Inverse Compton reflection - Time-dependent theory
We consider time-dependent behavior in inverse Compton reflection, in which an external flux of soft photons is incident upon a hot, thermal plasma of large scattering depth and small absorption depth. Fluctuations are assumed to arised from variability in the input of solf photons. Our treatment is...
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Veröffentlicht in: | Astrophys. J.; (United States) 1979-09, Vol.232, p.882 |
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container_title | Astrophys. J.; (United States) |
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creator | Lightman, A. P. Rybicki, G. B. |
description | We consider time-dependent behavior in inverse Compton reflection, in which an external flux of soft photons is incident upon a hot, thermal plasma of large scattering depth and small absorption depth. Fluctuations are assumed to arised from variability in the input of solf photons. Our treatment is largely analytic. We calculate in detail the spectral evolution during a fluctuation and show how such observables as the frequency-dependent rise time and the spectral hardness ratio may be used to derive the plasma parameters and soft photon frequency, or perhaps rule out an inverse Compton model altogether. Some of the results are qualitatively applicable to inverse Compton processes in general. Such considerations may be relevant to models for rapidly fluctuating X-ray sources. |
doi_str_mv | 10.1086/157350 |
format | Article |
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B.</creator><creatorcontrib>Lightman, A. P. ; Rybicki, G. B. ; Harvard-Smithsonian Center for Astrophysics</creatorcontrib><description>We consider time-dependent behavior in inverse Compton reflection, in which an external flux of soft photons is incident upon a hot, thermal plasma of large scattering depth and small absorption depth. Fluctuations are assumed to arised from variability in the input of solf photons. Our treatment is largely analytic. We calculate in detail the spectral evolution during a fluctuation and show how such observables as the frequency-dependent rise time and the spectral hardness ratio may be used to derive the plasma parameters and soft photon frequency, or perhaps rule out an inverse Compton model altogether. Some of the results are qualitatively applicable to inverse Compton processes in general. 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P.</creatorcontrib><creatorcontrib>Rybicki, G. B.</creatorcontrib><creatorcontrib>Harvard-Smithsonian Center for Astrophysics</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lightman, A. P.</au><au>Rybicki, G. B.</au><aucorp>Harvard-Smithsonian Center for Astrophysics</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Inverse Compton reflection - Time-dependent theory</atitle><jtitle>Astrophys. 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subjects | 70 PLASMA PHYSICS AND FUSION TECHNOLOGY 700108 - Fusion Energy- Plasma Research- Wave Phenomena BASIC INTERACTIONS COMPTON EFFECT COSMIC RAY SOURCES COSMIC X-RAY SOURCES ELASTIC SCATTERING ELECTROMAGNETIC INTERACTIONS FLUCTUATIONS FLUID MECHANICS FUNCTIONS GREEN FUNCTION HOMOGENEOUS PLASMA HOT PLASMA HYDRODYNAMICS INTERACTIONS INVERSE SCATTERING PROBLEM MECHANICS PLASMA SCATTERING TIME DEPENDENCE VARIATIONS |
title | Inverse Compton reflection - Time-dependent theory |
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