Computer Science
Scientific paper
Jan 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stin...9926289h&link_type=abstract
Technical Report, IAC 1997: International aerospace congress Office of Energy Research
Computer Science
Solar Probes, Atmospheric Effects, Solar Activity, In Situ Measurement, Solar Corona, Solar Wind, Heliosphere, Ion Distribution, Electron Distribution, Plasma Waves, Energetic Particles, Sun, Velocity Distribution, Plasma Diagnostics, Spacecraft
Scientific paper
The solar corona is the source of solar wind that leads to the existence of the heliosphere and plays a crucial role in solar terrestrial phenomena. A comprehensive understanding of these phenomena can be provided only by directly measuring ion and electron velocity distributions, plasma waves, and fluxes of energetic particles. The problem presented by the inherent atmosphere of a spacecraft moving in the vicinity of the sun (4--20)R(circle-dot) and its influence on in-situ measurements of the solar corona plasma is the key to the realization and success of any solar probe mission. Models are developed to study and evaluate the effect of the inherent atmosphere on the in-situ measurements of future solar probes.
Alekseev Vladimir A.
Hassanein A.
Konkashbaev A. I.
Konkashbaev I. K.
Nikandrov L. B.
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