Solar Wind Plasma Experiment on Solar Orbiter: dealing with the need for a sufficient phase-space resolution

Details Solar Wind Plasma Experiment on Solar Orbiter: dealing with the need for a sufficient phase-space resolution Solar Wind Plasma Experiment on Solar Orbiter: dealing with the need for a sufficient phase-space resolution

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..822d&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 822-8

Physics

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

Solar Orbiter is proposed as a space mission dedicated to study the solar surface, the corona and the solar wind by means of remote sensing and in-situ measurements, respectively. At 0.21 AU, closest approach to the Sun, the full 3-D particle velocity distribution should be sampled as fast as a few tens of msec in order to study the growth phase of the instabilities. This implies some restrictions on the maximum phase space resolution given the limited allowed bit-rate for data transmission. In this paper we evaluate consequences of this limitation for solar wind distributions with different parameters.

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