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Flare-generated coronal loop oscillations: A tool for MHD coronal seismology

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UNSPECIFIED (2000) Flare-generated coronal loop oscillations: A tool for MHD coronal seismology. In: International Workshop on Waves in Dusty, Solar, and Space Plasmas, MAY 22-26, 2000, LEUVEN, BELGIUM.

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Abstract

Quasi-periodical oscillations of positions of coronal loops were observed in the extreme- ultraviolet band (171A, FeIX) with the imaging telescope onboard the TRACE spacecraft. Oscillating transversal displacements (swinging) of a long (similar to 130 Mm) thin (diameter similar to2 Mm) bright loop, were detected. The oscillations were excited by a flare (14th July 1998 at about 12:55 UT) at distance of about 60 Mm from the loop. The frequency of the oscillations was about 4 mHz (the period about 265 s) and was determined by the wavelet analysis. Neighbouring perpendicular slits show synphase temporal behaviour, suggesting that the oscillations are produced by a Link global fast magnetoacoustic mode of the loop. With this interpretation, we determine the kink speed in the loop as 1040 km/s, which gives the Alfven speed of about 770+/-40 km/s. The detection and analysis of post-flare oscillations of coronal loops provides us with an efficient tool for indirect determination of coronal parameters, e.g. the magnetic field found to be of about 20 G.

Item Type: Conference Item (UNSPECIFIED)
Subjects: Q Science > QC Physics
Series Name: AIP CONFERENCE PROCEEDINGS
Journal or Publication Title: WAVES IN DUSTY, SOLAR, AND SPACE PLASMAS
Publisher: AMER INST PHYSICS
ISBN: 1-56396-962-9
ISSN: 0094-243X
Editor: Verheest, F and Goossens, M and Hellberg, MA and Bharuthram, R
Date: 2000
Volume: 537
Number of Pages: 7
Page Range: pp. 264-270
Publication Status: Published
Title of Event: International Workshop on Waves in Dusty, Solar, and Space Plasmas
Location of Event: LEUVEN, BELGIUM
Date(s) of Event: MAY 22-26, 2000
URI: http://wrap.warwick.ac.uk/id/eprint/12650

Data sourced from Thomson Reuters' Web of Knowledge

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