Physics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh32a0784h&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH32A-0784
Physics
7509 Corona, 7513 Coronal Mass Ejections (2101), 7514 Energetic Particles (2114), 7531 Prominence Eruptions, 7984 Space Radiation Environment
Scientific paper
The radio receivers on the Wind spacecraft (4-13825 kHz) and Ulysses spacecraft (1.25-940 kHz) have continuously observed radio and plasma waves in the interplanetary medium. In the present paper, we shall focus on the solar radio emissions that are generated by flare suprathermal electrons (type III bursts) and by Interplanetary Coronal Mass Ejection (ICME) related shocks (type II bursts), and on the plasma quasi-thermal noise which constitutes the limit background of all radio observations in space. We shall present some examples of simultaneous observations by Ulysses and Wind of type II emissions (radio tracking of ICME driven shocks), of type III bursts (emission mode, localization, directivity), and of plasma thermal noise (solar wind diagnostics).
Bonnin Xavier
Bougeret J-J.
Hoang Sang
Issautier Karine
Maksimovic Milan
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