The behavior of distant heliospheric pick-up ions and associated solar wind heating

Details The behavior of distant heliospheric pick-up ions and associated solar wind heating The behavior of distant heliospheric pick-up ions and associated solar wind heating

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...202..295f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 202, no. 1-2, Aug. 1988, p. 295-305.

Astronomy and Astrophysics

Astrophysics

36

Heliosphere, Ion Motion, Plasma-Particle Interactions, Solar Wind, Wave Interaction, Cold Plasmas, Energy Transfer, Plasma Turbulence, Solar Heating, Space Plasmas

Scientific paper

Recently, very exciting observations of pick-up ions in the solar wind that are due to cometary or interstellar origin could be made for the first time (e.g. by Möbius et al. 1985 - 1987), proving the existence of such ions. Although theory has dealt with these exotic ions for more than a decade, no conclusive, clear-cut picture of their behavior in phase and configuration space was offered up to now. The authors therefore reanalyse this problem starting from a very general basis and in particular they aim at the question whether or not interstellar pick-up ions can heat the bulk of the distant solar wind.

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