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An Observation of an Inverted Type U Solar Burst due to AR1429 Active Region
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An Observation of an Inverted Type U Solar Burst due to AR1429 Active Region

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Abstract:

A detailed investigation of an inverted type U solar burst in meter region and their associated the solar flare and Coronal Mass Ejections (CMEs) has been reported. Solar type U burst has been observed at the National Space Centre, Banting, Selangor detected by the Compound Low Cost Low Frequency Transportable Observatories (CALLISTO) system in the 150 MHz till 400 MHz at the low frequency band. An inverted U type is occurring on 9th March 2012 between 4:00 UT to 4:15 UT within 1 minute (4:12 − 4:13) UT. From the dynamic spectra of CALLISTO, we have identified metric type U burst with maximum emission near the frequency 385MHz. In specific, the continuum type III burst will soon structure this burst due to our observations. Other types such as type II and IV are only appearing only after type U burst is ejected and appear at the same point of the solar flare event. Since the U burst activity coincides with the peak of the hard X-ray flare at 4:12UT in AR1429, we classified that the event is associated with the injection of the high energetic particles. In conclusion, it is confirmed that an inverted type U burst is initiated after a complex and a group solar radio burst type III.

Info:

Periodical:
International Letters of Chemistry, Physics and Astronomy (Volume 29)
Pages:
81-90
DOI:
https://doi.org/10.18052/www.scipress.com/ILCPA.29.81
Citation:
Z. S. Hamidi et al., "An Observation of an Inverted Type U Solar Burst due to AR1429 Active Region", International Letters of Chemistry, Physics and Astronomy, Vol. 29, pp. 81-90, 2014
Online since:
March 2014
Authors:
Zety Sharizat Hamidi, N.N.M. Shariff, C. Monstein
Keywords:
CALLISTO, Low Frequency, Radio Frequency Interference (RFI), Solar Burst, Type U
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Distribution:
Open Access

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This work is licensed under a
Creative Commons Attribution 4.0 International License

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