Comparative analysis of loss-cone instabilities in the coronae of the Sun and stars

1Stepanov, AV, 2Tsap, YT
1Main Astronomical Observatory of the Russian Academy of Sciences, St. Petersburg, Russia
2Scientific-Research Institute «Crimean Astrophysical Observatory» of the Ministry for Education and Science of Ukraine, Nauchny, Crimea, Ukraine
Kosm. nauka tehnol. 2003, 9 ;(5-6):144-146
Publication Language: Russian
In a cold plasma approximation the excitation of electromagnetic and electrostatic waves by anisotropic electrons is considered. It was shown that whistlers are excited in the coronae of the Sun and stars most effectively. Results of this work may be used for the flare plasma diagnostics.
Keywords: cold plasma, flare plasma diagnostics, Sun's corona
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