Science with the Solar and Heliospheric Observatory (SOHO)

Details Science with the Solar and Heliospheric Observatory (SOHO) Science with the Solar and Heliospheric Observatory (SOHO)

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..177h&link_type=abstract

In ESA The Hydromagnetics of the Sun p 177-183 (SEE N85-25091 14-92)

Physics

European Space Programs, Heliosphere, Soho Mission, Solar Observatories, Solar Physics, Helioseismology, Plasma Diagnostics, Plasma Temperature, Solar Corona, Solar Wind, Spaceborne Experiments, Stellar Structure

Scientific paper

Use of the Solar and Heliospheric Observatory to study the interior structure of the Sun, the heating of the corona and its expansion as solar wind are discussed. The observations needed to pursue these questions will be taken from a halo orbit around Lagrange point L1 on the Earth-Sun line, which offers uninterrupted observations of the Sun and (lying outside the magnetosphere) solar wind streams. The payload includes helioseismology, optical plasma diagnostics of the corona at extreme ultraviolet and visible wavelengths, and in-situ particle and field measurements.

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