The solar radio corona: Manifestations of energetic electrons

Details The solar radio corona: Manifestations of energetic electrons The solar radio corona: Manifestations of energetic electrons

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sfcp.nasa..159p&link_type=abstract

In NASA. Marshall Space Flight Center Solar Flares and Coronal Physics Using P/OF as a Research Tool p 159-177 (SEE N86-24614

Physics

Energy Transfer, Particle Acceleration, Solar Corona, Solar Flares, Solar Radio Emission, Solar X-Rays, Electromagnetic Radiation, Impulses, Interplanetary Medium, Spectroheliographs

Scientific paper

Radio observations are powerful tools which are complementary to the space missions devoted to the physics of the flares, of the corona, or of the interplanetary medium. To undertake this task two multifrequency radioheliographs presently exist: the Nancay instrument (the multifrequency facility will be in operation by the end of 1985) observes the middle corona at decimeter-meter wavelengths, and the Clark Lake radioheliograph, operating at decameter wavelengths, is the only one in the world to have the ability of observing the outer corona above the disk.

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