Titlebook: Historisches Erz?hlen und Lernen; Historische, theoret Martin Buchsteiner,Martin Nitsche Book 2016 Springer Fachmedien Wiesbaden 2016 Gesch

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書目名稱Historisches Erz?hlen und Lernen影響因子(影響力)




書目名稱Historisches Erz?hlen und Lernen影響因子(影響力)學(xué)科排名




書目名稱Historisches Erz?hlen und Lernen網(wǎng)絡(luò)公開度




書目名稱Historisches Erz?hlen und Lernen網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Historisches Erz?hlen und Lernen被引頻次




書目名稱Historisches Erz?hlen und Lernen被引頻次學(xué)科排名




書目名稱Historisches Erz?hlen und Lernen年度引用




書目名稱Historisches Erz?hlen und Lernen年度引用學(xué)科排名




書目名稱Historisches Erz?hlen und Lernen讀者反饋




書目名稱Historisches Erz?hlen und Lernen讀者反饋學(xué)科排名

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Martin Nitsche,Martin Buchsteinerfacility will be available to all levels of experimenters — be they from small laboratories or large organisations — through the 1980s. A summary description of the Space Shuttle and Spacelab programmes is provided, to help the future user in the fields covered by this book, to better appreciate the

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Bodo von Borrieselatively weak component between 0.1 MK and 1 MK, (b) a dominant component somewhere between 2 MK and 10 MK, and (c) in all cases but one a component in the formal solution at temperatures exceeding ≈ 20 MK. Where this hot tail is not associated with a real hot component, it is a spurious result ref

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Martin Nitscherophysics.Includes discussions on the goals and the expected.This book discusses the state of the art of the basic theoretical and observational topics related to black hole astrophysics. It covers all the main topics in this wide field, from the theory of accretion disks and formation mechanisms of

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Martin Buchsteinerr transiting exoplanets three fundamental atmospheric measurements are possible: transmission spectra—where atmospheric absorption features are detected across an exoplanets limb during transit, emission spectra—where the day-side average emission of the planet is detected during secondary eclipse e

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Sven Güntherl means of expanding on this information is by spectroscopic study of atmospheres. To do this requires a knowledge of the spectroscopy of the molecules, present or likely to be present, in their atmosphere which in turn demands access to the extensive laboratory data that characterises these species

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