Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia

Apart of monitoring the Sun project, the Radio Frequency Interference (RFI) surveying in the region of (1-1200) MHz has been conducted. The main objective of this surveying is to test and qualify the potential of monitoring a continuous radio emission of Solar in Malaysia. This work is also an initi...

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Main Authors: Hamidi, Z.S., Abidin, Z.Z., Ibrahim, Z.A., Shariff, N.N.M.
Format: Article
Published: American Institute of Physics 2012
Subjects:
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author Hamidi, Z.S.
Abidin, Z.Z.
Ibrahim, Z.A.
Shariff, N.N.M.
author_facet Hamidi, Z.S.
Abidin, Z.Z.
Ibrahim, Z.A.
Shariff, N.N.M.
author_sort Hamidi, Z.S.
collection UM
description Apart of monitoring the Sun project, the Radio Frequency Interference (RFI) surveying in the region of (1-1200) MHz has been conducted. The main objective of this surveying is to test and qualify the potential of monitoring a continuous radio emission of Solar in Malaysia. This work is also an initiative of International Space Weather Initiative (ISWI) project where Malaysia is one of the country that participate a e-Callisto Spectrometer network in order to study the behavior of Solar radio burst in frequency of (45-800) MHz region which will be install in this October. Detail results will indicate the potential of monitoring a solar in Malaysia.
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spelling um.eprints-146022019-12-06T09:13:59Z http://eprints.um.edu.my/14602/ Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia Hamidi, Z.S. Abidin, Z.Z. Ibrahim, Z.A. Shariff, N.N.M. Q Science (General) Apart of monitoring the Sun project, the Radio Frequency Interference (RFI) surveying in the region of (1-1200) MHz has been conducted. The main objective of this surveying is to test and qualify the potential of monitoring a continuous radio emission of Solar in Malaysia. This work is also an initiative of International Space Weather Initiative (ISWI) project where Malaysia is one of the country that participate a e-Callisto Spectrometer network in order to study the behavior of Solar radio burst in frequency of (45-800) MHz region which will be install in this October. Detail results will indicate the potential of monitoring a solar in Malaysia. American Institute of Physics 2012 Article PeerReviewed Hamidi, Z.S. and Abidin, Z.Z. and Ibrahim, Z.A. and Shariff, N.N.M. (2012) Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia. AIP Conference Proceedings, 1454 (43). ISSN 0094-243X, DOI https://doi.org/10.1063/1.4730684 <https://doi.org/10.1063/1.4730684>. http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4730684 http://dx.doi.org/10.1063/1.4730684
spellingShingle Q Science (General)
Hamidi, Z.S.
Abidin, Z.Z.
Ibrahim, Z.A.
Shariff, N.N.M.
Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
title Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
title_full Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
title_fullStr Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
title_full_unstemmed Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
title_short Indication of radio frequency interference (RFI) sources for solar burst monitoring in Malaysia
title_sort indication of radio frequency interference rfi sources for solar burst monitoring in malaysia
topic Q Science (General)
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