The apparent source size of type III radio bursts: Preliminary results by the STEREO/WAVES instruments

Details The apparent source size of type III radio bursts: Preliminary results by the STEREO/WAVES instruments The apparent source size of type III radio bursts: Preliminary results by the STEREO/WAVES instruments

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..284k&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 284-287 (2010).

Computer Science

Solar Wind, Interplanetary Magnetic Fields, Solar Corona, Solar Flares, Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Coronal Mass Ejection, Flares

Scientific paper

The S/WAVES instrument onboard the STEREO spacecraft measures electromagnetic waves in the solar wind. This unique project allows us to investigate properties of type III and type II radio bursts related to solar flares and propagation of coronal mass ejections (CMEs) in the interplanetary medium, respectively. We have focused on the High Frequency Receiver (HFR a part of the STEREO/WAVES instrument) which covers the frequency range 125 kHz~16.025 MHz. We present first results of a goniopolarimetric inversion for an extended source using the Singular Value Decomposition technique (SVD). We show a joint observation (including the WIND spacecraft) of the single type III radio burst connected with the X flare as a preliminary example of estimation of the apparent source size and its position.

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