NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The observation of a coronal transient directed at earthThe paper reports the observation of a large coronal transient that can only be interpreted as a three-dimensional structure. Its form is one which has not been observed before: a gradually expanding, sun-centered disk of excess brightness, whose projected radius increased from 4 to 8 solar radii during 0832-0958 UT on November 27, 1979. This earth-directed transient was the source of an interplanetary shock wave that reached ISEE 3 at 0649 UT, November 30, and earth at 0738 UT, November 30. Fitting the shock speed at ISEE 3 and the average transit speed from the sun to ISEE 3 to a power law of the form V = (V sub 0)(r exp -n), it is found that V sub 0 = 1980 km/s and n = 0.294, in good agreement with shock wave models. The shock speed predicted by the power law at 10 solar radii is 1000 km/s, in good agreement with the estimated frontal speed of the transient.
Document ID
19830035818
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Howard, R. A.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Michels, D. J.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Sheeley, N. R., Jr.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Koomen, M. J.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Date Acquired
August 11, 2013
Publication Date
December 15, 1982
Publication Information
Publication: Astrophysical Journal
Subject Category
Solar Physics
Accession Number
83A17036
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-14429
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available