The solar probe mission

Details The solar probe mission The solar probe mission

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203..101f&link_type=abstract

Particle astrophysics. AIP Conference Proceedings, Volume 203, pp. 101-110 (1990).

Astronomy and Astrophysics

Astrophysics

2

Particle Emission, Solar Wind

Scientific paper

The Solar Probe will deliver a 133.5 kg science payload into a 4 Rs perihelion solar polar orbit (with the first perihelion passage in 2004) to explore in situ one of the last frontiers in the solar system-the solar corona. This mission is both affordable and technologically feasible. Using a payload of 12 (predominantly particles and fields) scientific experiments, it will be possible to answer many long-standing, fundamental problems concerning the structure and dynamics of the outer solar atmosphere, including the acceleration, storage, and transport of energetic particles near the Sun and in the inner (<65 Rs) heliosphere.

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