Physics
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..129m&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 129-1
Physics
78
Shock Waves, Solar Corona, Solar Radio Bursts, Solar Radio Emission, Spectrographs, Polarimeters, Soho Mission, Space Observations (From Earth)
Scientific paper
A radiospectrograph to observe the radioemission of the Sun in the range between 40 up to 800 MHz is described. In contrast to previous radiospectrographs, it consists of three different components: 4 sweep spectrographs, a grid of 14 single frequency polarimeters, and a multichannel spectrograph. Therefore, the instrument is able to observe the solar radio radiation with a very high spectral and temporal resolution up to a height of 2 solar radii and, thus, to provide important ground based observations to the SOHO (Solar and Heliospheric Observatory) mission. Observations of solar type 2 radio bursts by this instrument are presented with the aim of discussing some problems of the physical nature of coronal shock waves.
Aurass Henry
Mann Gottfried
Paschke Jens
Voigt W.
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