A kind of spikes excited by chromospheric ejection during the eruptive prominence period.

Details A kind of spikes excited by chromospheric ejection during the eruptive prominence period. A kind of spikes excited by chromospheric ejection during the eruptive prominence period.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pbeio..21...29x&link_type=abstract

Publications of the Beijing Astronomical Observatory, No. 21, p. 29 - 32

Astronomy and Astrophysics

Astronomy

Solar Chromosphere: Solar Prominences

Scientific paper

On May 13, 1991 the authors used the high resolution acoustic-optical spectrometer to observe spike groups which relate to eruptive prominence and type II radio burst during no flare period on the solar disk. In this paper, the frequency characteristics and time profiles of the spikes that associate with the ejection process of eruptive prominence is discussed.

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