High-frequency oscillations in a solar active region coronal loop

Details High-frequency oscillations in a solar active region coronal loop High-frequency oscillations in a solar active region coronal loop

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.326..428w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 326, Issue 2, pp. 428-436.

Astronomy and Astrophysics

Astronomy

52

Mhd, Waves, Eclipses, Sun: Activity, Sun: Corona, Sun: Oscillations

Scientific paper

The Solar Eclipse Corona Imaging System (SECIS) was used to record high-cadence observations of the solar corona during the total solar eclipse of 1999 August 11. During the 2min 23.5s of totality, 6364 images were recorded simultaneously in each of the two channels: a white light channel, and the Fexiv (5303Å) `green line' channel (T~2MK). Here we report initial results from the SECIS experiment, including the discovery of a 6-s intensity oscillation in an active region coronal loop.

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