Indication of Radio Frequency Interference (RFI) Sources for Solar Burst Monitoring in Malaysia

被引：5
|
作者：
Hamidi, Z. S. [1 ,2 ]
Abidin, Z. Z. [2 ]
Ibrahim, Z. A. [2 ]
Shariff, N. N. M. [2 ]
机构：
[1] Univ Teknol MARA, Fac Sci Appl, Uitm S Alam Selangor, Malaysia
[2] Univ Malaya, Fac Sci, Kuala Lumpur, Malaysia
来源：
INTERNATIONAL CONFERENCE ON PHYSICS AND ITS APPLICATIONS (ICPAP 2011) | 2012年 / 1454卷
关键词：
Radio Frequency Interference (RFI); radio astronomy; RFI sources;
D O I：
10.1063/1.4730684
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
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.
引用
收藏
页码：43 / 46
页数：4
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