Other
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.1295h&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 19, no. 12, June 19, 1992, p. 1295-1298. Research supported by CNES and CNRS
Other
20
Electron Density (Concentration), Solar Electrons, Solar Wind, Ulysses Mission, Ecliptic, Hot Electrons, Noise Spectra, Radio Receivers, Solar Radio Emission
Scientific paper
The radio receiver of the Unified Radio and Plasma experiment aboard the Ulysses spacecraft records spectra of the quasi-thermal plasma noise. The interpretation of these spectra allows the determination of the total electron density Ne and of the cold (core) electron temperature Tc in the solar wind. A single power law does not fit the variations of Ne which result from the contribution from different solar wind structures. The distribution of the values of Tc suggests that, on the average, the solar wind is nearly isothermal.
Bougeret Jean-Louis
Harvey Chris
Hoang Sang
Lacombe Catherine
Macdowall Robert J.
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