Physics
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984stin...8518935p&link_type=abstract
Unknown
Physics
Electron Distribution, Helios Satellites, Solar Wind, Angular Resolution, Ecliptic, Electron Energy, Electron Flux Density, Solar Flux Density, Temporal Resolution
Scientific paper
Methods to derive distribution functions for solar wind electrons from the measurements of the plasma experiment aboard the HELIOS probes are outlined. Electrons are measured in the energy range from 0.5 to 1660 eV with one-dimensional angular resolution along the ecliptic plane. From these measurements electron distribution functions with high time resolution (18 sec) but poor angular resolution in velocity space (45 deg) and electron distribution functions with high angular resolution ( 5 to 10 deg) but poor time resolution (several minutes to few hours) are derived.
Miggenrieder H.
Muehlhaeuser K.-H.
Pilipp Werner G.
Rosenbauer Helmut
Schuwen R.
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