The analysis for the symmetry of solar radio pulsations at short centimetric bands.

Details The analysis for the symmetry of solar radio pulsations at short centimetric bands. The analysis for the symmetry of solar radio pulsations at short centimetric bands.

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acasn..34..273h&link_type=abstract

Acta Astron. Sin., Vol. 34, No. 3, p. 273 - 278

Astronomy and Astrophysics

Astronomy

Scientific paper

A statistical analysis for the symmetry of solar radio pulsations at short centimetric bands is given. At first, it is proved theoretically that the decay time-scale of a single pulse is approximately proportional to its rise time-scale, hence, the expected time-scale at decay phase is inversely proportional to the radio burst flux, the modularity at decay phase of a single pulse decreases with increasing the radio burst flux, and increases with increasing the decay time, and etc. There is a statistical unsymmetry for the contour of the pulsations. Therefore, the pulsations at short centimetric bands may be excited by a plasma instability.

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