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Coronal Heating by MHD Waves: Results from the SECIS Instrument during the 1999 Eclipse
Published online by Cambridge University Press: 13 May 2016
Abstract
We report on results from the Solar Eclipse Coronal Imaging System (SECIS), an instrument using fast CCD cameras designed to search for short-period modulations in visible-light emission from the corona during an eclipse or with a coronagraph. The instrument was successfully used during the total eclipse of 1999 August 11 from a site in Bulgaria. This paper summarizes both the instrument and preliminary results.
- Type
- Session V: Coronal Heating and Solar Wind Acceleration
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- Copyright © Astronomical Society of the Pacific 2001