Radio sounding of the solar corona during 1995 solar conjunction of the ULYSSES spacecraft

Details Radio sounding of the solar corona during 1995 solar conjunction of the ULYSSES spacecraft Radio sounding of the solar corona during 1995 solar conjunction of the ULYSSES spacecraft

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...96b&link_type=abstract

International Solar Wind 8 Conference, p. 96

Computer Science

Sound

Solar Corona, Superhigh Frequencies, Ultrahigh Frequencies, Radio Signals, Atmospheric Sounding, Solar Diameter, Sun, Latitude Measurement, Sound Ranging, Solar Physics, Ulysses Mission, Very High Frequency Radio Equipment, Doppler Radar, Solar Eclipses, Time Series Analysis, Density Distribution

Scientific paper

The Ulysses spacecraft will pass through superior solar conjunction on March 5 1995, a few days before its perihelion and passage through the ecliptic plane. Dual-frequency S/X-band ranging and Doppler observations will be conducted in support of the Ulysses Solar Corona Experiment (SCE) during a three-week interval centered on the conjunction. The occultation geometry is unique in the annals of interplanetary exploration. As viewed from Earth, the spacecraft will appear to cut diagonally through the southwest quadrant of the solar corona from the South Pole to the equator. The minimum proximate distance to the Sun of the radio ray path will be 21.6 solar radius. The entire latitude scan from pole to equator occurs for a limited range of solar offset distances (is less than 30 solar radius thus facilitating the separation of latitudinal from radial variations in the coronal density and associated parameters of interest.

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