Type III Solar Radio Bursts Observed by Multiple Spacecraft

Details Type III Solar Radio Bursts Observed by Multiple Spacecraft Type III Solar Radio Bursts Observed by Multiple Spacecraft

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh54c..05b&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH54C-05

Physics

Plasma Physics

[6954] Radio Science / Radio Astronomy, [7534] Solar Physics, Astrophysics, And Astronomy / Radio Emissions, [7863] Space Plasma Physics / Turbulence, [7868] Space Plasma Physics / Wave/Wave Interactions

Scientific paper

Type III solar radio bursts, which are excited by electron beams accelerated by solar flares, are often simultaneously observed by multiple widely separated spacecraft. We analyze the simultaneous observations of major type III radio bursts obtained by the STEREO A, STEREO B, and Wind spacecraft from October 2006 to date, studying characteristics such as frequency drifts, intensities, time delays, and fundamental harmonic structures. This will enable us to determine the relationships between the speed of type III associated electron beams, intensities and time delays of type III radio bursts, and relative longitudes of the spacecraft.

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