Structure of a fast coronal mass ejection from radio observations.

Details Structure of a fast coronal mass ejection from radio observations. Structure of a fast coronal mass ejection from radio observations.

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13r..75g&link_type=abstract

Advances in Space Research, Vol. 13, No. 9, p. 75 - 78

Computer Science

Scientific paper

The authors investigate the thermal structure of a coronal mass ejection (CME) in meter-dekameter wavelengths and compare it with the optical evidence. The multifrequency observations enable us to infer the three dimensional structure of the CME. The authors estimated the mass of the CME and found to be in reasonable agreement with the range of values obtained from white light observations.

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