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

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Abstract:

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).

Info:

Periodical:
International Letters of Chemistry, Physics and Astronomy (Volume 23)
Pages:
29-36
Citation:
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:
Nov 2013
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References:

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