Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...103..415a&link_type=abstract
Astronomy and Astrophysics, vol. 103, no. 2, Nov. 1981, p. 415-421. NASA-supported research.
Astronomy and Astrophysics
Astrophysics
54
Radio Observation, Remote Sensors, Scintillation, Solar Wind Velocity, Spacecraft Instruments, Helios 1, Magnetohydrodynamic Flow, Plasma Density, Radial Velocity, Radio Signals, Random Signals, Solar Corona, Viking Orbiter Spacecraft
Scientific paper
New remote-sensing observations are reported of the solar wind motion within about 30 earth radii. Use is made of the interplanetary scintillation (IPS) spaced receiver technique with the radio source being a spacecraft signal (rather than a natural radio source as in previous spaced receiver studies). The spacecraft used are Helios A and B and the Viking orbiters. The purposes of the study are (1) to augment the scarce estimates of solar wind bulk flow speed near the sun and in the ecliptic with measurements made using spacecraft signals, and (2) to estimate random velocity components and identify the region where the random velocity is a significant fraction of the mean velocity. In addition, the radial evolution of speed and random velocity is compared with that of the plasma density fluctuation spectrum. Also reported are the first accurately normalized IPS scintillation index measurements using a monochromatic point source.
Armstrong John W.
Woo Richard
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