Characteristics of the fine structures in solar radio bursts at 3.2 cm

Details Characteristics of the fine structures in solar radio bursts at 3.2 cm Characteristics of the fine structures in solar radio bursts at 3.2 cm

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..339q&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 3, p. 339-346.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We briefly describe the results of observation of radio fine structures
at 3 cm by the Department of Astronomy, Nanjing University in the years
1989-1992. We point out that there are three kinds of fine structure and
briefly discuss possible mechanisms for their generation.

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