This (Large Angle and Spectrometric Coronagraph) LASCO C2 sequence of six consecutive images taken over one and a half hours on 11 November 2002 shows the propagation of a coronal mass ejection (CME) associated with a relatively small M1 flare. Flares are intense releases of radiant energy, often associated with violent mass motions such as eruptive prominences and CME's. The bright material in the center of the outward-propagating CME is probably denser, cooler prominence material. The Sun, bl

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This (Large Angle and Spectrometric Coronagraph) LASCO C2 sequence of six consecutive images taken over one and a half hours on 11 November 2002 shows the propagation of a coronal mass ejection (CME) associated with a relatively small M1 flare. Flares are intense releases of radiant energy, often associated with violent mass motions such as eruptive prominences and CME's. The bright material in the center of the outward-propagating CME is probably denser, cooler prominence material. The Sun, bl

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