Abstract
Measurements of S-band downlink frequency (Doppler) shift were collected for intervals of about 30 days during the 1994 and 1995 solar conjunctions of the Galileo spacecraft. The occultation geometries enabled coronal radio sounding of the heliographic equatorial region over a heliocentric range from about 5 to 20 R s (solar radii) for the 1994 conjunction and from about 4 to 35 R s for the 1995 conjunction. Spectral analysis was carried out with the S-band Doppler scintillations to determine the strength and spectral distribution of coronal electron density fluctuations. Cross-correlations of the Galileo downlink signals received simultaneously at two ground stations were computed to obtain the propagation velocity of plasma disturbances crossing the ray paths.
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© 1997 Springer Science+Business Media Dordrecht
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Wohlmuth, R., Plettemeier, D., Edenhofer, P., Bird, M.K., Asmar, S.W. (1997). Analysis of Galileo Doppler Measurements during the Solar Occultations in 1994 And 1995. In: Barbieri, C., Rahe, J.H., Johnson, T.V., Sohus, A.M. (eds) The Three Galileos: The Man, the Spacecraft, the Telescope. Astrophysics and Space Science Library, vol 220. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-8790-7_41
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DOI: https://doi.org/10.1007/978-94-015-8790-7_41
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