Spatial and temporal analysis of 3-minute oscillations in the chromosphere associated with the X2.2 Solar Flare on 2011 February 15
Laurel Farris, R. T. James McAteer

TL;DR
This study analyzes the spatial and temporal behavior of 3-minute chromospheric oscillations around a major solar flare, revealing localized power increases linked to energy injection by nonthermal particles, supporting the acoustic cutoff response theory.
Contribution
It provides detailed spatial-temporal analysis of chromospheric oscillations during a solar flare, highlighting localized power enhancements and their relation to energy injection mechanisms.
Findings
Higher 3-minute power during the flare, concentrated in small areas.
Localized oscillations suggest non-global chromospheric response.
Correlation between oscillation sites and nonthermal particle energy injection.
Abstract
3-minute oscillations in the chromosphere are attributed to both slow magnetoacoustic waves propagating from the photosphere, and to oscillations generated within the chromosphere itself at its natural frequency as a response to a disturbance. Here we present an investigation of the spatial and temporal behavior of the chromospheric 3-minute oscillations before, during, and after the SOL2011-02-15T01:56 X2.2 flare. Observations in ultraviolet emission centered on 1600 and 1700 Angstroms obtained at 24- second cadence from the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory are used to create power maps as functions of both space and time. We observe higher 3-minute power during the flare, spatially concentrated in small areas 10 pixels (4 arcseconds) across. This implies that the chromospheric plasma is not oscillating globally as a single body. The locations of…
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