Micro-type III Radio Bursts as Observed in Kilometer Wavelength

Details Micro-type III Radio Bursts as Observed in Kilometer Wavelength Micro-type III Radio Bursts as Observed in Kilometer Wavelength

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007asthe.100..272m&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 100, No. 6, p. 272 - 279 (2007)

Astronomy and Astrophysics

Astronomy

Radio Bursts

Scientific paper

Micro-type III radio bursts are characterized by short-lived, continuous, and weak emissions. The occurrence distribution of these bursts with respect to the emitted power flux is different from that of ordinary type III bursts, indicating that they are not just the weaker components of the ordinary bursts. We found that both micro and ordinary type-III bursts emanated from the same active region without interference, indicating the coexistence of independent electron acceleration processes. It has been suggested that the active regions responsible for micro-type-III bursts border the coronal holes.

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