The precursors of the 9 July 1982 solar proton flare event

Details The precursors of the 9 July 1982 solar proton flare event The precursors of the 9 July 1982 solar proton flare event

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..149z&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 149-152 (SEE N89-24974 1

Computer Science

Protons, Solar Flares, Solar Spectra, H Alpha Line, Solar Oscillations, Solar Prominences, Solar X-Rays

Scientific paper

Observational evidence is presented that radio precursors of a big flare event cover the whole microwave-decimeter range like the following impulsive phase. The quasiperiodic preflare radio emission combined with soft and hard X-ray and H-alpha data confirms preflare energization of the active region and is compatible with a temperature dependent prominence flare loop interaction model. The preflare signatures are highly important for a preflare diagnostic of energy release site parameters.

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