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Oscillations Observed in Intensity and Velocity for a Quiescent Prominence
Published online by Cambridge University Press: 13 May 2016
Abstract
We present the results obtained from analyzing SUMER/SOHO observation data of a quiescent solar prominence. From the 1 hour data set, we derive via a wavelet transform, characteristic frequencies in terms of intensity and velocity oscillations, as measured in 4 transition region lines.
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- Session IV: Structure and Dynamics of the Transiton Region and Corona
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- Copyright © Astronomical Society of the Pacific 2001