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Oscillations of the Magnetic Network
Published online by Cambridge University Press: 12 April 2016
Abstract
We present high-quality power spectra of oscillations in the quiet solar chromosphere measured from the Ca II H line. They show unambiguously that the network does not participate in chromospheric three-minute oscillations, but that instead it oscillates in slow wave motions which are neither present in the surrounding non-magnetic chromosphere, nor in the underlying photosphere.
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- Session 9. Convections and Oscillation in Active Regions
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- Copyright © Astronomical Society of the Pacific 1993
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