Physics
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..363j&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 95, Feb. 1985, p. 363-370.
Physics
13
Helios B, Stellar Mass Ejection, Astronomical Photometry, Coronagraphs, Helios A
Scientific paper
The Helios-spacecraft zodiacal light photometers are used to observe the earthward-directed solar-mass ejection transient of November 27, 1979 described by Howard et al. (1982) that completely circles the sun in coronagraph observations. At this time, Helios B was situated 30 deg east of the sun-earth line at 0.5 AU. The brightness increase moved outward directly along the sun-earth line over a period of approximately 24 hr, indicating a strong collimation of the ejection. The outward motion and mass estimates of the ejected material from the photometers compared with near-earth observations from IMP spacecraft show that at least a portion of the density increase observed at earth on November 29 and 30 was associated with this ejection.
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