Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...294..587f&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 294, no. 2, p. 587-600
Astronomy and Astrophysics
Astrophysics
42
Heliosphere, Hydrogen, Interstellar Gas, Oxygen, Shock Waves, Solar Wind, Space Plasmas, Cosmic Rays, Ulysses Mission
Scientific paper
Connected with the relative motion of the solar system with respect to the ambient interstellar medium is a series of qualitatively different physical influences on both the subsonic interstellar and the subsonic solar wind plasma regimes. These regimes form a region characterized by a perturbed interface or heliosheath plasma ahead of the solar system which interstellar neutrals have to penetrate prior to their arrival at the inner solar system. As is shown quantitatively here the distribution functions of neutral interstellar gas species in the heliosphere have experienced typical gas-specific imprints from this perturbed plasma region. In this paper we are especially interested in the influence of the interface plasma on the oxygen-to-hydrogen ratio since observational facts from pick-up ion and anomalous cosmic ray observations have now become available that shrink down the inaccuracy in the knowledge of this ratio to much lower numbers. Our aim is to study this ratio for different possible interface structures and to compare the result with the available data in order thereby to identify the best fitting interface. From our calculations it becomes evident that satisfactory theoretical representations of the most recent pick-up-ion data from ULYSSES can only be given if the local interstellar medium is partially ionized with a fractional degree of ionization of hydrogen of about 30 percent.
Fahr Hans Jörg
Osterbart Roger
Ruciński Daniel
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