A synoptic study of Doppler scintillation transients in the solar wind

Astronomy and Astrophysics – Astronomy

Scientific paper

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Doppler Effect, Shock Wave Propagation, Solar Neighborhood, Solar Wind, Synoptic Measurement, Terrestrial Planets, Interplanetary Spacecraft, Nasa Programs, Pioneer 11 Space Probe, Radio Sources (Astronomy), Remote Sensing

Scientific paper

This paper conducts the first synoptic study of Doppler scintillation transients caused by interplanetary disturbances. The Doppler scintillation data used are part of the 2.3-GHz navigation data collected by the NASA Deep Space Network when tracking planetary spacecraft during 1979-1983, a period that includes solar maximum. A total of 148 separate transients covering a heliocentric distance range of 5-179 solar radii were detected, including 26 transients detected by more than one spacecraft. The frequency of occurrence was highest near the sun and decreased with radial distance, a reflection of the radial evolution of the transients and the sensitivity of the Doppler scintillation measurements to transients. Since transients can be disruptive, as was demonstrated during the encounter of Saturn by Pioneer 11 in 1979, information on Doppler scintillation transients is essential.

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