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Observations of Different Type of Bursts Associated with M 6.3 Solar Flares

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Variation of solar bursts due to solar flares such as type an isolated type III , a complex type III, U is being highlighted. These bursts occurred on 9th March 2012 at the National Space Centre, Sg. Lang, Selangor, Malaysia Here, we study a unique case with a combination of two types burst associated with solar flare and CMEs. Our observation is focused on the low frequency region starting from 150 MHz till 400 MHz. We found that a solar flare type solar flare type M 6.3 which occurred in active region AR 1429 starting from 3:32 UT and ending at 05:00 UT. The flare has been confirmed to be the largest flare since 2005. Some physical parameters will be measured. We then compared our results with X-ray data from NOAA Space Weather Prediction Centre (SWPC).


International Letters of Chemistry, Physics and Astronomy (Volume 23)
Z. S. Hamidi and N.N.M. Shariff, "Observations of Different Type of Bursts Associated with M 6.3 Solar Flares", International Letters of Chemistry, Physics and Astronomy, Vol. 23, pp. 29-36, 2014
Online since:
November 2013

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