Determining the LIC H density from the solar wind slowdown

D. Richardson, Y. Liu, C. Wang, J. McComas

Research output: Contribution to journalArticlepeer-review

47 Scopus citations

Abstract

Context. The ionized solar wind interacts directly with the interstellar neutrals which flow into the heliosphere. These neutrals are ionized, mainly by charge exchange, then accelerated to the solar wind speed with the momentum and energy removed from the bulk flow of the solar wind. Thus, by measuring the solar wind slowdown, one can estimate the interstellar neutral density.Aims. In July 2005, Ulysses at 5 AU and Voyager 2 near 80 AU were at the same heliolatitude. We use this alignment to determine the solar wind speed decrease between these two spacecraft.Methods. Ulysses data are used as input to a 1-D MHD model which includes the effects of pickup ions. We removed a section of data contaminated by an ICME directed toward Voyager 2.Results. Comparison of the Voyager 2 speeds with the model results shows that the solar wind speed decreased by 67 kms-1 between Ulysses and Voyager 2, consistent with an interstellar neutral density at the termination shock of 0.09 cm -3.

Original languageEnglish (US)
Pages (from-to)1-5
Number of pages5
JournalAstronomy and Astrophysics
Volume491
Issue number1
DOIs
StatePublished - Nov 2008
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Interplanetary medium
  • Solar wind

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