Temperature Analysis of Flaring (AR11283) and non-Flaring (AR12194) Coronal Loops

Abstract Here, we study the temperature structure of flaring and non-flaring coronal loops, using extracted loops from images taken in six extreme ultraviolet (EUV) channels recorded by Atmospheric Imaging Assembly (AIA)/ Solar Dynamic Observatory (SDO). We use data for X2.1-class-flaring active region (AR11283) during 22:10UT till 23:00UT, on 2011, September 6; (AR12194) 08:00:00UT 09:00:00UT 2014, October 26. By spatially-synthesized Gaussian DEM forward-fitting method, calculate peak temperatures each strip loops. apply Lomb-Scargle method to compute oscillations periods series strip. The are ranged 7 min 28.4 min. These show very close behavior slow-mode oscillation. observe that started at least around 10 minutes before transverse continue a long time duration even after ended. amplitudes increased (during 20 min) obtained 8.5 30 min,but their significances less (below 0.5) comparison with ones (near one). Hence detected loops' strips probable ones, maybe they just fluctuations. Based our confined observations, it seems more diversity have wider ranges variation than ones. More accurate commentary this respect requires extensive statistical research broader observations.