Positively Drifting Structures During the 18 March 2003 Solar Flare

Details Positively Drifting Structures During the 18 March 2003 Solar Flare Positively Drifting Structures During the 18 March 2003 Solar Flare

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007soph..241...77n&link_type=abstract

Solar Physics, Volume 241, Issue 1, pp.77-84

Physics

3

Sun: Flares, Sun: Radio Radiation

Scientific paper

We analyze the high-frequency drift radio structures observed by the spectrometer at Purple Mountain Observatory (PMO) over the frequency range of 4.5 - 7.5 GHz during the 18 March 2003 solar flare. The drifting structures take place before the soft X-ray maximum, almost at the maximum of hard X-ray flux at 25 - 50 keV. For the first time, the positive drift in this kind of radio structures is detected in such a high frequency range. Their global drifting rate is roughly estimated as 3.6 GHz s-1. They appear in four groups, lasting in total for less than 6 s, and have a broad bandwidth of more than 2 GHz but a smaller ratio of the bandwidth of the drifting structures to mean frequency than that of the lower frequency range. The lifetime of each individual burst in this event can be derived by using the high temporal resolution of the spectrometer at PMO and has an average value of 36.3 ms. Since the negative drifting structures observed in the 0.6 - 4.5 GHz frequency range were interpreted to be a radio signature of a plasmoid ejected upward (moving out of the Sun), the present observation may imply that it is possible for a plasmoid to move downward during a solar flare. However, for a confirmation of this suggestion direct radio imaging observation would be needed.

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