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   <subfield code="a">The &quot;fan” instability as a possible generating mechanism of vlf quarter-gyrofrequency emissions during the recovery phase of a magnetospheric storm</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[J. Bošková, P. Tříska, Yu. Omelchenko, V. Shapiro, V. Sotnikov]</subfield>
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   <subfield code="a">Summary: VLF quarter-gyrofrequency emissions, whose experimental characteristics differ from those of discrete plasmaspheric emissions usual during active times, have been observed by low-altitude Intercosmos 24 and Magion 2 satellites within the plasmasphere during periods of quieting geomagnetic activity. A new kind of instability is proposed which could lead to the production of these emissions. It is shown that quasi-electrostatic whistler waves can be generated in the eqquatorial region due to the fan instability, with maximum growth rate and spectral energy density in a frequency band below one half of the equatorial electron gyrofrequency. The observations of low-energy electrons and plasma waves in the equatorial region within or in the vicinity of the plasmapause, which could support our hypothesis experimentally, are discussed.</subfield>
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   <subfield code="a">Academia, Publishing House of the Czechoslorak Academy of Sciences, 1992</subfield>
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