Influence Factors of Radio Frequency Interference (RFI) for Solar Radio Astronomy Purpose at National Space Centre

Hamidi, ZS and Shariff, NNM and Umar, Roslan (2012) Influence Factors of Radio Frequency Interference (RFI) for Solar Radio Astronomy Purpose at National Space Centre. Thail Journal of Physics, 3. pp. 235-238.

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Abstract

Important results on the Radio Frequencies Interference (RFI) at National Space Centre, Sg Lang Selangor, Malaysia has been reported. This data has been taken from (1-2000) MHz at the main site of installation e-Callisto system as a part of an initiative of International Space Weather Initiative (ISWI) research. In order to make sure that the data of solar monitoring in radio region is reliable, we need to study the variation of interference and the possible sources that contribute this interference. Our main objective is to qualify the potential of monitoring a continuous radio emission of the Sun. Due to our results as there is low interference in the channel range (1–800) MHz, it would be possible to simply not apply the projection to this portion of the spectrum. This is a good indicator for solar burst monitoring purpose as well as the other astronomical object, generally.

Item Type: Article
Subjects: Q Science > QB Astronomy
Faculty / Institute: Faculty of Contemporary Islamic Studies
Depositing User: Roslan Umar
Date Deposited: 21 Jan 2015 02:24
Last Modified: 21 Jan 2015 02:24
URI: http://erep.unisza.edu.my/id/eprint/1473

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