Little or no solar wind enters Venus’ atmosphere at solar minimum View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2007-11

AUTHORS

T L Zhang, M Delva, W Baumjohann, H-U Auster, C Carr, C T Russell, S Barabash, M Balikhin, K Kudela, G Berghofer, H K Biernat, H Lammer, H Lichtenegger, W Magnes, R Nakamura, K Schwingenschuh, M Volwerk, Z Vörös, W Zambelli, K-H Fornacon, K-H Glassmeier, I Richter, A Balogh, H Schwarzl, S A Pope, J K Shi, C Wang, U Motschmann, J-P Lebreton

ABSTRACT

Venus has no significant internal magnetic field, which allows the solar wind to interact directly with its atmosphere. A field is induced in this interaction, which partially shields the atmosphere, but we have no knowledge of how effective that shield is at solar minimum. (Our current knowledge of the solar wind interaction with Venus is derived from measurements at solar maximum.) The bow shock is close to the planet, meaning that it is possible that some solar wind could be absorbed by the atmosphere and contribute to the evolution of the atmosphere. Here we report magnetic field measurements from the Venus Express spacecraft in the plasma environment surrounding Venus. The bow shock under low solar activity conditions seems to be in the position that would be expected from a complete deflection by a magnetized ionosphere. Therefore little solar wind enters the Venus ionosphere even at solar minimum. More... »

PAGES

654-656

References to SciGraph publications

  • 1991-03. The magnetosheath and magnetotail of Venus in SPACE SCIENCE REVIEWS
  • 1986-09. The solar wind interaction with Venus in SPACE SCIENCE REVIEWS
  • 1991-03. The structure of the Venus ionosphere in SPACE SCIENCE REVIEWS
  • 1989-10. Magnetic fields near Mars: first results in NATURE
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1038/nature06026

    DOI

    http://dx.doi.org/10.1038/nature06026

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1026095038

    PUBMED

    https://www.ncbi.nlm.nih.gov/pubmed/18046399


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