Zharkov, S;
Green, LM;
Matthews, SA;
Zharkova, VV;
(2013)
Properties of the 15 February 2011 Flare Seismic Sources.
Solar Physics
, 284
(2)
pp. 315-327.
10.1007/s11207-012-0169-4.
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Abstract
The first near-side X-class flare of Solar Cycle 24 occurred in February 2011 (SOL2011-02-05T01:55) and produced a very strong seismic response in the photosphere. One sunquake was reported by Kosovichev (Astrophys. J. Lett. 734, L15, 2011), followed by the discovery of a second sunquake by Zharkov, Green, Matthews et al. (Astrophys. J. Lett. 741, L35, 2011). The flare had a two-ribbon structure and was associated with a flux-rope eruption and a halo coronal mass ejection (CME) as reported in the CACTus catalogue. Following the discovery of the second sunquake and the spatial association of both sources with the locations of the feet of the erupting flux rope (Zharkov, Green, Matthews et al., Astrophys. J. Lett. 741, L35, 2011), we present here a more detailed analysis of the observed photospheric changes in and around the seismic sources. These sunquakes are quite unusual, taking place early in the impulsive stage of the flare, with the seismic sources showing little hard X-ray (HXR) emission, and strongest X-ray emission sources located in the flare ribbons. We present a directional time–distance diagram computed for the second source, which clearly shows a ridge corresponding to the travelling acoustic-wave packet and find that the sunquake at the second source happened about 45 seconds to one minute earlier than the first source. Using acoustic holography we report different frequency responses of the two sources. We find strong downflows at both seismic locations and a supersonic horizontal motion at the second site of acoustic-wave excitation.
| Type: | Article |
|---|---|
| Title: | Properties of the 15 February 2011 Flare Seismic Sources |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1007/s11207-012-0169-4 |
| Publisher version: | http://dx.doi.org/10.1007/s11207-012-0169-4 |
| Language: | English |
| Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
| Keywords: | Sun: helioseismology, Sun: flares, Sun: X-rays, Gamma ray, TIME-DISTANCE HELIOSEISMOLOGY, SPECTROSCOPIC-IMAGER RHESSI, 2003 OCTOBER 28, SOLAR-FLARES, FIELD, ENERGY, SUN, HOLOGRAPHY, SUNSPOTS, OSCILLATIONS |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
| URI: | https://discovery.ucl.ac.uk/id/eprint/10044347 |
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