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Propagating EUV disturbances in the Solar corona: Two-wavelength observations

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UNSPECIFIED. (2003) Propagating EUV disturbances in the Solar corona: Two-wavelength observations. ASTRONOMY & ASTROPHYSICS, 404 (1). L1-L4. ISSN 0004-6361

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Official URL: http://dx.doi.org/10.1051/0004-6361:20030763

Abstract

Quasi-periodic EUV disturbances simultaneously observed in 171 Angstrom and 195 Angstrom TRACE bandpasses propagating outwardly in a fan-like magnetic structure of a coronal active region are analysed. Time series of disturbances observed in the different bandpasses have a relatively high correlation coefficient (up to about 0.7). The correlation has a tendency to decrease with distance along the structure: this is consistent with an interpretation of the disturbances in terms of parallel-propagating slow magnetoacoustic waves. The wavelet analysis does not show a significant difference between waves observed in different bandpasses. Periodic patterns of two distinct periods: 2-3 min and 5-8 min are detected in both bandpasses, existing simultaneously and at the same distance along the loop, suggesting the nonlinear generation of the second harmonics.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Journal or Publication Title: ASTRONOMY & ASTROPHYSICS
Publisher: E D P SCIENCES
ISSN: 0004-6361
Date: June 2003
Volume: 404
Number: 1
Number of Pages: 4
Page Range: L1-L4
Identification Number: 10.1051/0004-6361:20030763
Publication Status: Published
URI: http://wrap.warwick.ac.uk/id/eprint/9702

Data sourced from Thomson Reuters' Web of Knowledge

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