We investigate quasi-periodic coronal pulsations during the decay phase of an X 3.2 class flare on 14 May 2013, using soft X-ray data from the RHESSI satellite. Periodogram analyses of soft X-ray light curves show that ∼ 53 s and ∼ 72 s periods co-exist in the 3-6 keV, 6-12 keV and 12-25 keV energy bands. Considering the typical length of the flaring loop system and observed periodicities, we find that they are associated with multiple (first two harmonics) of fast magnetoacoustic sausage waves. The phase relationship of soft X-ray emissions in different energy bands using cross-correlation technique show that these modes are standing in nature as we do not find the phase lag. Considering the period ratio, we diagnose the local plasma conditions of the flaring region by invoking MHD seismology. The period ratio P1/2P2 is found to be ∼ 0.65, which indicates that such oscillations are most likely excited in longitudinal density stratified loops.
Advances in Space Research
- Pub Date:
- December 2015
- Magnetohydrodynamics (MHD);
- Astrophysics - Solar and Stellar Astrophysics
- 16 pages, 7 figures, accepted to Advances in Space Research, 2015