On the Magnetic Field Variations and HXR Emission of the First X-class Flare in the 24th Solar Cycle

Details On the Magnetic Field Variations and HXR Emission of the First X-class Flare in the 24th Solar Cycle On the Magnetic Field Variations and HXR Emission of the First X-class Flare in the 24th Solar Cycle

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.2225m&link_type=abstract

American Astronomical Society, SPD meeting #42, #22.25; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Multi-wavelength studies of energetic solar flares with seismic emissions have revealed interesting common features between them. We studied the first seismically active flare of the 24th solar cycle
(SOL2011-02-15T01:52 X2.2) detected by HMI/SDO (Kosovichev, 2011) using a pixel-by-pixel light-curve characterization of the fluctuations of the photospheric longitudinal magnetic field based on HMI data. For context we used HXR RHESSI data to find a correlation between these sources and the spatial location of the transient longitudinal magnetic field changes in the photospheric region where this flare took place.

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