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In this paper, we present a study of an M2.2 class solar flare of 26 November2000 from NOAA AR 9236. The flare was well observed by various ground basedobservatories (ARIES, Learmonths Solar Observatory) and space borne instruments(SOHO, HXRS, GOES) in time interval between 02:30 UT to 04:00 UT. The flarestarted with long arc-shape outer flare ribbon. Afterwards the main flarestarts with two main ribbons. Initially the outer ribbons start to expand withan average speed ($\sim$ 20 km s$^{-1}$) and later it shows contraction. Theflare was associated with partial halo coronal mass ejection (CMEs) which hasaverage speed of 495 km s$^{-1}$. The SOHO/MDI observations show that theactive region was in quadrupolar magnetic configuration. The flux cancellationwas observed before the flare onset close to flare site. Our analysis indicatethe flare was initiated by the magnetic breakout mechanism.

Multi-wavelength view of an M2.2 Solar Flare on 26 November 2000