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Kink oscillations of coronal loops as a tool for the determination of coronal magnetic field

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UNSPECIFIED (2002) Kink oscillations of coronal loops as a tool for the determination of coronal magnetic field. In: 10th European Solar Physics Meeting, SEP 09-14, 2002, PRAGUE, CZECH REPUBLIC.

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Abstract

We develop a new method for the determination of the absolute value of the magnetic field strength in coronal closed magnetic structures, based on the analysis of flare-generated oscillations of coronal loops. Interpretation of the quasi-harmonic oscillations observed in terms of global standing kink waves allows to connect the period of the oscillations and the loops length with the magnetic field strength in the loops. Improved diagnostic of the loop length, the oscillation period, and the plasma density in the loop will significantly improve the method's precision.

Item Type: Conference Item (UNSPECIFIED)
Subjects: Q Science > QB Astronomy
Series Name: ESA SPECIAL PUBLICATIONS
Journal or Publication Title: SOLAR VARIABILITY: FROM CORE TO OUTER FRONTIERS, VOLS 1 & 2
Publisher: EUROPEAN SPACE AGENCY
ISBN: 92-9092-816-6
ISSN: 0379-6566
Date: 2002
Volume: 506
Number of Pages: 4
Page Range: pp. 461-464
Publication Status: Published
Title of Event: 10th European Solar Physics Meeting
Location of Event: PRAGUE, CZECH REPUBLIC
Date(s) of Event: SEP 09-14, 2002
URI: http://wrap.warwick.ac.uk/id/eprint/9001

Data sourced from Thomson Reuters' Web of Knowledge

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