2004/01/20 by Fedor V. Prigara, F. V. Prigara, Prigara, F. V.
Physics and Astronomy · #Astro and Planetary Science #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Planetary Science and Exploration #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0401382
2 pages, LaTeX 2e, submitted to 35th Lunar and Planetary Science Conference
arxiv created 2004/01/20 · openalex publication_date 2004/01/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.