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Observations of Hα Intensity Oscillations in a Flare Ribbon

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© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation R. T. James McAteer et al 2005 ApJ 620 1101 DOI 10.1086/427084

0004-637X/620/2/1101

Abstract

High-cadence Hα blue wing observations of a C9.6 solar flare obtained at Big Bear Solar Observatory using the Rapid Dual Imager are presented. Wavelet and time-distance methods were used to study oscillatory power along the ribbon, finding periods of 40-80 s during the impulsive phase of the flare. A parametric study found statistically significant intensity oscillations with amplitudes of 3% of the peak flare amplitude, periods of 69 s (14.5 mHz) and oscillation decay times of 500 s. These measured properties are consistent with the existence of flare-induced acoustic waves within the overlying loops.

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10.1086/427084