Physics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsh33a..06r&link_type=abstract
American Geophysical Union, Spring Meeting 2007, abstract #SH33A-06
Physics
7509 Corona, 7513 Coronal Mass Ejections (2101), 7974 Solar Effects
Scientific paper
The radio receivers on the STEREO spacecraft provide the first dedicated remote stereoscopic observations of solar and interplanetary radio sources. These observations, from widely separated vantage points, together with simultaneous remote radio observations from Wind/WAVES and Ulysses/URAP, are expected to provide new information and insights about the 3D locations of these radio source regions, as well as their intrinsic radiation characteristics. The STEREO observations allow several ways of doing this, e. g., by using direction-finding techniques to triangulate and directly track the source locations and by using the complementary propagation- time differences. We present here preliminary results from the analysis of timing differences observed for solar type III radio bursts that are simultaneously observed by the two STEREO spacecraft and also by WIND/WAVES and Ulysses/URAP. We will examine how these timing differences vary with observing frequency and with the separation of the various spacecraft, particularly with the separation of the STEREO spacecraft.
Bougeret J-J.
Cecconi Baptiste
Fainberg Joe
Goetz Keith
Hoang Sang
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