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Titlebook: Laboratory Astrophysics ; Guillermo M. Mu?oz Caro,Rafael Escribano Book 2018 Springer International Publishing AG, part of Springer Natur

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發(fā)表于 2025-3-21 20:07:04 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Laboratory Astrophysics
編輯Guillermo M. Mu?oz Caro,Rafael Escribano
視頻videohttp://file.papertrans.cn/581/580283/580283.mp4
概述Provides a quick entry into laboratory astrophysics and astrochemistry.Presents fundamentals of main laboratory astrophysical techniques: spectroscopy, scattering, theoretical models.Gives detailed de
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Laboratory Astrophysics		;  Guillermo M. Mu?oz Caro,Rafael Escribano Book 2018 Springer International Publishing AG, part of Springer Natur
描述This book focuses on the most recent, relevant, comprehensive and significant aspects in the?well-established multidisciplinary field Laboratory Astrophysics. It focuses on astrophysical environments, which include asteroids, comets, the interstellar medium, and circumstellar and circumplanetary regions. Its scope lies between physics and chemistry, since it explores physical properties of the gas, ice, and dust present in those systems, as well as chemical reactions occurring in the gas phase, the bare dust surface, or in the ice bulk and its surface. Each chapter provides the necessary mathematical background to understand the subject, followed by a case study of the corresponding system.?.The book provides adequate material to help interpret the observations, or the computer models of astrophysical environments. It introduces and describes the use of spectroscopic tools for laboratory astrophysics. This book is mainly addressed to PhD graduates working in thisfield or observers and modelers searching for information on ice and dust processes..
出版日期Book 2018
關(guān)鍵詞Dust, ice, grain mantles; Interstellar medium; Light scattering, infrared techniques, plasmas; Cosmic d
版次1
doihttps://doi.org/10.1007/978-3-319-90020-9
isbn_softcover978-3-030-07916-1
isbn_ebook978-3-319-90020-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing AG, part of Springer Nature 2018
The information of publication is updating

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發(fā)表于 2025-3-22 00:04:34 | 只看該作者
Infrared Optical Constants and Band Strengths of Icesin astrophysical media. In this chapter we describe different experimental ways to obtain these magnitudes. They are based on infrared transmission absorption spectra of ice layers grown on infrared transparent substrates. The main approximations implicit in the procedures are reviewed.
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發(fā)表于 2025-3-22 09:36:38 | 只看該作者
Light Scattered by Cosmic Dust at Visible Wavelengthseres. In this chapter, the methodology of these measurements is explained through the presentation of an optical laboratory, its theoretical background, the calibration procedures and some applied examples.
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發(fā)表于 2025-3-22 14:34:49 | 只看該作者
Infrared Spectroscopy of Ions of Astrophysical Interestn survive for relatively long times due to the few collisions they suffer. On earth, molecular ions are “exotic” species much more difficult to produce in appreciable quantities. Electrical discharges in low pressure gases form cold plasmas which can be used to produce molecular ions in abundances high enough to enable their spectroscopic study.
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發(fā)表于 2025-3-22 19:39:08 | 只看該作者
Thermal Reactivity Dynamics in Interstellar Icelimited by UV or cosmic rays fluxes or the scarcity of radicals on the surface because they involve only dominant mantle molecules. Thermal reactions represent an important step in the formation of complex organic molecules that constitute the primitive material of comets and asteroids.
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發(fā)表于 2025-3-23 01:01:06 | 只看該作者
Book 2018physics. It focuses on astrophysical environments, which include asteroids, comets, the interstellar medium, and circumstellar and circumplanetary regions. Its scope lies between physics and chemistry, since it explores physical properties of the gas, ice, and dust present in those systems, as well
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發(fā)表于 2025-3-23 04:12:19 | 只看該作者
Interstellar Chemical Modelstellar cloud, describes which are the basic physical and chemical data needed to feed the model, and briefly discuss how these models assist in the interpretation of astronomical observations of molecules.
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發(fā)表于 2025-3-23 05:57:24 | 只看該作者
0067-0057 ectroscopy, scattering, theoretical models.Gives detailed deThis book focuses on the most recent, relevant, comprehensive and significant aspects in the?well-established multidisciplinary field Laboratory Astrophysics. It focuses on astrophysical environments, which include asteroids, comets, the in
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