Flare Associated Oscillations Observed with NoRH

Details Flare Associated Oscillations Observed with NoRH Flare Associated Oscillations Observed with NoRH

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spnr.conf...33a&link_type=abstract

Solar Physics with the Nobeyama Radioheliograph, Proceedings of Nobeyama Symposium 2004, held in Kiyosato, Japan, October 26- 29

Physics

Scientific paper

We present an examination of the multi-wavelength observation of a C7.9 flare which occurred on 1998 November 10. This is an imaging observation of the quasi-periodic pulsations (QPPs) obtained with Yohkoh/HXT and Nobeyama Radioheliograph (NoRH). We found that the Alfven transit time along the flare loop was almost equal to the period of the QPP. We therefore suggest that variations of macroscopic magnetic structures, such as oscillations of coronal loops, affect the efficiency of particle injection/acceleration. We also report other QPP events observed with NoRH, and review some works on these flare-associated oscillations.

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