Multiple radio echoes in the solar corona

Details Multiple radio echoes in the solar corona Multiple radio echoes in the solar corona

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...91..383a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 91, April 1984, p. 383-398.

Physics

8

Radio Echoes, Solar Corona, Solar Radio Bursts, Temporal Distribution, Time Lag

Scientific paper

In the echo-type solar radio bursts associated with preceding, short-lived bursts in double events, as in the present decameter echoes, an initial narrow band burst is followed after 5-10 sec by an echo-like burst of the same frequency. Intensity-time profiles of 25 MHz echo bursts are noted to have an extended leading edge and an abrupt decay at the trailing edge. Time parameters characterizing the profiles are evaluated, and the causes and conditions for multiple echo formation are discussed. The extended leading edge of the echo suggests that one may assume a quasi-radial fibrous structure in the corona which is capable of backscattering the incident radiation.

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