An indication for an intrinsically different coronal temperature

Details An indication for an intrinsically different coronal temperature An indication for an intrinsically different coronal temperature

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85..443g&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 443-449.

Astronomy and Astrophysics

Astrophysics

1

Solar Corona, Solar Temperature, Solar Wind, Helios Satellites, Interplanetary Magnetic Fields, Solar Magnetic Field, Solar Protons, Temperature Gradients

Scientific paper

Because the IMF is an extension of the solar magnetic field, and the solar wind is an extension of the solar corona, knowledge of these two interplanetary structures reflects knowledge of the solar corona itself. Calculations of the radial proton temperature gradients within magnetic sector boundaries observed by the Helios-1 and -2 heliocentric satellites between 0.3 and 1.0 AU have revealed lower temperatures in the solar corona, in the region where the magnetic sector boundaries merge.

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