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Scientific paper
Jun 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..495h&link_type=abstract
The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 495-497 (1999).
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3
Solar Wind Plasma, Sources Of Solar Wind, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays
Scientific paper
The charge state composition is a very sensitive measure for the electron properties at around 2 solar radii heliocentric distance. Even though the basic principle of the charge-state freeze-in process is rather well understood, it is not clear how the non-thermal properties of the electron distribution functions influence the frozen-in charge states. The obvious question to ask, then, is whether in situ electrons exhibit the same temporal variations as the charge state composition. Using SWICS/ACE and 3DP/WIND data, we find that the core electrons are dominated by local effects like compression and have no memory of their coronal origin. Supra-thermal electrons, on the other hand, show a clear correlation with the charge state data.
Fisk Len A.
Gloeckler George
Hefti Simon
Larson David
Lin Robert P.
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