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description Publicationkeyboard_double_arrow_right Article , Conference object 2008Publisher:Institute of Electrical and Electronics Engineers (IEEE) Authors: Shpanin, L.; Jones, G. R.; Spencer, J. W.; Djakov, B. E.;A new approach for the electromagnetic control and propulsion of a current carrying electric arc plasma ring is described. The essence of the approach is to form and manipulate the arc plasma outside rather than inside a magnetic field producing coil so that pulsed plasma thrusts can be produced in a choice of different directions. The interaction of the electric arc, formed in atmospheric pressure air, with such a magnetic field has been investigated. It has been shown that a stable azimuthal plasma ring can be rapidly produced by the simple process of separating two annular contacts. Pulsed plasma propulsion is obtained when the arc plasma and B-field sustaining current is reduced to zero whereby the constraining electromagnetic forces are removed and, as a consequence, the resulting plasma ring expands radially outwards. Several different measurement techniques have been deployed for investigating the behavior of the plasma ring. These include electrical probing, B-field probing and high-speed plus video photography. The results suggest that the plasma control and propulsion is governed by a combination of effects including ablation of the material around which the plasma ring is formed and self-pressurization related to the device geometry, as well as the electromagnetic forces. Preliminary results indicate that through the use of appropriate device geometries, the arc plasma may be propelled in axially opposite directions as well as radially.
IEEE Transactions on... arrow_drop_down IEEE Transactions on Plasma ScienceArticle . 2008 . Peer-reviewedLicense: IEEE CopyrightData sources: Crossrefadd 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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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/tps.2008.2004269&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu6 citations 6 popularity Average influence Top 10% impulse Average Powered by BIP!
more_vert IEEE Transactions on... arrow_drop_down IEEE Transactions on Plasma ScienceArticle . 2008 . Peer-reviewedLicense: IEEE CopyrightData 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=10.1109/tps.2008.2004269&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal , Conference object 2017 Switzerland, Saudi ArabiaPublisher:Elsevier BV Antoine Descoeudres; Stefaan De Wolf; Eiji Kobayashi; Eiji Kobayashi; Jacques Levrat; Matthieu Despeisse; Christophe Ballif; Franz-Josef Haug;handle: 10754/625637
Silicon heterojunction solar cells use crystalline silicon (c-Si) wafers as optical absorbers and employ bilayers of doped/intrinsic hydrogenated amorphous silicon (a-Si:H) to form passivating contacts. Recently, we demonstrated that such solar cells increase their operating voltages and thus their conversion efficiencies during light exposure. We found that this performance increase is due to improved passivation of the a-Si:H/c-Si interface and is induced by injected charge carriers (either by light soaking or forward-voltage biasing of the device). Here, we discuss this counterintuitive behavior and establish that: (i) the performance increase is observed in solar cells as well as modules; (ii) this phenomenon requires the presence of doped a-Si:H films, but is independent from whether light is incident from the a-Si:H(p) or the a-Si:H(n) side; (iii) UV and blue photons do not play a role in this effect; (iv) the performance increase can be observed under illumination intensities as low as 20 W m(-1) (0.02-sun) and appears to be almost identical in strength when under 1-sun (1000 W m(-1)); (v) the underlying physical mechanism likely differs from annealing-induced surface passivation.
Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 2017 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefInfoscience - École polytechnique fédérale de LausanneConference objectData sources: Infoscience - École polytechnique fédérale de LausanneKing Abdullah University of Science and Technology: KAUST RepositoryArticle . 2017Data 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=10.1016/j.solmat.2017.06.023&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 66 citations 66 popularity Top 1% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 2017 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefInfoscience - École polytechnique fédérale de LausanneConference objectData sources: Infoscience - École polytechnique fédérale de LausanneKing Abdullah University of Science and Technology: KAUST RepositoryArticle . 2017Data 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=10.1016/j.solmat.2017.06.023&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2017 United KingdomPublisher:Elsevier BV Mohammed Al-Faham; Ali Safa Alsaegh; Ali Safa Alsaegh; Agustin Valera-Medina; Fares Hatem; Fares Hatem;Swirl combustors have proven as effective flame stabilisers over a wide range of operation conditions thanks to the formation of well-known swirl coherent structures. However, employment of swirl combustors to work on lean premixed combustion modes while introducing alternative fuels such as high hydrogen blends result in many combustion instabilities. Under these conditions, flame flashback has been considered as one of the major instability problems that have the potential of causing considerable damages of the combustion systems hardware in addition to the significant increase in pollutant levels. Combustion Induced Vortex Breakdown (CIVB) is considered a very particular mode of flashback mechanism in swirling flows as this type of flashback occurs even when the fresh mixture’s velocity is higher than the flame speed, consequence of the interaction between swirl structures and swirl burner geometries. Improvements of burner geometries and manipulation of swirl flows can produce good resistance against this type of flashback. However, increase flame flashback resistance against CIVB can lead to an increase in the propensity of another flashback mechanism, Boundary Layer Flashback (BLF). Thus this paper presents an experimental and numerical approach that allows the increase in CIVB resistance by using diffusive air injection and simultaneously avoid BLF by changing the wall boundary layer characteristics using microsurface grids as a liner for the nozzle wall. Results show that using those two techniques together has promising potentials regarding wider stable operation for swirl combustors, enabling them to burn a great variety of fuel blends safely.
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=10.1016/j.egypro.2017.12.358&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 4 citations 4 popularity Average influence Average impulse Average Powered by BIP!
download 13download downloads 13 Powered bymore_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=10.1016/j.egypro.2017.12.358&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2020 JapanPublisher:Elsevier BV Tamer M. Ismail; Yasunori Kobayashi; Kunio Yoshikawa; Ding Lu; Takahiro Kobori; Kuniomi Araki; Kiryu Kanazawa; Fumitake Takahashi; M.Abd El-Salam;Abstract Many organizations in the world are interested in waste management problems and their potential solutions. In order to solve these problems, a Japanese venture company has developed an innovative thermal decomposer for organic wastes called ERCM (Earth-Resource-Ceramic-Machine). The ERCM reactor employs electron injected air to promote the thermal decomposition reaction, while the effect of electron injection into air has not yet been clarified. An experimental work was performed using a fixed bed reactor to explore the effects of different parameters of electron injection into air, the reaction temperature and different feedstock on the syngas generation. The main purpose of this study is to clarify the phenomena occurring in the ERCM reactor where a direct current electric field is produced in the flame reaction zone to enhance the thermal decomposition of wastes. In this regard, a mathematical model for simulating the thermal decomposition of solid waste in the presence of an electric field have been developed. The equations of aero-thermochemistry are coupled to the balance equations for densities of charged species, and the Poisson equation for the electrical potential is solved. The model was validated by the experimental data and showed a good agreement. The results showed that the electric field significantly improves the stabilization of the flame. From the release behavior of CO and CO2, it is noted that the electron injection would affect the char combustion process significantly. Finally the effect of the flame reaction zone generated by the field induced ion wind on the thermal decomposition was investigated.
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=10.1016/j.apenergy.2020.115157&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 3 citations 3 popularity Top 10% influence Average impulse Average 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=10.1016/j.apenergy.2020.115157&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Journal 2018Publisher:Springer Science and Business Media LLC Galib Hashmi; Mohammad Junaebur Rashid; Zahid Mahmood; Mahbubul Hoq; Md. Habibur Rahman;En este trabajo, se ha investigado el impacto de seis capas diferentes de recubrimiento antirreflectante (ARC) utilizando el software de simulación PC1D. La simulación muestra que el rango de 500–700 nm sería adecuado para diseñar un ARCO. Diseñando un ARCO de nitruro de silicio de una sola capa (Si3N4) para una longitud de onda de 600 nm y con un espesor de 74.257 nm, se ha simulado una célula solar de silicio con una eficiencia del 20.35%. Le sigue muy de cerca una célula solar de silicio con una eficiencia del 20,34% con una capa de ARCO de óxido de zinc (ZnO) de 74,87 nm de espesor. Se ha observado un aumento significativo en la eficiencia al aplicar ARC con respecto a no aplicar ningún tipo de ARC. Después de un modelado eficiente de las células solares, se está logrando una eficiencia óptima del 20,67% mediante el uso de la pasivación superficial de SiO2 y la capa de ARCO de Si3N4. Los efectos sobre la tensión, la corriente, la eficiencia fotovoltaica, la reflectividad y la eficiencia cuántica externa debidos a los ARC también están representados en este trabajo. Dans ce travail, l'impact de six couches différentes de revêtement antireflet (ARC) a été étudié à l'aide du logiciel de simulation PC1D. La simulation montre que la plage de 500–700 nm serait appropriée pour concevoir un ARC. En concevant un ARC de nitrure de silicium monocouche (Si3N4) pour une longueur d'onde de 600 nm et une épaisseur de 74,257 nm, une cellule solaire en silicium avec une efficacité de 20,35% a été simulée. Très étroitement suivie par une cellule solaire en silicium à 20,34 % d'efficacité avec une couche d'ARC en oxyde de zinc (ZnO) de 74,87 nm d'épaisseur. Une augmentation significative de l'efficacité a été observée en appliquant L'ARC par rapport à l'absence d'application de tout type d'ARC. Après une modélisation efficace des cellules solaires, une efficacité optimale de 20,67 % est obtenue en utilisant la passivation de surface SiO2 et la couche D'ARC Si3N4. Les effets sur la tension, le courant, l'efficacité photovoltaïque, la réflectivité et l'efficacité quantique externe dus aux ARC sont également représentés dans ce travail. In this work, the impact of six different anti-reflection coating (ARC) layers has been investigated using PC1D simulation software. Simulation shows that the range of 500–700 nm would be suitable for designing an ARC. Designing a single-layer silicon nitride (Si3N4) ARC for 600 nm wavelength and with a thickness of 74.257 nm, a silicon solar cell with 20.35% efficiency has been simulated. Very closely followed by a 20.34% efficient silicon solar cell with 74.87 nm thick zinc oxide (ZnO) ARC layer. Significant increase in efficiency has been observed by applying ARC in respect to not applying any kind of ARC. After efficient solar cell modeling, optimum efficiency of 20.67% is being achieved by using SiO2 surface passivation and Si3N4 ARC layer. The effects on voltage, current, photovoltaic efficiency, reflectivity and external quantum efficiency due to ARCs are also represented in this work. في هذا العمل، تم التحقيق في تأثير ست طبقات مختلفة من الطلاء المضاد للانعكاس (ARC) باستخدام برنامج محاكاة PC1D. تظهر المحاكاة أن النطاق من 500–700 نانومتر سيكون مناسبًا لتصميم القوس. تصميم قوس نيتريد السيليكون أحادي الطبقة (Si3N4) بطول موجي 600 نانومتر وبسمك 74.257 نانومتر، تمت محاكاة خلية شمسية من السيليكون بكفاءة 20.35 ٪. تليها عن كثب خلية شمسية من السيليكون فعالة بنسبة 20.34 ٪ مع طبقة قوسية من أكسيد الزنك بسماكة 74.87 نانومتر (ZnO). لوحظت زيادة كبيرة في الكفاءة من خلال تطبيق القوس فيما يتعلق بعدم تطبيق أي نوع من القوس. بعد نمذجة الخلايا الشمسية بكفاءة، يتم تحقيق الكفاءة المثلى بنسبة 20.67 ٪ باستخدام تخميل سطح SiO2 وطبقة Si3N4 القوسية. يتم تمثيل التأثيرات على الجهد والتيار والكفاءة الكهروضوئية والانعكاسية والكفاءة الكمية الخارجية بسبب ARCs أيضًا في هذا العمل.
Journal of Theoretic... arrow_drop_down Journal of Theoretical and Applied PhysicsArticle . 2018 . 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=10.1007/s40094-018-0313-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesgold 39 citations 39 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Journal of Theoretic... arrow_drop_down Journal of Theoretical and Applied PhysicsArticle . 2018 . 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=10.1007/s40094-018-0313-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2018 United KingdomPublisher:MDPI AG Yuanwei Zhu; Shengtao Li; Daomin Min; Shijun Li; Huize Cui; George Chen;doi: 10.3390/en11061547
Based on the existing acknowledgment that space charge modulates AC and DC breakdown of insulating materials, this investigation promotes the related investigation into the situations of more complex electrical stress, i.e., AC-DC combined voltages. Experimentally, the AC-DC breakdown characteristics of oil impregnated paper insulation were systematically investigated. The effects of pre-applied voltage waveform, AC component ratio, and sample thickness on AC-DC breakdown characteristics were analyzed. After that, based on an improved bipolar charge transport model, the space charge profiles and the space charge induced electric field distortion during AC-DC breakdown were numerically simulated to explain the differences in breakdown characteristics between the pre-applied AC and pre-applied DC methods under AC-DC combined voltages. It is concluded that large amounts of homo-charges are accumulated during AC-DC breakdown, which results in significantly distorted inner electric field, leading to variations of breakdown characteristics of oil impregnated paper insulation. Therefore, space charges under AC-DC combined voltages must be considered in the design of converter transformers. In addition, this investigation could provide supporting breakdown data for insulation design of converter transformers and could promote better understanding on the breakdown mechanism of insulating materials subjected to AC-DC combined voltages.
e-Prints Soton 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.
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=10.3390/en11061547&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 7 citations 7 popularity Top 10% influence Average impulse Average Powered by BIP!
visibility 12visibility views 12 download downloads 102 Powered bymore_vert e-Prints Soton 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.
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=10.3390/en11061547&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2023Publisher:Elsevier BV Authors: Tarek O. Abdul Fattah; Janet Jacobs; Vladimir P. Markevich; Nikolay V. Abrosimov; +3 AuthorsTarek O. Abdul Fattah; Janet Jacobs; Vladimir P. Markevich; Nikolay V. Abrosimov; Matthew P. Halsall; Iain F. Crowe; Anthony R. Peaker;Before lower purity, lower cost silicon (Si) materials, such as compensated Si, can play a role in the terawatt-level (TW) capacity of photovoltaics, a better understanding of the fundamental properties of impurities in compensated Si is essential. In this work, high-resolution photoluminescence (PL) has been used to study the charge carrier radiative recombination through Donor-Acceptor pairs (DAPs) in phosphorus (P) and gallium (Ga) co-doped Si material grown for solar cell applications. The high spectral resolution of our PL system, 0.06 meV, enables us to overcome hitherto prior issues of overlapping spectral lines, giving access to extremely fine structures associated with DA pair (DAP) recombination. Our results confirm the presence of three broad bands and a discrete line structure related to DAP luminescence. The comparison of the discrete line structure due to DAPs recombination in the PL spectra with the theoretically predicted one allows the accurate determination of the Ga ionization energy. Temperature-dependent PL is then used to understand the thermally-induced changes in the DAP luminescence. In particular, we observe that the radiative recombination channel remains active for distant DAPs up to ∼40 K, unlike that for close-range DAPs for which the radiative channel is quenched after only slight increases in the temperature range 10–25 K. Furthermore, the analysis of the temperature dependent changes in the PL intensity of the broad DAP bands up to ∼200 K is used to derive the ionization energy of P donors in compensated Si material. In light of this important information, the significance of using high resolution PL to analyse spectral features in compensated Si is demonstrated.
Journal of Science: ... arrow_drop_down Journal of Science: Advanced Materials and DevicesArticle . 2023 . 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.euAccess RoutesGreen gold 2 citations 2 popularity Average influence Average impulse Average Powered by BIP!
more_vert Journal of Science: ... arrow_drop_down Journal of Science: Advanced Materials and DevicesArticle . 2023 . 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=10.1016/j.jsamd.2023.100629&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 1995Publisher:Elsevier BV R. D. Tomlinson; A.A. Dost; Arthur E. Hill; O. Kusmartseva; Seppo Leppävuori; A. Zegadi; Richard D. Pilkington; Waqar Ahmed; J. Levoska; E. Ahmed;Abstract The efficiency of a solar cells utilizing polycrystalline Cu(In,Ga)Se 2 is to a large extent limited by crystalline defects of the semiconductor. Depending on the fabrication process the density of grain boundaries and dislocations, can vary considerably. However, the material properties can be improved significantly by the subsequent processing steps. In this paper results obtained using various post deposition methods to improve the structural and electro-optical properties of CuIn 0.75 Ga 0.25 Se 2 (CIGS) thin films have been presented and discussed. Films deposited by the evaporation of pre-reacted polycrystalline CIGS onto glass substrate were subsequently processed under several sets of conditions including vacuum, selenium, inert and forming gas ambients at different temperature and times. The structural and electro-optical properties of both as-deposited and annealed films were studied using a variety of analytical techniques. X-ray diffraction (XRD) and scanning electron microscopy (SEM) studies of the films showed a columnar structure with strong orientation, which after heat treatments was relaxed to form a chalcopyrite structure. Raman analysis showed that full wave half maximum (FWHM) value reduced from 20 to 10 cm −1 with the annealing process indicating a change in both film composition and microstructure. In addition, investigations using energy dispersive X-ray analysis (EDAX), X-ray fluorescence (XRF) and Rutherford backscattering spectroscopy (RBS) revealed that the composition was approaching that of the starting polycrystalline material. Both n- and p-type conductivities were observed and gave resistivity values in the range 10 −1 to 10 6 Ω cm. Annealing in selenium changed the observed n-type conductivity of the as-deposited films to p-type. Photoacoustic spectroscopy (PAS) have also been applied to verify the improvement in the optical properties of annealed films.
Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 1995 . Peer-reviewedLicense: Elsevier TDMData 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=10.1016/0927-0248(94)00175-8&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 16 citations 16 popularity Average influence Top 10% impulse Average Powered by BIP!
more_vert Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 1995 . Peer-reviewedLicense: Elsevier TDMData 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=10.1016/0927-0248(94)00175-8&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2008 Australia, Australia, United Kingdom, AustraliaPublisher:Springer Science and Business Media LLC S. Golenetskii; Fabrizio Fiore; David N. Burrows; Martin Jelínek; Krzysztof Nawrocki; L. Vetere; Javier Gorosabel; A. J. van der Horst; P. A. Curran; Iain A. Steele; S. B. Pandey; A. J. Castro-Tirado; A. Melandri; Peter Mészáros; A. Cucchiara; Raffaella Margutti; E. P. Mazets; Andrew S. Fruchter; R. L. C. Starling; P. D'Avanzo; G. Greco; Nial R. Tanvir; Ralph A. M. J. Wijers; J. Cummings; Stefan Immler; Gino Tosti; Tsvi Piran; Andreja Gomboc; M. T. Page; J. M. Winters; Klaas Wiersema; Enrico Ramirez-Ruiz; Grzegorz Kasprowicz; Bing Zhang; M. Della Valle; R. Aptekar; V. La Parola; A. P. Beardmore; Patricia Schady; C. Guidorzi; C. Guidorzi; Robert J. Smith; Neil Gehrels; Guido Chincarini; Guido Chincarini; Corrado Bartolini; V. Pal'Shin; K. L. Page; G. M. Beskin; Lech Mankiewicz; Marcin Sokolowski; Chryssa Kouveliotou; Stefano Covino; F. M. Zerbi; Jonathan Granot; Atish Kamble; D. B. Fox; P. T. O'Brien; A. D. Falcone; Judith Racusin; Zsolt Paragi; Scott Barthelmy; A. Moretti; S. Bondar; S. V. Karpov; Grzegorz Wrochna; Dino Fugazza; Sergio Campana; P. A. Evans; P. W. A. Roming; E. Molinari; Richard G. Strom; Richard G. Strom; Valerio D'Elia; S. R. Oates; Xue-Feng Wu; Xue-Feng Wu; Katarzyna Małek; P. Oleynik; Stephen T. Holland; Stephen T. Holland; Adalberto Piccioni; J. P. Osborne; D. D. Frederiks; V. Mangano; M. Cwiok; C. Pagani; M. Perri; Malcolm N. Bremer; M. A. Garrett; M. A. Garrett; M. A. Garrett; Lech Wiktor Piotrowski; Aleksander Filip Zarnecki; Adriano Guarnieri; M. Ulanov; W. Dominik; A. de Ugarte Postigo; Andrew J. Levan; Vincenzo Testa;doi: 10.1038/nature07270
handle: 11245/1.301930 , 2381/25356 , 2381/42419 , 1959.3/47559 , 20.500.11937/15775
doi: 10.1038/nature07270
handle: 11245/1.301930 , 2381/25356 , 2381/42419 , 1959.3/47559 , 20.500.11937/15775
Long-duration gamma-ray bursts (GRBs) release copious amounts of energy across the entire electromagnetic spectrum, and so provide a window into the process of black hole formation from the collapse of massive stars. Previous early optical observations of even the most exceptional GRBs (990123 and 030329) lacked both the temporal resolution to probe the optical flash in detail and the accuracy needed to trace the transition from the prompt emission within the outflow to external shocks caused by interaction with the progenitor environment. Here we report observations of the extraordinarily bright prompt optical and gamma-ray emission of GRB 080319B that provide diagnostics within seconds of its formation, followed by broadband observations of the afterglow decay that continued for weeks. We show that the prompt emission stems from a single physical region, implying an extremely relativistic outflow that propagates within the narrow inner core of a two-component jet.
Nature arrow_drop_down Swinburne University of Technology: Swinburne Research BankArticle . 2008Data 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=10.1038/nature07270&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 436 citations 436 popularity Top 1% influence Top 1% impulse Top 0.1% Powered by BIP!
visibility 4visibility views 4 download downloads 207 Powered bymore_vert Nature arrow_drop_down Swinburne University of Technology: Swinburne Research BankArticle . 2008Data 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=10.1038/nature07270&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Other literature type 2010 United KingdomPublisher:Optica Publishing Group Kang Kang Chen; Shaif-ul Alam; J.H.V. Price; J. R. Hayes; Di Lin; A. Malinowski; Christophe A. Codemard; Debashri Ghosh; Mrinmay Pal; Shyamal K. Bhadra; David J. Richardson;Presentamos una fuente supercontinua bombeada con mopa de fibra de picosegundos con una salida de 39 W, que abarca al menos 0,4-2,25 micrómetros a una velocidad de repetición de 114,8 MHz. El PCF de 2 m de largo tenía un núcleo grande de 4,4 micrómetros de diámetro y un diseño de delta alto que condujo a una eficiencia de acoplamiento del 80%, un umbral de daño alto y una generación rápida de generación continua visible a partir de los pulsos de entrada de picosegundos. La densidad de potencia alta y relativamente uniforme a través de la región espectral visible fue de aproximadamente 31.7 mW/nm correspondiente a la densidad de potencia máxima de aproximadamente 12.5 W/nm para los pulsos de entrada de 21 ps. La densidad de potencia máxima se incrementó a 26,9 W/nm mediante la reducción de la tasa de repetición a 28 MHz. Esto representa un aumento en la potencia media y máxima en comparación con las fuentes de supercontinuo visibles informadas anteriormente de sistemas bombeados o pulsados CW. Nous rapportons une source de supercontinuum pompée MOPA à fibre picoseconde avec une sortie de 39 W, couvrant au moins 0,4-2,25 micromètres à un taux de répétition de 114,8 MHz. Le PCF de 2 m de long avait un grand noyau de 4,4 micromètres de diamètre et une conception à delta élevé qui a conduit à une efficacité de couplage de 80 %, à un seuil de dommage élevé et à une génération rapide de continuum visible à partir des impulsions d'entrée picosecondes. La densité de puissance élevée et relativement uniforme dans la région spectrale visible était d'environ 31,7 mW/nm, ce qui correspond à une densité de puissance de crête d'environ 12,5 W/nm pour les impulsions d'entrée de 21 ps. La densité de puissance de crête a été augmentée à 26,9 W/nm en réduisant le taux de répétition à 28 MHz. Cela représente une augmentation de la puissance moyenne et de crête par rapport aux sources de supercontinuum visibles précédemment rapportées provenant de systèmes pompés par ondes entretenues ou pulsés. We report a picosecond fiber MOPA pumped supercontinuum source with 39 W output, spanning at least 0.4-2.25 microm at a repetition rate of 114.8 MHz. The 2m long PCF had a large, 4.4 microm diameter core and a high-delta design which led to an 80% coupling efficiency, high damage threshold and rapid generation of visible continuum generation from the picosecond input pulses. The high and relatively uniform power density across the visible spectral region was approximately 31.7 mW/nm corresponding to peak power density of approximately 12.5 W/nm for the 21 ps input pulses. The peak power density was increased to 26.9 W/nm by reducing the repetition rate to 28 MHz. This represents an increase in both average and peak power compared to previously reported visible supercontinuum sources from either CW pumped or pulsed-systems. نبلغ عن مصدر فائق الاستمرارية لضخ ألياف بيكو ثانية مع خرج 39 واط، يمتد على الأقل 0.4-2.25 ميكروم بمعدل تكرار 114.8 ميجا هرتز. كان لـ PCF بطول 2 متر قلب كبير بقطر 4.4 ميكروم وتصميم عالي الدلتا مما أدى إلى كفاءة اقتران 80 ٪ وعتبة تلف عالية وتوليد سريع لتوليد سلسلة متصلة مرئية من نبضات إدخال البيكوثانية. كانت كثافة القدرة العالية والمنتظمة نسبيًا عبر المنطقة الطيفية المرئية حوالي 31.7 مللي واط/نانومتر المقابلة لكثافة القدرة القصوى التي تبلغ حوالي 12.5 واط/نانومتر لنبضات الإدخال 21 جزء في الثانية. تمت زيادة كثافة الطاقة القصوى إلى 26.9 واط/نانومتر عن طريق تقليل معدل التكرار إلى 28 ميجاهرتز. ويمثل هذا زيادة في كل من متوسط الطاقة وذروتها مقارنة بمصادر الاستمرارية المرئية التي تم الإبلاغ عنها سابقًا من أنظمة ضخ الأسلحة الكيميائية أو الأنظمة النبضية.
e-Prints Soton 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.
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=10.1364/oe.18.005426&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu112 citations 112 popularity Top 10% influence Top 1% impulse Top 1% Powered by BIP!
more_vert e-Prints Soton 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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description Publicationkeyboard_double_arrow_right Article , Conference object 2008Publisher:Institute of Electrical and Electronics Engineers (IEEE) Authors: Shpanin, L.; Jones, G. R.; Spencer, J. W.; Djakov, B. E.;A new approach for the electromagnetic control and propulsion of a current carrying electric arc plasma ring is described. The essence of the approach is to form and manipulate the arc plasma outside rather than inside a magnetic field producing coil so that pulsed plasma thrusts can be produced in a choice of different directions. The interaction of the electric arc, formed in atmospheric pressure air, with such a magnetic field has been investigated. It has been shown that a stable azimuthal plasma ring can be rapidly produced by the simple process of separating two annular contacts. Pulsed plasma propulsion is obtained when the arc plasma and B-field sustaining current is reduced to zero whereby the constraining electromagnetic forces are removed and, as a consequence, the resulting plasma ring expands radially outwards. Several different measurement techniques have been deployed for investigating the behavior of the plasma ring. These include electrical probing, B-field probing and high-speed plus video photography. The results suggest that the plasma control and propulsion is governed by a combination of effects including ablation of the material around which the plasma ring is formed and self-pressurization related to the device geometry, as well as the electromagnetic forces. Preliminary results indicate that through the use of appropriate device geometries, the arc plasma may be propelled in axially opposite directions as well as radially.
IEEE Transactions on... arrow_drop_down IEEE Transactions on Plasma ScienceArticle . 2008 . Peer-reviewedLicense: IEEE CopyrightData 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=10.1109/tps.2008.2004269&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu6 citations 6 popularity Average influence Top 10% impulse Average Powered by BIP!
more_vert IEEE Transactions on... arrow_drop_down IEEE Transactions on Plasma ScienceArticle . 2008 . Peer-reviewedLicense: IEEE CopyrightData 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=10.1109/tps.2008.2004269&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal , Conference object 2017 Switzerland, Saudi ArabiaPublisher:Elsevier BV Antoine Descoeudres; Stefaan De Wolf; Eiji Kobayashi; Eiji Kobayashi; Jacques Levrat; Matthieu Despeisse; Christophe Ballif; Franz-Josef Haug;handle: 10754/625637
Silicon heterojunction solar cells use crystalline silicon (c-Si) wafers as optical absorbers and employ bilayers of doped/intrinsic hydrogenated amorphous silicon (a-Si:H) to form passivating contacts. Recently, we demonstrated that such solar cells increase their operating voltages and thus their conversion efficiencies during light exposure. We found that this performance increase is due to improved passivation of the a-Si:H/c-Si interface and is induced by injected charge carriers (either by light soaking or forward-voltage biasing of the device). Here, we discuss this counterintuitive behavior and establish that: (i) the performance increase is observed in solar cells as well as modules; (ii) this phenomenon requires the presence of doped a-Si:H films, but is independent from whether light is incident from the a-Si:H(p) or the a-Si:H(n) side; (iii) UV and blue photons do not play a role in this effect; (iv) the performance increase can be observed under illumination intensities as low as 20 W m(-1) (0.02-sun) and appears to be almost identical in strength when under 1-sun (1000 W m(-1)); (v) the underlying physical mechanism likely differs from annealing-induced surface passivation.
Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 2017 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefInfoscience - École polytechnique fédérale de LausanneConference objectData sources: Infoscience - École polytechnique fédérale de LausanneKing Abdullah University of Science and Technology: KAUST RepositoryArticle . 2017Data 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=10.1016/j.solmat.2017.06.023&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 66 citations 66 popularity Top 1% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 2017 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefInfoscience - École polytechnique fédérale de LausanneConference objectData sources: Infoscience - École polytechnique fédérale de LausanneKing Abdullah University of Science and Technology: KAUST RepositoryArticle . 2017Data 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=10.1016/j.solmat.2017.06.023&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2017 United KingdomPublisher:Elsevier BV Mohammed Al-Faham; Ali Safa Alsaegh; Ali Safa Alsaegh; Agustin Valera-Medina; Fares Hatem; Fares Hatem;Swirl combustors have proven as effective flame stabilisers over a wide range of operation conditions thanks to the formation of well-known swirl coherent structures. However, employment of swirl combustors to work on lean premixed combustion modes while introducing alternative fuels such as high hydrogen blends result in many combustion instabilities. Under these conditions, flame flashback has been considered as one of the major instability problems that have the potential of causing considerable damages of the combustion systems hardware in addition to the significant increase in pollutant levels. Combustion Induced Vortex Breakdown (CIVB) is considered a very particular mode of flashback mechanism in swirling flows as this type of flashback occurs even when the fresh mixture’s velocity is higher than the flame speed, consequence of the interaction between swirl structures and swirl burner geometries. Improvements of burner geometries and manipulation of swirl flows can produce good resistance against this type of flashback. However, increase flame flashback resistance against CIVB can lead to an increase in the propensity of another flashback mechanism, Boundary Layer Flashback (BLF). Thus this paper presents an experimental and numerical approach that allows the increase in CIVB resistance by using diffusive air injection and simultaneously avoid BLF by changing the wall boundary layer characteristics using microsurface grids as a liner for the nozzle wall. Results show that using those two techniques together has promising potentials regarding wider stable operation for swirl combustors, enabling them to burn a great variety of fuel blends safely.
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=10.1016/j.egypro.2017.12.358&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 4 citations 4 popularity Average influence Average impulse Average Powered by BIP!
download 13download downloads 13 Powered bymore_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=10.1016/j.egypro.2017.12.358&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2020 JapanPublisher:Elsevier BV Tamer M. Ismail; Yasunori Kobayashi; Kunio Yoshikawa; Ding Lu; Takahiro Kobori; Kuniomi Araki; Kiryu Kanazawa; Fumitake Takahashi; M.Abd El-Salam;Abstract Many organizations in the world are interested in waste management problems and their potential solutions. In order to solve these problems, a Japanese venture company has developed an innovative thermal decomposer for organic wastes called ERCM (Earth-Resource-Ceramic-Machine). The ERCM reactor employs electron injected air to promote the thermal decomposition reaction, while the effect of electron injection into air has not yet been clarified. An experimental work was performed using a fixed bed reactor to explore the effects of different parameters of electron injection into air, the reaction temperature and different feedstock on the syngas generation. The main purpose of this study is to clarify the phenomena occurring in the ERCM reactor where a direct current electric field is produced in the flame reaction zone to enhance the thermal decomposition of wastes. In this regard, a mathematical model for simulating the thermal decomposition of solid waste in the presence of an electric field have been developed. The equations of aero-thermochemistry are coupled to the balance equations for densities of charged species, and the Poisson equation for the electrical potential is solved. The model was validated by the experimental data and showed a good agreement. The results showed that the electric field significantly improves the stabilization of the flame. From the release behavior of CO and CO2, it is noted that the electron injection would affect the char combustion process significantly. Finally the effect of the flame reaction zone generated by the field induced ion wind on the thermal decomposition was investigated.
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=10.1016/j.apenergy.2020.115157&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 3 citations 3 popularity Top 10% influence Average impulse Average 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=10.1016/j.apenergy.2020.115157&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Journal 2018Publisher:Springer Science and Business Media LLC Galib Hashmi; Mohammad Junaebur Rashid; Zahid Mahmood; Mahbubul Hoq; Md. Habibur Rahman;En este trabajo, se ha investigado el impacto de seis capas diferentes de recubrimiento antirreflectante (ARC) utilizando el software de simulación PC1D. La simulación muestra que el rango de 500–700 nm sería adecuado para diseñar un ARCO. Diseñando un ARCO de nitruro de silicio de una sola capa (Si3N4) para una longitud de onda de 600 nm y con un espesor de 74.257 nm, se ha simulado una célula solar de silicio con una eficiencia del 20.35%. Le sigue muy de cerca una célula solar de silicio con una eficiencia del 20,34% con una capa de ARCO de óxido de zinc (ZnO) de 74,87 nm de espesor. Se ha observado un aumento significativo en la eficiencia al aplicar ARC con respecto a no aplicar ningún tipo de ARC. Después de un modelado eficiente de las células solares, se está logrando una eficiencia óptima del 20,67% mediante el uso de la pasivación superficial de SiO2 y la capa de ARCO de Si3N4. Los efectos sobre la tensión, la corriente, la eficiencia fotovoltaica, la reflectividad y la eficiencia cuántica externa debidos a los ARC también están representados en este trabajo. Dans ce travail, l'impact de six couches différentes de revêtement antireflet (ARC) a été étudié à l'aide du logiciel de simulation PC1D. La simulation montre que la plage de 500–700 nm serait appropriée pour concevoir un ARC. En concevant un ARC de nitrure de silicium monocouche (Si3N4) pour une longueur d'onde de 600 nm et une épaisseur de 74,257 nm, une cellule solaire en silicium avec une efficacité de 20,35% a été simulée. Très étroitement suivie par une cellule solaire en silicium à 20,34 % d'efficacité avec une couche d'ARC en oxyde de zinc (ZnO) de 74,87 nm d'épaisseur. Une augmentation significative de l'efficacité a été observée en appliquant L'ARC par rapport à l'absence d'application de tout type d'ARC. Après une modélisation efficace des cellules solaires, une efficacité optimale de 20,67 % est obtenue en utilisant la passivation de surface SiO2 et la couche D'ARC Si3N4. Les effets sur la tension, le courant, l'efficacité photovoltaïque, la réflectivité et l'efficacité quantique externe dus aux ARC sont également représentés dans ce travail. In this work, the impact of six different anti-reflection coating (ARC) layers has been investigated using PC1D simulation software. Simulation shows that the range of 500–700 nm would be suitable for designing an ARC. Designing a single-layer silicon nitride (Si3N4) ARC for 600 nm wavelength and with a thickness of 74.257 nm, a silicon solar cell with 20.35% efficiency has been simulated. Very closely followed by a 20.34% efficient silicon solar cell with 74.87 nm thick zinc oxide (ZnO) ARC layer. Significant increase in efficiency has been observed by applying ARC in respect to not applying any kind of ARC. After efficient solar cell modeling, optimum efficiency of 20.67% is being achieved by using SiO2 surface passivation and Si3N4 ARC layer. The effects on voltage, current, photovoltaic efficiency, reflectivity and external quantum efficiency due to ARCs are also represented in this work. في هذا العمل، تم التحقيق في تأثير ست طبقات مختلفة من الطلاء المضاد للانعكاس (ARC) باستخدام برنامج محاكاة PC1D. تظهر المحاكاة أن النطاق من 500–700 نانومتر سيكون مناسبًا لتصميم القوس. تصميم قوس نيتريد السيليكون أحادي الطبقة (Si3N4) بطول موجي 600 نانومتر وبسمك 74.257 نانومتر، تمت محاكاة خلية شمسية من السيليكون بكفاءة 20.35 ٪. تليها عن كثب خلية شمسية من السيليكون فعالة بنسبة 20.34 ٪ مع طبقة قوسية من أكسيد الزنك بسماكة 74.87 نانومتر (ZnO). لوحظت زيادة كبيرة في الكفاءة من خلال تطبيق القوس فيما يتعلق بعدم تطبيق أي نوع من القوس. بعد نمذجة الخلايا الشمسية بكفاءة، يتم تحقيق الكفاءة المثلى بنسبة 20.67 ٪ باستخدام تخميل سطح SiO2 وطبقة Si3N4 القوسية. يتم تمثيل التأثيرات على الجهد والتيار والكفاءة الكهروضوئية والانعكاسية والكفاءة الكمية الخارجية بسبب ARCs أيضًا في هذا العمل.
Journal of Theoretic... arrow_drop_down Journal of Theoretical and Applied PhysicsArticle . 2018 . 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=10.1007/s40094-018-0313-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesgold 39 citations 39 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Journal of Theoretic... arrow_drop_down Journal of Theoretical and Applied PhysicsArticle . 2018 . 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=10.1007/s40094-018-0313-0&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2018 United KingdomPublisher:MDPI AG Yuanwei Zhu; Shengtao Li; Daomin Min; Shijun Li; Huize Cui; George Chen;doi: 10.3390/en11061547
Based on the existing acknowledgment that space charge modulates AC and DC breakdown of insulating materials, this investigation promotes the related investigation into the situations of more complex electrical stress, i.e., AC-DC combined voltages. Experimentally, the AC-DC breakdown characteristics of oil impregnated paper insulation were systematically investigated. The effects of pre-applied voltage waveform, AC component ratio, and sample thickness on AC-DC breakdown characteristics were analyzed. After that, based on an improved bipolar charge transport model, the space charge profiles and the space charge induced electric field distortion during AC-DC breakdown were numerically simulated to explain the differences in breakdown characteristics between the pre-applied AC and pre-applied DC methods under AC-DC combined voltages. It is concluded that large amounts of homo-charges are accumulated during AC-DC breakdown, which results in significantly distorted inner electric field, leading to variations of breakdown characteristics of oil impregnated paper insulation. Therefore, space charges under AC-DC combined voltages must be considered in the design of converter transformers. In addition, this investigation could provide supporting breakdown data for insulation design of converter transformers and could promote better understanding on the breakdown mechanism of insulating materials subjected to AC-DC combined voltages.
e-Prints Soton 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.
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=10.3390/en11061547&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 7 citations 7 popularity Top 10% influence Average impulse Average Powered by BIP!
visibility 12visibility views 12 download downloads 102 Powered bymore_vert e-Prints Soton 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.
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=10.3390/en11061547&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2023Publisher:Elsevier BV Authors: Tarek O. Abdul Fattah; Janet Jacobs; Vladimir P. Markevich; Nikolay V. Abrosimov; +3 AuthorsTarek O. Abdul Fattah; Janet Jacobs; Vladimir P. Markevich; Nikolay V. Abrosimov; Matthew P. Halsall; Iain F. Crowe; Anthony R. Peaker;Before lower purity, lower cost silicon (Si) materials, such as compensated Si, can play a role in the terawatt-level (TW) capacity of photovoltaics, a better understanding of the fundamental properties of impurities in compensated Si is essential. In this work, high-resolution photoluminescence (PL) has been used to study the charge carrier radiative recombination through Donor-Acceptor pairs (DAPs) in phosphorus (P) and gallium (Ga) co-doped Si material grown for solar cell applications. The high spectral resolution of our PL system, 0.06 meV, enables us to overcome hitherto prior issues of overlapping spectral lines, giving access to extremely fine structures associated with DA pair (DAP) recombination. Our results confirm the presence of three broad bands and a discrete line structure related to DAP luminescence. The comparison of the discrete line structure due to DAPs recombination in the PL spectra with the theoretically predicted one allows the accurate determination of the Ga ionization energy. Temperature-dependent PL is then used to understand the thermally-induced changes in the DAP luminescence. In particular, we observe that the radiative recombination channel remains active for distant DAPs up to ∼40 K, unlike that for close-range DAPs for which the radiative channel is quenched after only slight increases in the temperature range 10–25 K. Furthermore, the analysis of the temperature dependent changes in the PL intensity of the broad DAP bands up to ∼200 K is used to derive the ionization energy of P donors in compensated Si material. In light of this important information, the significance of using high resolution PL to analyse spectral features in compensated Si is demonstrated.
Journal of Science: ... arrow_drop_down Journal of Science: Advanced Materials and DevicesArticle . 2023 . 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=10.1016/j.jsamd.2023.100629&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 2 citations 2 popularity Average influence Average impulse Average Powered by BIP!
more_vert Journal of Science: ... arrow_drop_down Journal of Science: Advanced Materials and DevicesArticle . 2023 . 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=10.1016/j.jsamd.2023.100629&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 1995Publisher:Elsevier BV R. D. Tomlinson; A.A. Dost; Arthur E. Hill; O. Kusmartseva; Seppo Leppävuori; A. Zegadi; Richard D. Pilkington; Waqar Ahmed; J. Levoska; E. Ahmed;Abstract The efficiency of a solar cells utilizing polycrystalline Cu(In,Ga)Se 2 is to a large extent limited by crystalline defects of the semiconductor. Depending on the fabrication process the density of grain boundaries and dislocations, can vary considerably. However, the material properties can be improved significantly by the subsequent processing steps. In this paper results obtained using various post deposition methods to improve the structural and electro-optical properties of CuIn 0.75 Ga 0.25 Se 2 (CIGS) thin films have been presented and discussed. Films deposited by the evaporation of pre-reacted polycrystalline CIGS onto glass substrate were subsequently processed under several sets of conditions including vacuum, selenium, inert and forming gas ambients at different temperature and times. The structural and electro-optical properties of both as-deposited and annealed films were studied using a variety of analytical techniques. X-ray diffraction (XRD) and scanning electron microscopy (SEM) studies of the films showed a columnar structure with strong orientation, which after heat treatments was relaxed to form a chalcopyrite structure. Raman analysis showed that full wave half maximum (FWHM) value reduced from 20 to 10 cm −1 with the annealing process indicating a change in both film composition and microstructure. In addition, investigations using energy dispersive X-ray analysis (EDAX), X-ray fluorescence (XRF) and Rutherford backscattering spectroscopy (RBS) revealed that the composition was approaching that of the starting polycrystalline material. Both n- and p-type conductivities were observed and gave resistivity values in the range 10 −1 to 10 6 Ω cm. Annealing in selenium changed the observed n-type conductivity of the as-deposited films to p-type. Photoacoustic spectroscopy (PAS) have also been applied to verify the improvement in the optical properties of annealed films.
Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 1995 . Peer-reviewedLicense: Elsevier TDMData 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=10.1016/0927-0248(94)00175-8&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 16 citations 16 popularity Average influence Top 10% impulse Average Powered by BIP!
more_vert Solar Energy Materia... arrow_drop_down Solar Energy Materials and Solar CellsArticle . 1995 . Peer-reviewedLicense: Elsevier TDMData 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=10.1016/0927-0248(94)00175-8&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2008 Australia, Australia, United Kingdom, AustraliaPublisher:Springer Science and Business Media LLC S. Golenetskii; Fabrizio Fiore; David N. Burrows; Martin Jelínek; Krzysztof Nawrocki; L. Vetere; Javier Gorosabel; A. J. van der Horst; P. A. Curran; Iain A. Steele; S. B. Pandey; A. J. Castro-Tirado; A. Melandri; Peter Mészáros; A. Cucchiara; Raffaella Margutti; E. P. Mazets; Andrew S. Fruchter; R. L. C. Starling; P. D'Avanzo; G. Greco; Nial R. Tanvir; Ralph A. M. J. Wijers; J. Cummings; Stefan Immler; Gino Tosti; Tsvi Piran; Andreja Gomboc; M. T. Page; J. M. Winters; Klaas Wiersema; Enrico Ramirez-Ruiz; Grzegorz Kasprowicz; Bing Zhang; M. Della Valle; R. Aptekar; V. La Parola; A. P. Beardmore; Patricia Schady; C. Guidorzi; C. Guidorzi; Robert J. Smith; Neil Gehrels; Guido Chincarini; Guido Chincarini; Corrado Bartolini; V. Pal'Shin; K. L. Page; G. M. Beskin; Lech Mankiewicz; Marcin Sokolowski; Chryssa Kouveliotou; Stefano Covino; F. M. Zerbi; Jonathan Granot; Atish Kamble; D. B. Fox; P. T. O'Brien; A. D. Falcone; Judith Racusin; Zsolt Paragi; Scott Barthelmy; A. Moretti; S. Bondar; S. V. Karpov; Grzegorz Wrochna; Dino Fugazza; Sergio Campana; P. A. Evans; P. W. A. Roming; E. Molinari; Richard G. Strom; Richard G. Strom; Valerio D'Elia; S. R. Oates; Xue-Feng Wu; Xue-Feng Wu; Katarzyna Małek; P. Oleynik; Stephen T. Holland; Stephen T. Holland; Adalberto Piccioni; J. P. Osborne; D. D. Frederiks; V. Mangano; M. Cwiok; C. Pagani; M. Perri; Malcolm N. Bremer; M. A. Garrett; M. A. Garrett; M. A. Garrett; Lech Wiktor Piotrowski; Aleksander Filip Zarnecki; Adriano Guarnieri; M. Ulanov; W. Dominik; A. de Ugarte Postigo; Andrew J. Levan; Vincenzo Testa;doi: 10.1038/nature07270
handle: 11245/1.301930 , 2381/25356 , 2381/42419 , 1959.3/47559 , 20.500.11937/15775
doi: 10.1038/nature07270
handle: 11245/1.301930 , 2381/25356 , 2381/42419 , 1959.3/47559 , 20.500.11937/15775
Long-duration gamma-ray bursts (GRBs) release copious amounts of energy across the entire electromagnetic spectrum, and so provide a window into the process of black hole formation from the collapse of massive stars. Previous early optical observations of even the most exceptional GRBs (990123 and 030329) lacked both the temporal resolution to probe the optical flash in detail and the accuracy needed to trace the transition from the prompt emission within the outflow to external shocks caused by interaction with the progenitor environment. Here we report observations of the extraordinarily bright prompt optical and gamma-ray emission of GRB 080319B that provide diagnostics within seconds of its formation, followed by broadband observations of the afterglow decay that continued for weeks. We show that the prompt emission stems from a single physical region, implying an extremely relativistic outflow that propagates within the narrow inner core of a two-component jet.
Nature arrow_drop_down Swinburne University of Technology: Swinburne Research BankArticle . 2008Data 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=10.1038/nature07270&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 436 citations 436 popularity Top 1% influence Top 1% impulse Top 0.1% Powered by BIP!
visibility 4visibility views 4 download downloads 207 Powered bymore_vert Nature arrow_drop_down Swinburne University of Technology: Swinburne Research BankArticle . 2008Data 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=10.1038/nature07270&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Other literature type 2010 United KingdomPublisher:Optica Publishing Group Kang Kang Chen; Shaif-ul Alam; J.H.V. Price; J. R. Hayes; Di Lin; A. Malinowski; Christophe A. Codemard; Debashri Ghosh; Mrinmay Pal; Shyamal K. Bhadra; David J. Richardson;Presentamos una fuente supercontinua bombeada con mopa de fibra de picosegundos con una salida de 39 W, que abarca al menos 0,4-2,25 micrómetros a una velocidad de repetición de 114,8 MHz. El PCF de 2 m de largo tenía un núcleo grande de 4,4 micrómetros de diámetro y un diseño de delta alto que condujo a una eficiencia de acoplamiento del 80%, un umbral de daño alto y una generación rápida de generación continua visible a partir de los pulsos de entrada de picosegundos. La densidad de potencia alta y relativamente uniforme a través de la región espectral visible fue de aproximadamente 31.7 mW/nm correspondiente a la densidad de potencia máxima de aproximadamente 12.5 W/nm para los pulsos de entrada de 21 ps. La densidad de potencia máxima se incrementó a 26,9 W/nm mediante la reducción de la tasa de repetición a 28 MHz. Esto representa un aumento en la potencia media y máxima en comparación con las fuentes de supercontinuo visibles informadas anteriormente de sistemas bombeados o pulsados CW. Nous rapportons une source de supercontinuum pompée MOPA à fibre picoseconde avec une sortie de 39 W, couvrant au moins 0,4-2,25 micromètres à un taux de répétition de 114,8 MHz. Le PCF de 2 m de long avait un grand noyau de 4,4 micromètres de diamètre et une conception à delta élevé qui a conduit à une efficacité de couplage de 80 %, à un seuil de dommage élevé et à une génération rapide de continuum visible à partir des impulsions d'entrée picosecondes. La densité de puissance élevée et relativement uniforme dans la région spectrale visible était d'environ 31,7 mW/nm, ce qui correspond à une densité de puissance de crête d'environ 12,5 W/nm pour les impulsions d'entrée de 21 ps. La densité de puissance de crête a été augmentée à 26,9 W/nm en réduisant le taux de répétition à 28 MHz. Cela représente une augmentation de la puissance moyenne et de crête par rapport aux sources de supercontinuum visibles précédemment rapportées provenant de systèmes pompés par ondes entretenues ou pulsés. We report a picosecond fiber MOPA pumped supercontinuum source with 39 W output, spanning at least 0.4-2.25 microm at a repetition rate of 114.8 MHz. The 2m long PCF had a large, 4.4 microm diameter core and a high-delta design which led to an 80% coupling efficiency, high damage threshold and rapid generation of visible continuum generation from the picosecond input pulses. The high and relatively uniform power density across the visible spectral region was approximately 31.7 mW/nm corresponding to peak power density of approximately 12.5 W/nm for the 21 ps input pulses. The peak power density was increased to 26.9 W/nm by reducing the repetition rate to 28 MHz. This represents an increase in both average and peak power compared to previously reported visible supercontinuum sources from either CW pumped or pulsed-systems. نبلغ عن مصدر فائق الاستمرارية لضخ ألياف بيكو ثانية مع خرج 39 واط، يمتد على الأقل 0.4-2.25 ميكروم بمعدل تكرار 114.8 ميجا هرتز. كان لـ PCF بطول 2 متر قلب كبير بقطر 4.4 ميكروم وتصميم عالي الدلتا مما أدى إلى كفاءة اقتران 80 ٪ وعتبة تلف عالية وتوليد سريع لتوليد سلسلة متصلة مرئية من نبضات إدخال البيكوثانية. كانت كثافة القدرة العالية والمنتظمة نسبيًا عبر المنطقة الطيفية المرئية حوالي 31.7 مللي واط/نانومتر المقابلة لكثافة القدرة القصوى التي تبلغ حوالي 12.5 واط/نانومتر لنبضات الإدخال 21 جزء في الثانية. تمت زيادة كثافة الطاقة القصوى إلى 26.9 واط/نانومتر عن طريق تقليل معدل التكرار إلى 28 ميجاهرتز. ويمثل هذا زيادة في كل من متوسط الطاقة وذروتها مقارنة بمصادر الاستمرارية المرئية التي تم الإبلاغ عنها سابقًا من أنظمة ضخ الأسلحة الكيميائية أو الأنظمة النبضية.
e-Prints Soton 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.
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=10.1364/oe.18.005426&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu112 citations 112 popularity Top 10% influence Top 1% impulse Top 1% Powered by BIP!
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