What should be observed on the sun

Details What should be observed on the sun What should be observed on the sun

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...47..375s&link_type=abstract

(NASA, IAU, IUGG, and International Council of Scientific Unions, Workshop on Flare Build-up Study, Falmouth, Mass., Sept. 8-11,

Physics

3

Magnetic Field Configurations, Magnetic Variations, Solar Activity Effects, Solar Flares, Solar Magnetic Field, Velocity Distribution, Far Ultraviolet Radiation, High Resolution, Magnetic Effects, Particle Acceleration, Radiant Flux Density, Solar Corona

Scientific paper

Three problems are emphasized in particular: the preflare magnetic field configuration, velocity fields, and the nature of acceleration processes in flares. It is concluded that what we need most urgently are high-resolution hard X-ray, soft X-ray, and EUV-pictures, coronal spectra, and magnetograms with high resolution both in space and time. A space-shuttle equipped with instrumentation of this kind would contribute significantly to our knowledge of the flare process.

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