... This matter may absorb the radiation from the source, scatter it or in fact emit fur ther radiation. ... For the case of a homogeneous cloud with a constant source function and optical depth with initial incident intensity , the emergent intensity is This makes a lot of sense: the emergent radiation is the sum of the incident intensity attenuated by the total optical depth plus the sum of each section of cloud emission attenuated by the optical ...
... High Energy Astrophysics: Emission and Absorption 1/114 HST optical image of 3C273 Note the very strong central point source and the less luminous jet. ... 4 I n 2 F = d B ( T ) cos sin d = B ( T ) 0 0 High Energy Astrophysics: Emission and Absorption 16/114 6 The Einstein relations 6.1 Definition of the Einstein coefficients These relations are arrived at in a similar manner to Kirchhoff's law via the inclusion of a new process stimulated emission. ... They are separated in energy by h . ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/7_Emission_and_Absorption.pdf -- 1698.7 Кб -- 27.05.2003 Похожие документы
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