Although the Phobos spacecraft will make some limited in situ measurements of Mars' upper ionosphere during its transfer orbits, the major part of the mission will be limited to remote sensing by radio occultation and topside sounding methods. To 'calibrate' the former as a means of studying the ionosphere and solar wind interaction, the Pioneer Venus Orbiter radio occultation experiment results are examined in light of what is known from in situ plasma and magnetic field data. This calibration can be used to reassess the data from previous Mars missions and to provide a basis for interpreting data from the upcoming Phobos mission.


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    Titel :

    Remote sensing of Mars' ionosphere and solar wind interaction - Lessons from Venus


    Beteiligte:
    Luhmann, J. G. (Autor:in) / Kliore, A. (Autor:in) / Barnes, A. (Autor:in) / Brace, L. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1990



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch




    Remote sensing of mars' ionosphere and solar wind interaction: Lessons from venus

    Luhmann, J.G. / Kliore, A. / Barnes, A. et al. | Elsevier | 1989




    The Topside Ionosphere of Venus and Its Interaction with the Solar Wind

    S. J. Bauer / R. E. Hartle / J. R. Herman | NTIS | 1969


    The Venus ionosphere as an obstacle to the solar wind

    Theis, R.F. / Brace, L.H. / Schatten, K.H. et al. | Elsevier | 1981