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作者:Mai, Liqiang; Tian, Xiaocong; Zhao, Yunlong
作者单位:Wuhan University of Technology; Imperial College London; Imperial College London
摘要:Small electric aeroplanes flying at low altitude will need energy sources that can withstand crashes and deliver power reliably. Standards need to be decided now.
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作者:[Anonymous]
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作者:Assael, Yannis; Sommerschield, Thea; Cooley, Alison; Shillingford, Brendan; Pavlopoulos, John; Suresh, Priyanka; Herms, Bailey; Grayston, Justin; Maynard, Benjamin; Dietrich, Nicholas; Wulgaert, Robbe; Prag, Jonathan; Mullen, Alex; Mohamed, Shakir
作者单位:Alphabet Inc.; DeepMind; Google Incorporated; University of Nottingham; University of Warwick; Athens University of Economics & Business; Alphabet Inc.; Google Incorporated; University of Oxford
摘要:Human history is born in writing. Inscriptions are among the earliest written forms, and offer direct insights into the thought, language and history of ancient civilizations. Historians capture these insights by identifying parallels-inscriptions with shared phrasing, function or cultural setting-to enable the contextualization of texts within broader historical frameworks, and perform key tasks such as restoration and geographical or chronological attribution1. However, current digital metho...
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作者:Bi, Huixing; Sun, Daoyuan; Sun, Ningyu; Mao, Zhu; Dai, Mingwei; Hemingway, Douglas
作者单位:Chinese Academy of Sciences; University of Science & Technology of China, CAS; Chinese Academy of Sciences; University of Science & Technology of China, CAS; University of Texas System; University of Texas Austin
摘要:For rocky planets, the presence of a solid inner core has notable implications on the composition and thermal evolution of the core and on the magnetic history of the planet1, 2-3. On Mars, geophysical observations have confirmed that the core is at least partially liquid4, 5, 6-7, but it is unknown whether any part of the core is solid. Here we present an analysis of seismic data acquired by the InSight mission, demonstrating that Mars has a solid inner core. We identify two seismic phases, t...
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作者:Florczak, Sammy; Grossbacher, Gabriel; Ribezzi, Davide; Longoni, Alessia; Gueye, Marieme; Grandidier, Estee; Malda, Jos; Levato, Riccardo
作者单位:Utrecht University; Utrecht University Medical Center; Utrecht University
摘要:We introduce Generative, Adaptive, Context-Aware 3D Printing (GRACE), a new approach combining 3D imaging, computer vision and parametric modelling to create tailored, context-aware geometries using volumetric additive manufacturing. GRACE rapidly and automatically generates complex structures capable of conforming directly around features ranging from cellular to macroscopic scales with minimal user intervention. Here we demonstrate its versatility in applications ranging from synthetic objec...
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作者:Gidden, Matthew J.; Joshi, Siddharth; Armitage, John J.; Christ, Alina-Berenice; Boettcher, Miranda; Brutschin, Elina; Koberle, Alexandre C.; Riahi, Keywan; Schellnhuber, Hans Joachim; Schleussner, Carl-Friedrich; Rogelj, Joeri
作者单位:International Institute for Applied Systems Analysis (IIASA); University System of Maryland; University of Maryland College Park; IFP Energies Nouvelles; Utrecht University; Universidade de Lisboa; Potsdam Institut fur Klimafolgenforschung; Imperial College London; Humboldt University of Berlin; Humboldt University of Berlin; Imperial College London; Imperial College London
摘要:Geologically storing carbon is a key strategy for abating emissions from fossil fuels and durably removing carbon dioxide (CO2) from the atmosphere1,2. However, the storage potential is not unlimited3,4. Here we establish a prudent planetary limit of around 1,460 (1,290-2,710) Gt of CO2 storage through a risk-based, spatially explicit analysis of carbon storage in sedimentary basins. We show that only stringent near-term gross emissions reductions can lower the risk of breaching this limit bef...
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作者:[Anonymous]
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作者:Tupman, Charlotte
作者单位:University of Exeter
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作者:Zhang, Yulin; Zhang, Yi; Fang, Zezheng; Ni, Shilei
作者单位:Shandong University
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作者:Faherty, Jacqueline K.; Meisner, Aaron M.; Burningham, Ben; Visscher, Channon; Line, Michael; Suarez, Genaro; Gagne, Jonathan; Alejandro Merchan, Sherelyn; Rothermich, Austin James; Burgasser, Adam J.; Schneider, Adam C.; Caselden, Dan; Kirkpatrick, J. Davy; Kuchner, Marc Jason; Bardalez Gagliuffi, Daniella Carolina; Eisenhardt, Peter; Gelino, Christopher R.; Gonzales, Eileen C.; Marocco, Federico; Leggett, Sandy; Lodieu, Nicolas; Casewell, Sarah L.; Tremblin, Pascal; Cushing, Michael; Zapatero Osorio, Maria Rosa; Bejar, Victor J. S.; Gauza, Bartosz; Wright, Edward; Phillips, Mark W.; Zhang, Jun-Yan; Martin, Eduardo L.
作者单位:American Museum of Natural History (AMNH); City University of New York (CUNY) System; University of Hertfordshire; Arizona State University; Arizona State University-Tempe; Universite de Montreal; University of California System; University of California San Diego; California Institute of Technology; National Aeronautics & Space Administration (NASA); Amherst College; National Aeronautics & Space Administration (NASA); NASA Jet Propulsion Laboratory (JPL); California Institute of Technology; California State University System; San Francisco State University; Instituto de Astrofisica de Canarias; Universidad de la Laguna; University of Leicester; Universite Paris Saclay; CEA; Centre National de la Recherche Scientifique (CNRS); University System of Ohio; University of Toledo; Consejo Superior de Investigaciones Cientificas (CSIC); CSIC - Centro de Astrobiologia (INTA); University of Zielona Gora; University of California System; University of California Los Angeles; University of Edinburgh
摘要:Within 20 pc of the Sun, there are currently 29 known cold brown dwarfs-sources with measured distances and an estimated effective temperature between that of Jupiter (170 K) and approximately 500 K (ref. 1). These sources are almost all isolated and are the closest laboratories we have for detailed atmospheric studies of giant planets formed outside the Solar System. Here we report JWST observations of one such source, WISEA J153429.75-104303.3 (W1534), which we confirm is a substellar mass m...