Preliminary Analysis of Type III Radio Bursts from Stereo/Waves Data

Details Preliminary Analysis of Type III Radio Bursts from Stereo/Waves Data Preliminary Analysis of Type III Radio Bursts from Stereo/Waves Data

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009pobeo..86..287v&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 86, pp. 287-291

Astronomy and Astrophysics

Astronomy

Scientific paper

Solar Type III radio observations in the range 125 kHz - 16 025 kHz from the STEREO/Waves experiment have been preliminary analyzed. These bursts are generated by energetic electrons traveling away from the Sun along open magnetic field lines. A subset of 88 burst has been selected for this study. The dependence of the observed intensity radiation as a function of time at given frequency has been fitted with a Gram-Charlier type A function. The flux density spectra for all the selected type III radio bursts at each frequency channel have been determined. This preliminary analysis gives an empirical expression for the frequency drift rate as a function of frequency for the type III radio bursts.

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