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Satellite Observations of the Outer Oorona Near Sunspot Maximum

Published online by Cambridge University Press:  14 August 2015

D. J. Michels ,
R. A. Howard ,
M. J. Koomen  and
N. R. Sheeley Jr.
D. J. Michels
Affiliation:
E. O. Hulburt Center for Space Research U. S. Naval Research Laboratory Washington, D. C. 20375
R. A. Howard
Affiliation:
E. O. Hulburt Center for Space Research U. S. Naval Research Laboratory Washington, D. C. 20375
M. J. Koomen
Affiliation:
E. O. Hulburt Center for Space Research U. S. Naval Research Laboratory Washington, D. C. 20375
N. R. Sheeley Jr.
Affiliation:
E. O. Hulburt Center for Space Research U. S. Naval Research Laboratory Washington, D. C. 20375

Abstract

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This paper shows the first satellite observations of the Sun's white light corona (2.6 R⊙ −10.0 R⊙) during the active phase of a sunspot cycle. Since March 28, 1979, these observations have been obtained routinely with a spatial resolution of 1.25 arc min and a repetition rate of 10 minutes during the one-hour sunlit portion of each 97-minute satellite orbital period. As an illustration of these new observations, we show the coronal changes associated with the great mass ejection of May 8, 1979.

Type
Session VII - Solar Bursts - Radio, White Light and X-ray Observations
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 439 - 442
Copyright
Copyright © Reidel 1980 

References

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