Multispectral observations complementary to the study of high-energy solar phenomena

Details Multispectral observations complementary to the study of high-energy solar phenomena Multispectral observations complementary to the study of high-energy solar phenomena

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..118..209w&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 209-229.

Physics

4

Energetic Particles, Energy Spectra, Solar Flares, Solar Radiation, Particle Acceleration, Solar Atmosphere, Solar Maximum Mission

Scientific paper

Multispectral observations of phenomena associated with nonthermal events on the sun and characterized by the transient acceleration of electrons and ions to energies ranging from several keV to tens of GeV are discussed. It is shown that observations of the thermal and quasi-thermal phenomena preceeding, coinciding with, and following the impulsive acceleration and heating event itself can be used to study the evolution of magnetic structures in the solar convection zone and atmosphere. Observational techniques are discussed in detail.

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