The 3-D solar radioastronomy and the structure of the corona and the solar wind

Details The 3-D solar radioastronomy and the structure of the corona and the solar wind The 3-D solar radioastronomy and the structure of the corona and the solar wind

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ssim.conf...65s&link_type=abstract

In NASA. Goddard Space Flight Center Proc. of the Symp. on the Study of the Sun and Interplanetary Medium in Three Dimensions

Astronomy and Astrophysics

Astronomy

Radio Astronomy, Solar Activity, Solar Corona, Solar Probes, Solar Radio Bursts, Solar Wind, Solar Magnetic Field, Solar Physics, Stereoscopy

Scientific paper

The mechanism causing solar radio bursts (1 and 111) is examined. It is proposed that a nonthermal energy source is responsible for the bursts; nonthermal energy is converted into electromagnetic energy. The advantages are examined for an out-of-the-ecliptic solar probe mission, which is proposed as a means of stereoscopically viewing solar radio bursts, solar magnetic fields, coronal structure, and the solar wind.

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