Investigation on the formation of herringbone structure in type II solar radio bursts
We report detailed observation of the ``herringbone'' of a Type II solar radio burst that occurred on 2010 November 3rd. Data from the Space Weather Prediction Center, National Oceanic and Atmospheric Administration, e-CALLISTO, and Nancay RadioHeliograph are analyzed. We determine the bri...
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Natl Astronomical Observatories, Chin Acad Sciences
2023
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my.um.eprints.382562024-06-10T04:46:38Z http://eprints.um.edu.my/38256/ Investigation on the formation of herringbone structure in type II solar radio bursts Abidin, Zamri Zainal Zulkiplee, A. N. Epin, V. Pauzi, F. A. M. QC Physics We report detailed observation of the ``herringbone'' of a Type II solar radio burst that occurred on 2010 November 3rd. Data from the Space Weather Prediction Center, National Oceanic and Atmospheric Administration, e-CALLISTO, and Nancay RadioHeliograph are analyzed. We determine the brightness temperature and degree of circular polarization of the ``herringbone'' burst. Correlations between the physical parameters and the ``herringbone'' are examined. Based on the relationship, this is the first study that suggested this ``herringbone'' was generated through fundamental plasma. Natl Astronomical Observatories, Chin Acad Sciences 2023-05 Article PeerReviewed Abidin, Zamri Zainal and Zulkiplee, A. N. and Epin, V. and Pauzi, F. A. M. (2023) Investigation on the formation of herringbone structure in type II solar radio bursts. Research in Astronomy and Astrophysics, 23 (5). ISSN 1674-4527, DOI https://doi.org/10.1088/1674-4527/acc14e <https://doi.org/10.1088/1674-4527/acc14e>. 10.1088/1674-4527/acc14e |
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QC Physics Abidin, Zamri Zainal Zulkiplee, A. N. Epin, V. Pauzi, F. A. M. Investigation on the formation of herringbone structure in type II solar radio bursts |
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We report detailed observation of the ``herringbone'' of a Type II solar radio burst that occurred on 2010 November 3rd. Data from the Space Weather Prediction Center, National Oceanic and Atmospheric Administration, e-CALLISTO, and Nancay RadioHeliograph are analyzed. We determine the brightness temperature and degree of circular polarization of the ``herringbone'' burst. Correlations between the physical parameters and the ``herringbone'' are examined. Based on the relationship, this is the first study that suggested this ``herringbone'' was generated through fundamental plasma. |
format |
Article |
author |
Abidin, Zamri Zainal Zulkiplee, A. N. Epin, V. Pauzi, F. A. M. |
author_facet |
Abidin, Zamri Zainal Zulkiplee, A. N. Epin, V. Pauzi, F. A. M. |
author_sort |
Abidin, Zamri Zainal |
title |
Investigation on the formation of herringbone structure in type II solar radio bursts |
title_short |
Investigation on the formation of herringbone structure in type II solar radio bursts |
title_full |
Investigation on the formation of herringbone structure in type II solar radio bursts |
title_fullStr |
Investigation on the formation of herringbone structure in type II solar radio bursts |
title_full_unstemmed |
Investigation on the formation of herringbone structure in type II solar radio bursts |
title_sort |
investigation on the formation of herringbone structure in type ii solar radio bursts |
publisher |
Natl Astronomical Observatories, Chin Acad Sciences |
publishDate |
2023 |
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http://eprints.um.edu.my/38256/ |
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1805881101802012672 |
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13.18916 |