Aspects of the observation of solar-flare phenomena

Details Aspects of the observation of solar-flare phenomena Aspects of the observation of solar-flare phenomena

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..161p&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, June 1977, p. 161-196. In Italian.

Astronomy and Astrophysics

Astronomy

Solar Flares, Solar Radiation, Solar Spectra, Solar X-Rays, Spaceborne Astronomy, Far Ultraviolet Radiation, H Alpha Line, Microwave Emission, Particle Acceleration, Radiant Flux Density, Solar Corpuscular Radiation, Solar Magnetic Field, Solar Radio Emission, Type 3 Bursts, Visual Observation, X Ray Astronomy

Scientific paper

A review is presented of electromagnetic and particle emission from solar flares, with particular emphasis on relationships between characteristic features of flares in different spectral bands. Three main phases in the development of a typical event are identified: precursor, pulsed, and gradual. The association of hard X-ray bursts with pulsed EUV and microwave bursts as well as with pulsed optical phenomena and type III bursts is discussed. Considerable attention is given to magnetic fields associated with flares and to the location of sources of different types of emission with respect to the magnetic field structure.

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