An effect of stimulated radiation processes on radio emission from major planets

Details An effect of stimulated radiation processes on radio emission from major planets An effect of stimulated radiation processes on radio emission from major planets

2004-01-20

arxiv.org/abs/astro-ph/0401382v1

Astronomy and Astrophysics

Astrophysics

2 pages, LaTeX 2e, submitted to 35th Lunar and Planetary Science Conference

Scientific paper

The standard theory of thermal radio emission encounters some difficulties. The most crucial one is nonpossibility to explain the radio spectrum of Venus in the decimeter range (Ksanfomality 1985). The radio spectra of planetary nebulae at high frequencies also are not comfortably consistent with the standard theory (Siodmiak & Tylenda 2001). Here we show that the account for an induced character of radiation processes sufficiently improves the predictions of the standard theory.

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