Relative timing of microwave bursts and metric type III bursts - Implication on the energy of type III burst exciter

Details Relative timing of microwave bursts and metric type III bursts - Implication on the energy of type III burst exciter Relative timing of microwave bursts and metric type III bursts - Implication on the energy of type III burst exciter

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..125r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 120, no. 1, 1989, p. 125-136.

Physics

7

Electron Acceleration, Microwave Emission, Type 3 Bursts, Solar Corona, Wave Propagation

Scientific paper

The propagation speed of the exciter of solar type III bursts is derived from observations with high space and time resolution at 22 GHz and 169 MHz. A survey of an active region during two successive days revealed a high degree of association between microwave and type III bursts. From a detailed investigation of their location and timing, which requires neither a coronal density model nor the assumption of radial propagation, the exciter is found to propagate at a speed above at least 0.6c, i.e., much faster than the commonly cited value of c/3. Type III bursts in the dm-m wave band, hence, may reveal the energization of electrons up to energies far above 100 keV.

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