haute altitude sont de très bonnes archivesclimatiques. Les glaciers présents sur les sommets des Andes sud-américaines sont ainsi exploités depuis les années 80. Une dizainede carottages ont été réalisés depuis l’équateur jusqu’en Patagonie. Ils recouvrent des périodes très différentes allant du derniersiècle, jusqu’à la dernière transition glaciaire-interglaciaire qui débute il y a 21 000 ans. La datation de ces carottes combine unensemble de méthodes : comptage des cycles saisonniers des éléments chimiques et de la composition isotopique de la glace, analysede la concentration des éléments radioactifs issus des tests atmosphériques nucléaires au XXe siècle et modélisation de l’écoulementdu glacier pour la partie la plus profonde. Le présent article illustre deux résultats intéressants apportés par l’étude de la compositionisotopique de ces glaces. Le premier concerne la période du Petit Âge Glaciaire au XVIIe-XVIIIe siècle. L’analyse isotopique de la glacede deux carottes prélevées en Bolivie (Illimani) et au Pérou (Quelccaya), couplée à l’étude de l’extension des glaciers au mêmemoment, montre des conditions climatiques légèrement plus humides et plus froides de 1650 à 1780. Le second résultat est déduitde l’analyse isotopique d’une carotte prélevée en Patagonie du Nord (San Valentin) qui recouvre les 120 dernières années. L’enregistrementisotopique suggère que la température dans cette région a progressivement diminué au cours de cette période d’environ0,2 °C par décennie, venant prolonger une tendance mesurée par les stations météorologiques chiliennes depuis les années 70 malgréun contexte de réchauffement global. The reconstruction of past climate variability offers important information about our climate system. Ice cores extractedfrom polar ice sheets or from mountainous glaciers are among the most popular climate archives. Ice cores from Andean glaciersin South America have been studied since the 1980’s. Almost ten ice cores have been extracted from the equator to Patagonia. Theycover different time periods from the last century to the last glacial-interglacial termination that started 21,000 years ago. Those icecores are usually dated by using a combination of methods: annual layers counting in both isotopic and chemical ice composition,radionuclides concentration analysis to detect atmospheric nuclear tests during the 20th century and ice flow modeling for the deepestpart of those cores. This paper presents two interesting results arising from the isotopic composition of the ice. The first one dealswith the isotopic records of Bolivian (Illimani) and Peruvian (Quelccaya) ice cores in regards to the reconstruction of glacier extentduring the little ice age in the 17th-18th century. Both approaches suggest a slightly moister and cooler period from 1650 to 1780. Thesecond result arises from the 120-year long isotopic record of an ice core drilled in Patagonia (San Valentin). It suggests that at theregional scale, temperature has regularly decreased of about 0.2 °C per decade, extending the temperature decrease shown by Chileanmeteorological data since the 1970’s despite a global warming.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2014 NetherlandsPublisher:Elsevier BV Isabelle Sioen; Gabriele Eiben; Lauren Lissner; Silvia Bel-Serrat; Karin Bammann; Karin Bammann; Inge Huybrechts; Inge Huybrechts; M. Rayson; M.I. Mesana; Theodora Mouratidou; K.R. Westerterp; Iris Pigeot; L. A. Moreno; S. De Henauw; S. De Henauw; Claudia Börnhorst; Vittorio Krogh; V. Pala; C. Ottavaere;pmid: 23622780
Little is known about the validity of repeated 24-h dietary recalls (24-HDR) as a measure of total energy intake (EI) in young children. This study aimed to evaluate the validity of proxy-reported EI by comparison with total energy expenditure (TEE) measured by the doubly labeled water (DLW) technique.The agreement between EI and TEE was investigated in 36 (47.2% boys) children aged 4-10 years from Belgium and Spain using subgroup analyses and Bland-Altman plots. Low-energy-reporters (LER), adequate-energy-reporters (AER) and high-energy-reporters (HER) were defined from the ratio of EI over TEE by application of age- and sex-specific cut-off values.There was good agreement between means of EI (1500 kcal/day) and TEE (1523 kcal/day) at group level though in single children, i.e. at the individual level, large differences were observed. Almost perfect agreement between EI and TEE was observed in thin/normal weight children (EI: 1511 kcal/day; TEE: 1513 kcal/day). Even in overweight/obese children the mean difference between EI and TEE was only -86 kcal/day. Among the participants, 28 (78%) were classified as AER, five (14%) as HER and three (8%) as LER.Two proxy-reported 24-HDRs were found to be a valid instrument to assess EI on group level but not on the individual level.
Clinical Nutrition arrow_drop_down Clinical NutritionArticle . 2014License: taverneData sources: Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routeshybrid 57 citations 57 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Clinical Nutrition arrow_drop_down Clinical NutritionArticle . 2014License: taverneData sources: Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Doctoral thesis 2015 FrancePublisher:HAL CCSD Authors: Giesen, Gaelle;Les preuves pour l'existence de la matière noire (MN), sous forme d'une particule inconnue qui rempli les halos galactiques, sont issues d'observations astrophysiques et cosmologiques: son effet gravitationnel est visible dans les rotations des galaxies, des amas de galaxies et dans la formation des grandes structures de l'univers. Une manifestation non-gravitationnelle de sa présence n'a pas encore été découverte. L'une des techniques les plus prometteuse est la détection indirecte de la MN, consistant à identifier des excès dans les flux de rayons cosmiques pouvant provenir de l'annihilation ou la désintégration de la MN dans le halo de la Voie Lactée. Les efforts expérimentaux actuels se focalisent principalement sur une gamme d'énergie de l'ordre du GeV au TeV, où un signal de WIMP (Weakly Interacting Massive Particles) est attendu. L'analyse des mesures récentes et inédites des rayons cosmiques chargés (antiprotons, électrons et positrons) et leurs émissions secondaires et les améliorations des modèles astrophysiques sont présentées.Les données de PAMELA sur les antiprotons contraignent l'annihilation et la désintégration de la MN de manière similaire (et même légèrement meilleurs) que les contraintes les plus fortes venant des rayons gamma, même dans le cas où les énergies cinétiques inférieures à 10 GeV sont écartées. En choisissant des paramètres astrophysiques différents (modèles de propagation et profils de MN), les contraintes peuvent changer d'un à deux ordres de grandeur. Pour exploiter la totalité de la capacité des antiprotons à contraindre la MN, des effets précédemment négligés sont incorporés et se révèlent être importants dans l'analyse des données inédites de AMS-02 : ajouter les pertes d'énergie, la diffusion dans l'espace des moments et la modulation solaire peut modifier les contraintes, même à de hautes masses. Une mauvaise interprétation des données peut survenir si ces effets ne sont pas pris en compte. Avec les flux de protons et d'hélium exposé par AMS-02, le fond astrophysique et ces incertitudes du ratio antiprotons sur protons sont réévalués et comparés aux données inédites de AMS-02. Aucune indication pour un excès n'est trouvé. Une préférence pour un halo confinant plus large et une dépendance en énergie du coefficient de diffusion plus plate apparaissent. De nouvelles contraintes sur l'annihilation et la désintégration de la MN sont ainsi dérivés.Les émissions secondaires des électrons et des positrons peuvent aussi contraindre l'annihilation et la désintégration de la MN dans le halo galactique : le signal radio dû à la radiation synchrotron des électrons et positrons dans le champs magnétique galactique, les rayons gamma des processus de bremsstrahlung avec le gas galactique et de Compton Inverse avec le champs radiatif interstellaire sont considérés. Différentes configurations de champs magnétique galactique et de modèles de propagation et des cartes de gas et de champs radiatif interstellaire améliorés sont utilisées pour obtenir des outils permettant le calculs des émissions synchrotrons et bremsstrahlung venant de MN de type WIMP. Tous les résultats numériques sont incorporés dans la dernière version du Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID).Une interprétation d'un possible excès dans les données de rayons gamma de Fermi-LAT au centre galactique comme étant dû à l'annihilation de MN en canaux hadronique et leptonique est analysée. Dans une approche de messagers multiples, le calcul des émissions secondaires est amélioré et se révèle être important pour la détermination du spectre pour le canal leptonique. Ensuite, les limites provenant des antiprotons sur l'annihilation en canal hadronique contraignent sévèrement l'interprétation de cet excès comme étant dû à la MN, dans le cas de paramètres de propagation et de modulation solaire standards. Avec un choix plus conservatif de ces paramètres elles s'assouplissent considérablement. Overwhelming evidence for the existence of Dark Matter (DM), in the form of an unknownparticle filling the galactic halos, originates from many observations in astrophysics and cosmology: its gravitational effects are apparent on galactic rotations, in galaxy clusters and in shaping the large scale structure of the Universe. On the other hand, a non-gravitational manifestation of its presence is yet to be unveiled. One of the most promising techniques is the one of indirect detection, aimed at identifying excesses in cosmic ray fluxes which could possibly be produced by DM annihilations or decays in the Milky Way halo. The current experimental efforts mainly focus in the GeV to TeV energy range, which is also where signals from WIMPs (Weakly Interacting Massive Particles) are expected. Focussing on charged cosmic rays, in particular antiprotons, electrons and positrons, as well as their secondary emissions, an analysis of current and forseen cosmic ray measurements and improvements on astrophysical models are presented. Antiproton data from PAMELA imposes contraints on annihilating and decaying DM which are similar to (or even slightly stronger than) the most stringent bounds from gamma ray experiments, even when kinetic energies below 10 GeV are discarded. However, choosing different sets of astrophysical parameters, in the form of propagation models and halo profiles, allows the contraints to span over one or two orders of magnitude. In order to exploit fully the power of antiprotons to constrain or discover DM, effects which were previously perceived as subleading turn out to be relevant especially for the analysis of the newly released AMS-02 data. In fact, including energy losses, diffusive reaccelleration and solar modulation can somewhat modify the current bounds, even at large DM masses. A wrong interpretation of the data may arise if they are not taken into account. Finally, using the updated proton and helium fluxes just released by the AMS-02 experiment, the astrophysical antiproton to proton ratio and its uncertainties are reevaluated and compared to the preliminarly reported AMS-02 measurements. No unambiguous evidence for a significant excess with respect to expectations is found. Yet, some preference for thicker halos and a flatter energy dependence of the diffusion coefficient starts to emerge. New stringed constraints on DM annihilation and decay are derived. Secondary emissions from electrons and positrons can also be used to constrain DM annihilation or decay in the galactic halo. The radio signal due to synchrotron radiation of electrons and positrons on the galactic magnetic field, gamma rays from bremsstrahlung processes on the galactic gas densities and from Inverse Compton scattering processes on the interstellar radiation field are considered. With several magnetic field configurations, propagation scenarios and improved gas density maps and interstellar radiation field, state-of-art tools allowing the computaion of synchrotron and bremssttrahlung radiation for any WIMP DM model are provided. All numerical results for DM are incorporated in the release of the Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID). Finally, the possible GeV gamma-ray excess identified in the Fermi-LAT data from the Galactic Center in terms of DM annihilation, either in hadronic or leptonic channels is studied. In order to test this tantalizing interprestation, a multi-messenger approach is used: first, the computation of secondary emisison from DM with respect to previous works confirms it to be relevant for determining the DM spectrum in leptonic channels. Second, limits from antiprotons severely constrain the DM interpretation of the excess in the hadronic channel, for standard assumptions on the Galactic propagation parameters and solar modulation. However, they considerably relax if more conservative choices are adopted.
Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverDoctoral thesis . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationDoctoral thesis . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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more_vert Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverDoctoral thesis . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationDoctoral thesis . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article 2010Publisher:IEEE Camara, M.B.; Gualous, H.; Dakyo, B.; Nichita, C.; Makany, P.;This paper presents a careful study related to a more efficient energy management between lithium battery (with rated voltage of 24V) and Ultracapacitors (UC) for Hybrid Electric Vehicle (HEV) applications. This association is due to the present trend in the field, knowing that the major drawback of the HEV is the autonomy problem. Thus, using the Hybrid energy source (such as UC + battery) and with a good energy management improves the HEV performances. In this paper, battery and Ultracapacitors (10 cells of 2.7V in series) are coupled to DC-bus using two buck-boost converters. The main contribution of this paper is focused on DC-bus voltage and currents control strategy based on polynomial (RST) controller. Through some simulations in MATLAB/Simulink software and experimental results, the authors present an improved energy management for HEV.
Hyper Article en Lig... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYMémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/vppc.2010.5729140&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 10 citations 10 popularity Top 10% influence Top 10% impulse Average Powered by BIP!
more_vert Hyper Article en Lig... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYMémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/vppc.2010.5729140&type=result"></script>'); --> </script>
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description Publicationkeyboard_double_arrow_right Article , Other literature type 2021Publisher:Springer Science and Business Media LLC Lucy Allington; Carla Cannone; Ioannis Pappis; Karla Cervantes Barron; Will Usher; Steve Pye; Edward Brown; Mark Howells; Constantinos Taliotis; Caroline Sundin; Vignesh Sridha; Eunice Ramos; Maarten Brinkerink; Paul Deane; Andrii Gritsevskyi; Gustavo Moura; Arnaud Rouget; David Wogan; Edito Barcelona; Holger Rogner; Stephanie Hirmer;Abstract Energy system modelling can be used to assess the implications of different scenarios and support improved policymaking. However, access to data is often a barrier to starting energy system modelling in developing countries, thereby causing delays. This article therefore provides data that can be used to create a simple zero order energy system model for Mauritania, which can act as a starting point for further model development and scenario analysis. The data are collected entirely from publicly available and accessible sources, including the websites and databases of international organizations, journal articles, and existing modelling studies. This means that the dataset can be easily updated based on the latest available information or more detailed and accurate local data. These data were also used to calibrate a simple energy system model using the Open Source Energy Modelling System (OSeMOSYS) and two stylized scenarios (Fossil Future and Least Cost ) for 2020-2050. The assumptions used and results of these scenarios are presented in the appendix as an illustrative example of what can be done with these data. This simple model can be adapted and further developed by in-country analysts and academics, providing a platform for future work.
https://doi.org/10.2... arrow_drop_down https://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefhttps://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert https://doi.org/10.2... arrow_drop_down https://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefhttps://doi.org/10.21203/rs.3....Article . 2021 . Peer-reviewedLicense: CC BYData sources: Crossrefadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.21203/rs.3.rs-479591/v2&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2024Publisher:Springer Science and Business Media LLC Amel Kasri; Kamel Ouari; Youcef Belkhier; Mohit Bajaj; Ievgen Zaitsev;AbstractEnhancing the efficiency of the electric vehicle’s powertrain becomes a crucial focus, wherein the control system for the traction motor plays a significant role. This paper presents a novel electric vehicle traction motor control system based on a robust predictive direct torque control approach, an improved version of the conventional DTC, where the traditional switching table and the hysteresis regulators are substituted with a predictive block based on an optimization algorithm. Additionally, a robust predictive speed loop regulator is employed instead of the proportional-integral regulator, which integrates a new cost function with a finite horizon, incorporating integral action into the control law based on a Taylor series expansion. This technique’s primary benefit is its independence from the necessity to measure and observe external disturbances, as well as uncertainties related to parameters. The effectiveness of the suggested system was confirmed through simulation and experimental results under the OPAL-RT platform. The findings indicate that the proposed approach outperforms the conventional method in terms of rejecting disturbances, exhibiting robustness to variations in parameters, and minimizing torque ripple.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1038/s41598-024-65988-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 6 citations 6 popularity Average influence Average impulse Top 10% Powered by BIP!
more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1038/s41598-024-65988-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2014 FrancePublisher:Springer Science and Business Media LLC Authors: Arnoult, Stéphanie; Brancourt-Hulmel, Maryse;The lignocellulosic C4 perennial crop miscanthus and, more particularly, one of its species, Miscanthus × giganteus, are especially interesting for bioenergy production because they combine high biomass production with a low environmental impact. However, few varieties are available, which is risky due to disease susceptibility. Gathering worldwide references, this review shows a high genotypic and environmental variability for traits of interest related to miscanthus biomass production and composition, which may be useful in breeding programs for enhancing the availability of suitable clones for bioenergy production. The M. × giganteus species and certain clones in the Miscanthus sinensis species seem particularly interesting due to high biomass production per hectare. Although the industrial requirements for biomass composition have not been fully defined for the different bioenergy conversion processes, the M. × giganteus and Miscanthus sacchariflorus species, which show high lignin contents, appear more suitable for thermochemical conversion processes. In contrast, the M. sinensis species and certain M. × giganteus clones with low lignin contents were interesting for biochemical conversion processes. The M. sacchariflorus species is also interesting as a progenitor for breeding programs, due to its low ash content, which is suitable for the different bioenergy conversion processes. Moreover, mature miscanthus crops harvested in winter seem preferred by industry to enhance efficiency and reduce the expense of the processes. This investigation on miscanthus can be extrapolated to other monocotyledons and perennial crops, which may be proposed as feedstocks in addition to miscanthus.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1007/s12155-014-9524-7&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routeshybrid 82 citations 82 popularity Top 1% influence Top 10% impulse Top 10% Powered by BIP!
more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article 2015 FrancePublisher:IEEE Authors: Cany, Camille; Mansilla, Christine; Mathonnière, Gilles; da Costa, Pascal;n the French context of increasing renewable penetration and significant nuclear power, the optimal contribution of this energy source is discussed from two viewpoints. On the one hand, from the social planner viewpoint, the nuclear optimum contribution is the one that minimizes the overall electric price, whatever the resulting load factor. The use of screening curves, often implemented to design the optimal power mix is questioned, being highly sensitive to the assumptions. On the other hand, from the plant operator viewpoint, the nuclear power plants need to amortize the capital expenses, hence achieve the longest operating time. With a view to make the two viewpoints meet, we propose to operate nuclear power plants as baseloads and consider modulation through the power use, i.e. supply electricity to the electric system when requested and use the remaining power to produce other valuable products, such as heat or hydrogen.
Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverConference object . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationConference object . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/eem.2015.7216627&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverConference object . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationConference object . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/eem.2015.7216627&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint , Journal 2012Embargo end date: 01 Jan 2012 Italy, France, Spain, Italy, France, Italy, France, Italy, Netherlands, United Kingdom, Spain, Italy, Italy, Italy, Spain, United Kingdom, Italy, Switzerland, Spain, France, United Kingdom, United Kingdom, United Kingdom, France, France, Italy, Spain, Netherlands, France, France, France, Italy, Netherlands, FrancePublisher:Springer Science and Business Media LLC Publicly fundedFunded by:SNSF | Search for New Physics in..., SNSF | High Precision CP Violati..., SNSF | Particle Physics in the L...SNSF| Search for New Physics in Electroweak Penguin Transitions at LHCb ,SNSF| High Precision CP Violation Physics at LHCb ,SNSF| Particle Physics in the LHC EraAlexey Novoselov; J. Magnin; V. N. La Thi; Naylya Sagidova; Antonio Falabella; Albert Bursche; M. Matveev; Evelina Gersabeck; V. Tisserand; Maximilian Schlupp; C. Potterat; Cristina Lazzeroni; U. Kerzel; Marie Helene Schune; B. Schmidt; C. J. Parkinson; B. Sciascia; F. Xing; G. N. Patrick; Massimiliano Ferro-Luzzi; R. Vazquez Gomez; P. M. Bjørnstad; O. Francisco; J. Dickens; B. Pietrzyk; Jessica Prisciandaro; J. Buytaert; Nazim Hussain; Marcin Kucharczyk; Marcin Kucharczyk; Marcin Kucharczyk; T. E. Latham; I. R. Kenyon; H. Ruiz; D. Souza; F. Eisele; Th. S. Bauer; E. van Herwijnen; A. Bates; N. A. Smith; R. Silva Coutinho; Marc-Olivier Bettler; Alessia Satta; J. Anderson; Leonid Kravchuk; C. D'Ambrosio; D. Savrina; J. Panman; Manuel Schiller; Z. Mathe; Alexey Zhelezov; E. Grauges; Timothy Gershon; Timothy Gershon; S. C. Haines; David Ward; A. Puig Navarro; D. Wiedner; T. Huse; K. Hennessy; P. Rodriguez Perez; Andrey Vorobyev; Po-Hsun Chen; Po-Hsun Chen; Evgeny Gushchin; Jack Benton; Sebastian Bachmann; R. S. Huston; H. Dijkstra; A. D. Nguyen; Gregory Ciezarek; N. Chiapolini; A. Borgia; Adriano Lai; S. Eidelman; Ronan McNulty; Daniel Lacarrere; J. Rouvinet; Krzysztof Grzegorz Sobczak; Minh Tâm Tran; A. D. Webber; T. Lesiak; Y.Y. Li; Mikhail Zavertyaev; Ph. Charpentier; Ronan Wallace; Giulia Manca; Marcin Chrzaszcz; P. Diniz Batista; Dmitry Popov; C. Voß; V. V. Gligorov; Ivan Belyaev; Andrey Golutvin; Andrey Golutvin; Andrey Golutvin; W. Witzeling; Alessandro Petrolini; J. van Tilburg; Thomas Blake; A. Nomerotski; A. Nomerotski; R. Lefèvre; V.G. Shevchenko; Jing Wang; Robert Currie; S. Roiser; Rustem Dzhelyadin; Edwige Tournefier; Edwige Tournefier; K. De Bruyn; A. Gomes; Giacomo Graziani; A. Richards; Marc S. Williams; Patrick Owen; A. Palano; Piotr Morawski; J. P. Lees; P. Shatalov; T. Brambach; M. Seco; Nikolay Bondar; Marco Clemencic; K. Ciba; E. Lanciotti; Iurii Raniuk; P. Henrard; G. Raven; C. Langenbruch; V. Fave; Andrew Cook; G. D. Patel; Miriam Gandelman; S. Belogurov; Harry Cliff; Sandra Amato; David Websdale; F. Dupertuis; O. Kochebina; V. A. Kudryavtsev; Neville Harnew; E. Ben-Haim; Olaf Steinkamp; Oleg Yushchenko; Haonan Lu; Chung Nguyen-Mau; A. Camboni; Oliver Grünberg; Ilya Komarov; J. A. Hernando Morata; Roberta Santacesaria; Carla Göbel; Francesca Dordei; Daniel Charles Craik; J. J. Saborido Silva; D. A. Milanes; S. Schleich; A. Sparkes; Rolf Lindner; Vitaly Vorobyev; T. M. Karbach; A. Dosil Suárez; Hamish Gordon; M. Whitehead; Giampiero Mancinelli; L. A. Granado Cardoso; Biagio Saitta; Mehul Patel; A. N. Solomin; D. Gascon; D. Voong; X. Cid Vidal; Lain-Jong Li; Thierry Gys; R. Muresan; E. Teodorescu; Tjeerd Ketel; T. Pilař; Guy Wilkinson; Thomas Ruf; V. Obraztsov; Vincenzo Vagnoni; B. Gui; J. Mylroie-Smith; Oleg Maev; Oleg Maev; M. Calvi; A. Martens; Paolo Gandini; Pierluigi Campana; Raymond Mountain; A. Mac Raighne; Konstantin Belous; Mikhail Shapkin; A. A. Alves; D. Elsby; G. D. Lafferty; D. van Eijk; C. Hadjivasiliou;arXiv: http://arxiv.org/abs/1206.5160 , 1206.5160
The charged-particle production ratios $\bar{p}/p$, $K^-/K^+$, $��^-/��^+$, $(p + \bar{p})/(��^+ + ��^-)$, $(K^+ + K^-)/(��^+ + ��^-)$ and $(p + \bar{p})/(K^+ + K^-)$ are measured with the LHCb detector using $0.3 {\rm nb^{-1}}$ of $pp$ collisions delivered by the LHC at $\sqrt{s} = 0.9$ TeV and $1.8 {\rm nb^{-1}}$ at $\sqrt{s} = 7$ TeV. The measurements are performed as a function of transverse momentum $p_{\rm T}$ and pseudorapidity $��$. The production ratios are compared to the predictions of several Monte Carlo generator settings, none of which are able to describe adequately all observables. The ratio $\bar{p}/p$ is also considered as a function of rapidity loss, $��y \equiv y_{\rm beam} - y$, and is used to constrain models of baryon transport. Incorrect entries in Table 2 corrected. No consequences for rest of paper
CORE arrow_drop_down COREArticle . 2012License: CC BYFull-Text: https://eprints.gla.ac.uk/80224/1/80224.pdfData sources: COREWarwick Research Archives Portal RepositoryArticle . 2012License: CC BY NDData sources: CORE (RIOXX-UK Aggregator)EnlightenArticle . 2012License: CC BYFull-Text: http://eprints.gla.ac.uk/80224/1/80224.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2012 . Peer-reviewedData sources: CrossrefEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: DANS (Data Archiving and Networked Services)Recolector de Ciencia Abierta, RECOLECTAArticle . 2012License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2012European Physical Journal C: Particles and FieldsArticle . 2012License: CC BYData sources: Maastricht University | MUMC+ Research InformationSpiral - Imperial College Digital RepositoryArticle . 2012Data sources: Spiral - Imperial College Digital RepositoryEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: Oxford University Research ArchiveINRIA a CCSD electronic archive serverArticle . 2012Data sources: INRIA a CCSD electronic archive serverZurich Open Repository and ArchiveArticle . 2012 . Peer-reviewedData sources: Zurich Open Repository and ArchiveDiposit Digital de la Universitat de BarcelonaArticle . 2012License: CC BYData sources: Diposit Digital de la Universitat de BarcelonaRecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTAArchivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della ricerca- Università di Roma La SapienzaArticle . 2012Data sources: Archivio della ricerca- Università di Roma La SapienzaThe University of Manchester - Institutional RepositoryArticle . 2012Data sources: The University of Manchester - Institutional RepositoryDAU - Arxiu Digital de la URLArticle . 2021License: CC BYData sources: DAU - Arxiu Digital de la URLUniversità degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi della Basilicata: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1140/epjc/s10052-012-2168-x&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 31 citations 31 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
visibility 248visibility views 248 download downloads 237 Powered bymore_vert CORE arrow_drop_down COREArticle . 2012License: CC BYFull-Text: https://eprints.gla.ac.uk/80224/1/80224.pdfData sources: COREWarwick Research Archives Portal RepositoryArticle . 2012License: CC BY NDData sources: CORE (RIOXX-UK Aggregator)EnlightenArticle . 2012License: CC BYFull-Text: http://eprints.gla.ac.uk/80224/1/80224.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2012 . Peer-reviewedData sources: CrossrefEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: DANS (Data Archiving and Networked Services)Recolector de Ciencia Abierta, RECOLECTAArticle . 2012License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAEuropean Physical Journal C: Particles and FieldsArticle . 2012European Physical Journal C: Particles and FieldsArticle . 2012License: CC BYData sources: Maastricht University | MUMC+ Research InformationSpiral - Imperial College Digital RepositoryArticle . 2012Data sources: Spiral - Imperial College Digital RepositoryEuropean Physical Journal C: Particles and FieldsArticle . 2012Data sources: Oxford University Research ArchiveINRIA a CCSD electronic archive serverArticle . 2012Data sources: INRIA a CCSD electronic archive serverZurich Open Repository and ArchiveArticle . 2012 . Peer-reviewedData sources: Zurich Open Repository and ArchiveDiposit Digital de la Universitat de BarcelonaArticle . 2012License: CC BYData sources: Diposit Digital de la Universitat de BarcelonaRecolector de Ciencia Abierta, RECOLECTAArticle . 2012Data sources: Recolector de Ciencia Abierta, RECOLECTAArchivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della ricerca- Università di Roma La SapienzaArticle . 2012Data sources: Archivio della ricerca- Università di Roma La SapienzaThe University of Manchester - Institutional RepositoryArticle . 2012Data sources: The University of Manchester - Institutional RepositoryDAU - Arxiu Digital de la URLArticle . 2021License: CC BYData sources: DAU - Arxiu Digital de la URLUniversità degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Università degli Studi della Basilicata: CINECA IRISArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di Roma Tor vergataArticle . 2012Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2024Embargo end date: 01 Jan 2024 France, SwitzerlandPublisher:California Digital Library (CDL) Funded by:EC | TRIATLASEC| TRIATLASArtana, Camila; Capitani, Leonardo; Santos Garcia, Gabriel; Angelini, Ronaldo; Coll, Marta;pmid: 38790092
1. Marine Heat Waves (MHWs) are episodes of anomalous warming in the ocean that can last from a few days to months. MHWs have different characteristics in terms of intensity, duration, and frequency and generate thermal stress on marine ecosystems. In reef ecosystems, they are one of the main causes of decreased presence and abundance of corals, invertebrates, and fish. The deleterious capacity of thermal stress often depends upon biotic factors such as resource availability (bottom-up control on predators) and predation (top-down control on prey). Despite the evidence of thermal stress and biotic factors affecting individual species, the combined effects of both stressors on the entire reef ecosystems are far less studied. 2. Here, using a food-web modeling approach, we estimated the rate of change in species’ biomass due to different MHW scenarios based on their physical characteristics. Specifically, we modeled the mechanistic link between species’ consumption rate and seawater temperature (thermal stressor), simulating species’ biomass dynamics for different MHW scenarios under different trophic control assumptions (biotic factor). 3. We find that total reef ecosystem biomass declined by 10% ± 5% under MHWs with severe intensity and top-down control assumption. The bottom-up control assumption moderates the total ecosystem biomass reduction by 5% ± 5%. Irrespective of the MHW scenario and the trophic control assumption, the most substantial biomass changes occur among top, meso-predators, and corals (5% to 20% ± 10%).4. Since habitat degradation may lead to reef ecosystems governed by top-down control on prey, our findings point to the critical importance of protecting reef ecosystems as a pivotal strategy to alleviate the impacts of thermal stress induced by MHWs. Overall, our results provide a unified understanding of the interplay between abiotic stressors and biotic factors in reef ecosystems under extreme thermal events, offering insights into present baselines and future ecological states for reef ecosystems.
Journal of Animal Ec... arrow_drop_down École Polytechnique, Université Paris-Saclay: HALArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.32942/x2gk63&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert Journal of Animal Ec... arrow_drop_down École Polytechnique, Université Paris-Saclay: HALArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQArticle . 2024License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.32942/x2gk63&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2017 FrancePublisher:HAL CCSD Authors: Vimeux, Françoise;Reconstruire les variations passées de notre climat permet de mieux appréhender le fonctionnement de notre système climatique.Les carottes de glace issues des calottes polaires et des glaciers montagneux de haute altitude sont de très bonnes archivesclimatiques. Les glaciers présents sur les sommets des Andes sud-américaines sont ainsi exploités depuis les années 80. Une dizainede carottages ont été réalisés depuis l’équateur jusqu’en Patagonie. Ils recouvrent des périodes très différentes allant du derniersiècle, jusqu’à la dernière transition glaciaire-interglaciaire qui débute il y a 21 000 ans. La datation de ces carottes combine unensemble de méthodes : comptage des cycles saisonniers des éléments chimiques et de la composition isotopique de la glace, analysede la concentration des éléments radioactifs issus des tests atmosphériques nucléaires au XXe siècle et modélisation de l’écoulementdu glacier pour la partie la plus profonde. Le présent article illustre deux résultats intéressants apportés par l’étude de la compositionisotopique de ces glaces. Le premier concerne la période du Petit Âge Glaciaire au XVIIe-XVIIIe siècle. L’analyse isotopique de la glacede deux carottes prélevées en Bolivie (Illimani) et au Pérou (Quelccaya), couplée à l’étude de l’extension des glaciers au mêmemoment, montre des conditions climatiques légèrement plus humides et plus froides de 1650 à 1780. Le second résultat est déduitde l’analyse isotopique d’une carotte prélevée en Patagonie du Nord (San Valentin) qui recouvre les 120 dernières années. L’enregistrementisotopique suggère que la température dans cette région a progressivement diminué au cours de cette période d’environ0,2 °C par décennie, venant prolonger une tendance mesurée par les stations météorologiques chiliennes depuis les années 70 malgréun contexte de réchauffement global. The reconstruction of past climate variability offers important information about our climate system. Ice cores extractedfrom polar ice sheets or from mountainous glaciers are among the most popular climate archives. Ice cores from Andean glaciersin South America have been studied since the 1980’s. Almost ten ice cores have been extracted from the equator to Patagonia. Theycover different time periods from the last century to the last glacial-interglacial termination that started 21,000 years ago. Those icecores are usually dated by using a combination of methods: annual layers counting in both isotopic and chemical ice composition,radionuclides concentration analysis to detect atmospheric nuclear tests during the 20th century and ice flow modeling for the deepestpart of those cores. This paper presents two interesting results arising from the isotopic composition of the ice. The first one dealswith the isotopic records of Bolivian (Illimani) and Peruvian (Quelccaya) ice cores in regards to the reconstruction of glacier extentduring the little ice age in the 17th-18th century. Both approaches suggest a slightly moister and cooler period from 1650 to 1780. Thesecond result arises from the 120-year long isotopic record of an ice core drilled in Patagonia (San Valentin). It suggests that at theregional scale, temperature has regularly decreased of about 0.2 °C per decade, extending the temperature decrease shown by Chileanmeteorological data since the 1970’s despite a global warming.
Hyper Article en Lig... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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more_vert Hyper Article en Lig... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2014 NetherlandsPublisher:Elsevier BV Isabelle Sioen; Gabriele Eiben; Lauren Lissner; Silvia Bel-Serrat; Karin Bammann; Karin Bammann; Inge Huybrechts; Inge Huybrechts; M. Rayson; M.I. Mesana; Theodora Mouratidou; K.R. Westerterp; Iris Pigeot; L. A. Moreno; S. De Henauw; S. De Henauw; Claudia Börnhorst; Vittorio Krogh; V. Pala; C. Ottavaere;pmid: 23622780
Little is known about the validity of repeated 24-h dietary recalls (24-HDR) as a measure of total energy intake (EI) in young children. This study aimed to evaluate the validity of proxy-reported EI by comparison with total energy expenditure (TEE) measured by the doubly labeled water (DLW) technique.The agreement between EI and TEE was investigated in 36 (47.2% boys) children aged 4-10 years from Belgium and Spain using subgroup analyses and Bland-Altman plots. Low-energy-reporters (LER), adequate-energy-reporters (AER) and high-energy-reporters (HER) were defined from the ratio of EI over TEE by application of age- and sex-specific cut-off values.There was good agreement between means of EI (1500 kcal/day) and TEE (1523 kcal/day) at group level though in single children, i.e. at the individual level, large differences were observed. Almost perfect agreement between EI and TEE was observed in thin/normal weight children (EI: 1511 kcal/day; TEE: 1513 kcal/day). Even in overweight/obese children the mean difference between EI and TEE was only -86 kcal/day. Among the participants, 28 (78%) were classified as AER, five (14%) as HER and three (8%) as LER.Two proxy-reported 24-HDRs were found to be a valid instrument to assess EI on group level but not on the individual level.
Clinical Nutrition arrow_drop_down Clinical NutritionArticle . 2014License: taverneData sources: Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routeshybrid 57 citations 57 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Clinical Nutrition arrow_drop_down Clinical NutritionArticle . 2014License: taverneData sources: Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Doctoral thesis 2015 FrancePublisher:HAL CCSD Authors: Giesen, Gaelle;Les preuves pour l'existence de la matière noire (MN), sous forme d'une particule inconnue qui rempli les halos galactiques, sont issues d'observations astrophysiques et cosmologiques: son effet gravitationnel est visible dans les rotations des galaxies, des amas de galaxies et dans la formation des grandes structures de l'univers. Une manifestation non-gravitationnelle de sa présence n'a pas encore été découverte. L'une des techniques les plus prometteuse est la détection indirecte de la MN, consistant à identifier des excès dans les flux de rayons cosmiques pouvant provenir de l'annihilation ou la désintégration de la MN dans le halo de la Voie Lactée. Les efforts expérimentaux actuels se focalisent principalement sur une gamme d'énergie de l'ordre du GeV au TeV, où un signal de WIMP (Weakly Interacting Massive Particles) est attendu. L'analyse des mesures récentes et inédites des rayons cosmiques chargés (antiprotons, électrons et positrons) et leurs émissions secondaires et les améliorations des modèles astrophysiques sont présentées.Les données de PAMELA sur les antiprotons contraignent l'annihilation et la désintégration de la MN de manière similaire (et même légèrement meilleurs) que les contraintes les plus fortes venant des rayons gamma, même dans le cas où les énergies cinétiques inférieures à 10 GeV sont écartées. En choisissant des paramètres astrophysiques différents (modèles de propagation et profils de MN), les contraintes peuvent changer d'un à deux ordres de grandeur. Pour exploiter la totalité de la capacité des antiprotons à contraindre la MN, des effets précédemment négligés sont incorporés et se révèlent être importants dans l'analyse des données inédites de AMS-02 : ajouter les pertes d'énergie, la diffusion dans l'espace des moments et la modulation solaire peut modifier les contraintes, même à de hautes masses. Une mauvaise interprétation des données peut survenir si ces effets ne sont pas pris en compte. Avec les flux de protons et d'hélium exposé par AMS-02, le fond astrophysique et ces incertitudes du ratio antiprotons sur protons sont réévalués et comparés aux données inédites de AMS-02. Aucune indication pour un excès n'est trouvé. Une préférence pour un halo confinant plus large et une dépendance en énergie du coefficient de diffusion plus plate apparaissent. De nouvelles contraintes sur l'annihilation et la désintégration de la MN sont ainsi dérivés.Les émissions secondaires des électrons et des positrons peuvent aussi contraindre l'annihilation et la désintégration de la MN dans le halo galactique : le signal radio dû à la radiation synchrotron des électrons et positrons dans le champs magnétique galactique, les rayons gamma des processus de bremsstrahlung avec le gas galactique et de Compton Inverse avec le champs radiatif interstellaire sont considérés. Différentes configurations de champs magnétique galactique et de modèles de propagation et des cartes de gas et de champs radiatif interstellaire améliorés sont utilisées pour obtenir des outils permettant le calculs des émissions synchrotrons et bremsstrahlung venant de MN de type WIMP. Tous les résultats numériques sont incorporés dans la dernière version du Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID).Une interprétation d'un possible excès dans les données de rayons gamma de Fermi-LAT au centre galactique comme étant dû à l'annihilation de MN en canaux hadronique et leptonique est analysée. Dans une approche de messagers multiples, le calcul des émissions secondaires est amélioré et se révèle être important pour la détermination du spectre pour le canal leptonique. Ensuite, les limites provenant des antiprotons sur l'annihilation en canal hadronique contraignent sévèrement l'interprétation de cet excès comme étant dû à la MN, dans le cas de paramètres de propagation et de modulation solaire standards. Avec un choix plus conservatif de ces paramètres elles s'assouplissent considérablement. Overwhelming evidence for the existence of Dark Matter (DM), in the form of an unknownparticle filling the galactic halos, originates from many observations in astrophysics and cosmology: its gravitational effects are apparent on galactic rotations, in galaxy clusters and in shaping the large scale structure of the Universe. On the other hand, a non-gravitational manifestation of its presence is yet to be unveiled. One of the most promising techniques is the one of indirect detection, aimed at identifying excesses in cosmic ray fluxes which could possibly be produced by DM annihilations or decays in the Milky Way halo. The current experimental efforts mainly focus in the GeV to TeV energy range, which is also where signals from WIMPs (Weakly Interacting Massive Particles) are expected. Focussing on charged cosmic rays, in particular antiprotons, electrons and positrons, as well as their secondary emissions, an analysis of current and forseen cosmic ray measurements and improvements on astrophysical models are presented. Antiproton data from PAMELA imposes contraints on annihilating and decaying DM which are similar to (or even slightly stronger than) the most stringent bounds from gamma ray experiments, even when kinetic energies below 10 GeV are discarded. However, choosing different sets of astrophysical parameters, in the form of propagation models and halo profiles, allows the contraints to span over one or two orders of magnitude. In order to exploit fully the power of antiprotons to constrain or discover DM, effects which were previously perceived as subleading turn out to be relevant especially for the analysis of the newly released AMS-02 data. In fact, including energy losses, diffusive reaccelleration and solar modulation can somewhat modify the current bounds, even at large DM masses. A wrong interpretation of the data may arise if they are not taken into account. Finally, using the updated proton and helium fluxes just released by the AMS-02 experiment, the astrophysical antiproton to proton ratio and its uncertainties are reevaluated and compared to the preliminarly reported AMS-02 measurements. No unambiguous evidence for a significant excess with respect to expectations is found. Yet, some preference for thicker halos and a flatter energy dependence of the diffusion coefficient starts to emerge. New stringed constraints on DM annihilation and decay are derived. Secondary emissions from electrons and positrons can also be used to constrain DM annihilation or decay in the galactic halo. The radio signal due to synchrotron radiation of electrons and positrons on the galactic magnetic field, gamma rays from bremsstrahlung processes on the galactic gas densities and from Inverse Compton scattering processes on the interstellar radiation field are considered. With several magnetic field configurations, propagation scenarios and improved gas density maps and interstellar radiation field, state-of-art tools allowing the computaion of synchrotron and bremssttrahlung radiation for any WIMP DM model are provided. All numerical results for DM are incorporated in the release of the Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID). Finally, the possible GeV gamma-ray excess identified in the Fermi-LAT data from the Galactic Center in terms of DM annihilation, either in hadronic or leptonic channels is studied. In order to test this tantalizing interprestation, a multi-messenger approach is used: first, the computation of secondary emisison from DM with respect to previous works confirms it to be relevant for determining the DM spectrum in leptonic channels. Second, limits from antiprotons severely constrain the DM interpretation of the excess in the hadronic channel, for standard assumptions on the Galactic propagation parameters and solar modulation. However, they considerably relax if more conservative choices are adopted.
Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverDoctoral thesis . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationDoctoral thesis . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
more_vert Hyper Article en Lig... arrow_drop_down INRIA a CCSD electronic archive serverDoctoral thesis . 2015Data sources: INRIA a CCSD electronic archive serverMémoires en Sciences de l'Information et de la CommunicationDoctoral thesis . 2015add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article 2010Publisher:IEEE Camara, M.B.; Gualous, H.; Dakyo, B.; Nichita, C.; Makany, P.;This paper presents a careful study related to a more efficient energy management between lithium battery (with rated voltage of 24V) and Ultracapacitors (UC) for Hybrid Electric Vehicle (HEV) applications. This association is due to the present trend in the field, knowing that the major drawback of the HEV is the autonomy problem. Thus, using the Hybrid energy source (such as UC + battery) and with a good energy management improves the HEV performances. In this paper, battery and Ultracapacitors (10 cells of 2.7V in series) are coupled to DC-bus using two buck-boost converters. The main contribution of this paper is focused on DC-bus voltage and currents control strategy based on polynomial (RST) controller. Through some simulations in MATLAB/Simulink software and experimental results, the authors present an improved energy management for HEV.
Hyper Article en Lig... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYMémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/vppc.2010.5729140&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 10 citations 10 popularity Top 10% influence Top 10% impulse Average Powered by BIP!
more_vert Hyper Article en Lig... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYMémoires en Sciences de l'Information et de la CommunicationConference object . 2010License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1109/vppc.2010.5729140&type=result"></script>'); --> </script>
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