Characteristics of nonstationary solar radio emission corresponding to CMEs formation in solar atmosphere

Details Characteristics of nonstationary solar radio emission corresponding to CMEs formation in solar atmosphere Characteristics of nonstationary solar radio emission corresponding to CMEs formation in solar atmosphere

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..373s&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Astronomy and Astrophysics

Astronomy

Solar Radio Emission, Cmes, Solar Atmosphere

Scientific paper

The results of analysis of solar radio emission during high solar activity coincided with CME's onset are presented. Observations of nonstationary radio emission corresponding to CME's formation and passage in the lower layers of solar atmosphere have been carried out at Radioastronopmical Observatory "Zimenki" (Russia) on 6 discrete wavelengths cm, dm and m range. The possibility of creation an algorithm to determine the formation of CMEs using solar radio observations in wide frequency range is shown.

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