Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts

An investigation into Type II solar radio bursts was carried out to understand the frequency gap between fundamental and harmonic emissions of the radio burst. This investigation focused on Type II solar radio bursts with flares and coronal mass ejections by relating the separation between fundament...

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Main Authors: Pauzi, F.A.M., Abidin, Zamri Zainal, Guo, Shao Jie, Gao, Guan Nan, Dong, L., Monstein, Christian
Format: Article
Published: Springer 2020
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Online Access:http://eprints.um.edu.my/25407/
https://doi.org/10.1007/s11207-019-1404-z
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spelling my.um.eprints.254072020-08-18T07:33:10Z http://eprints.um.edu.my/25407/ Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts Pauzi, F.A.M. Abidin, Zamri Zainal Guo, Shao Jie Gao, Guan Nan Dong, L. Monstein, Christian Q Science (General) QC Physics An investigation into Type II solar radio bursts was carried out to understand the frequency gap between fundamental and harmonic emissions of the radio burst. This investigation focused on Type II solar radio bursts with flares and coronal mass ejections by relating the separation between fundamental and harmonic emissions. We used the Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Spectrometers (CALLISTO) and a newly designed low-frequency antenna array. This article describes the proposed new instrument in terms of its antenna design, the bandpass testing of the antenna, the new system significance in studying Type II solar radio bursts, and its comparison with other leading radio solar monitoring instruments. Upon setting up the new technology, the radio-frequency interference of the observation site at the University of Malaya was shown to emphasize the suitability of the selected site. This article also shows the preliminary results of the proposed new instrument by reporting the detection of a Type III solar radio burst that was confirmed by CALLISTO. Moreover, it also includes the optimal observation design and strategies for future detections. © 2020, Springer Nature B.V. Springer 2020 Article PeerReviewed Pauzi, F.A.M. and Abidin, Zamri Zainal and Guo, Shao Jie and Gao, Guan Nan and Dong, L. and Monstein, Christian (2020) Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts. Solar Physics, 295 (3). p. 42. ISSN 0038-0938 https://doi.org/10.1007/s11207-019-1404-z doi:10.1007/s11207-019-1404-z
institution Universiti Malaya
building UM Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Malaya
content_source UM Research Repository
url_provider http://eprints.um.edu.my/
topic Q Science (General)
QC Physics
spellingShingle Q Science (General)
QC Physics
Pauzi, F.A.M.
Abidin, Zamri Zainal
Guo, Shao Jie
Gao, Guan Nan
Dong, L.
Monstein, Christian
Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts
description An investigation into Type II solar radio bursts was carried out to understand the frequency gap between fundamental and harmonic emissions of the radio burst. This investigation focused on Type II solar radio bursts with flares and coronal mass ejections by relating the separation between fundamental and harmonic emissions. We used the Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Spectrometers (CALLISTO) and a newly designed low-frequency antenna array. This article describes the proposed new instrument in terms of its antenna design, the bandpass testing of the antenna, the new system significance in studying Type II solar radio bursts, and its comparison with other leading radio solar monitoring instruments. Upon setting up the new technology, the radio-frequency interference of the observation site at the University of Malaya was shown to emphasize the suitability of the selected site. This article also shows the preliminary results of the proposed new instrument by reporting the detection of a Type III solar radio burst that was confirmed by CALLISTO. Moreover, it also includes the optimal observation design and strategies for future detections. © 2020, Springer Nature B.V.
format Article
author Pauzi, F.A.M.
Abidin, Zamri Zainal
Guo, Shao Jie
Gao, Guan Nan
Dong, L.
Monstein, Christian
author_facet Pauzi, F.A.M.
Abidin, Zamri Zainal
Guo, Shao Jie
Gao, Guan Nan
Dong, L.
Monstein, Christian
author_sort Pauzi, F.A.M.
title Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts
title_short Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts
title_full Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts
title_fullStr Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts
title_full_unstemmed Investigation into CME Shock Speed Resulting from Type II Solar Radio Bursts
title_sort investigation into cme shock speed resulting from type ii solar radio bursts
publisher Springer
publishDate 2020
url http://eprints.um.edu.my/25407/
https://doi.org/10.1007/s11207-019-1404-z
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score 13.211869