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Solar Observations with a New Earth-Orbiting Coronagraph
Published online by Cambridge University Press: 14 August 2015
Abstract
Since March 28, 1979, the Solwind coronagraph has been observing the Sun's white light corona (2.6 − 10.0 R⊙) routinely with a spatial resolution of approximately 1.25 arc min and a repetition rate of 10 minutes during the one-hour sunlit portion of each 97-minute satellite orbital period. These are the first satellite observations of the outer corona near the peak of a sunspot cycle when coronal transients and high-latitude streamers are common.
- Type
- Part I. The Life History of Coronal Structures and Fields
- Information
- Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 55 - 59
- Copyright
- Copyright © Reidel 1980
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