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

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dc.creatorPrigara, F. V.
dc.date2004-01-20
dc.date.accessioned2026-07-07T02:11:56Z
dc.date.available2026-07-07T02:11:56Z
dc.descriptionThe 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.
dc.description2 pages, LaTeX 2e, submitted to 35th Lunar and Planetary Science Conference
dc.identifierhttps://arxiv.org/abs/astro-ph/0401382
dc.identifierhttp://arxiv.org/abs/astro-ph/0401382
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7279
dc.subjectAstrophysics
dc.titleAn effect of stimulated radiation processes on radio emission from major planets
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