Turbulent scattering of high-frequency radiation in accretion discs

Details Turbulent scattering of high-frequency radiation in accretion discs Turbulent scattering of high-frequency radiation in accretion discs

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...225..555l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 225, no. 2, Nov. 1989, p. 555-558.

Astronomy and Astrophysics

Astrophysics

1

Accretion Disks, Plasma Turbulence, Radiation Distribution, Compton Effect, Electrostatic Waves, Energy Dissipation

Scientific paper

The strong scattering effects by turbulent plasma on high-frequency radiation resulting from the Compton process are discussed. It is found that energy dissipation due to viscosity, as a source of Langmuir turbulent waves, could lead to form power-law spectra of high-frequency radiation. It is shown that the spectra index is an important factor in determining the atmosphere structure of accretion disks; when a specified condition is met, a high-temperature corona above the disk would appear.

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