Microwave fine structures in 1-7.6 GHz range and associated dynamic processes

Details Microwave fine structures in 1-7.6 GHz range and associated dynamic processes Microwave fine structures in 1-7.6 GHz range and associated dynamic processes

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..375y&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Sun: Radio Radiation, Sun: Corona, Sun: Activity

Scientific paper

In this paper, the data observed by Solar Radio Broadband Spectrometer at Huairou Station, National Astronomical Observatories, Chinese Academy of Sciences are presented. With very high temporal and spectral resolutions in a broadband frequency range, the radio dynamic spectra of fast fine structures in microwave bursts offer a significant means for the diagnosis of energy releases and particle accelerations. Their implications as compared with other observations are discussed as well.

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