Population density effect on Radio Frequencies Interference (RFI) in radio astronomy

Radio astronomical observation is infected by wide range of Radio Frequency Interference (RFI). We will also use information gathered from on-site RFI level measurements on selected 'good' areas generated by this study. After investigating a few suitable sites we will commence to the site...

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Published in:AIP Conference Proceedings
Main Author: Umar R.; Abidin Z.Z.; Ibrahim Z.A.; Hassan M.S.R.; Rosli Z.; Hamidi Z.S.
Format: Conference paper
Language:English
Published: American Institute of Physics Inc. 2011
Online Access:https://www.scopus.com/inward/record.uri?eid=2-s2.0-84867394502&doi=10.1063%2f1.4730683&partnerID=40&md5=cc8dc13c8283b4cde39fc0d6f9805cf6
id 2-s2.0-84867394502
spelling 2-s2.0-84867394502
Umar R.; Abidin Z.Z.; Ibrahim Z.A.; Hassan M.S.R.; Rosli Z.; Hamidi Z.S.
Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
2011
AIP Conference Proceedings
1454
1
10.1063/1.4730683
https://www.scopus.com/inward/record.uri?eid=2-s2.0-84867394502&doi=10.1063%2f1.4730683&partnerID=40&md5=cc8dc13c8283b4cde39fc0d6f9805cf6
Radio astronomical observation is infected by wide range of Radio Frequency Interference (RFI). We will also use information gathered from on-site RFI level measurements on selected 'good' areas generated by this study. After investigating a few suitable sites we will commence to the site and construct the RFI observation. Eventually, the best area we will be deciding from the observations soon. The result of this experiment will support our planning to build the first radio telescope in Malaysia. Radio observatories normally are located in remote area, in order to combat RFI from active spectrum users and radio noise produced in industrial or residential areas. The other solution for this problem is regulating the use of radio frequencies in the country (spectrum management). Measurement of RFI level on potential radio astronomical site can be done to measure the RFI levels at sites. Seven sites are chosen divide by three group, which is A, B and C. In this paper, we report the initial testing RFI survey for overall spectrum (0-2GHz) for those sites. The averaged RFI level above noise level at the three group sites are 19.0 (±1.79) dBm, 19.5 (±3.71) dBm and 17.0 (±3.71) dBm and the averaged RFI level above noise level for without main peaks are 20.1 (±1.77) dBm, 19.6 (±3.65) dBm and 17.2 (±1.43) dBm respectively. © 2012 American Institute of Physics.
American Institute of Physics Inc.
0094243X
English
Conference paper

author Umar R.; Abidin Z.Z.; Ibrahim Z.A.; Hassan M.S.R.; Rosli Z.; Hamidi Z.S.
spellingShingle Umar R.; Abidin Z.Z.; Ibrahim Z.A.; Hassan M.S.R.; Rosli Z.; Hamidi Z.S.
Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
author_facet Umar R.; Abidin Z.Z.; Ibrahim Z.A.; Hassan M.S.R.; Rosli Z.; Hamidi Z.S.
author_sort Umar R.; Abidin Z.Z.; Ibrahim Z.A.; Hassan M.S.R.; Rosli Z.; Hamidi Z.S.
title Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
title_short Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
title_full Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
title_fullStr Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
title_full_unstemmed Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
title_sort Population density effect on Radio Frequencies Interference (RFI) in radio astronomy
publishDate 2011
container_title AIP Conference Proceedings
container_volume 1454
container_issue 1
doi_str_mv 10.1063/1.4730683
url https://www.scopus.com/inward/record.uri?eid=2-s2.0-84867394502&doi=10.1063%2f1.4730683&partnerID=40&md5=cc8dc13c8283b4cde39fc0d6f9805cf6
description Radio astronomical observation is infected by wide range of Radio Frequency Interference (RFI). We will also use information gathered from on-site RFI level measurements on selected 'good' areas generated by this study. After investigating a few suitable sites we will commence to the site and construct the RFI observation. Eventually, the best area we will be deciding from the observations soon. The result of this experiment will support our planning to build the first radio telescope in Malaysia. Radio observatories normally are located in remote area, in order to combat RFI from active spectrum users and radio noise produced in industrial or residential areas. The other solution for this problem is regulating the use of radio frequencies in the country (spectrum management). Measurement of RFI level on potential radio astronomical site can be done to measure the RFI levels at sites. Seven sites are chosen divide by three group, which is A, B and C. In this paper, we report the initial testing RFI survey for overall spectrum (0-2GHz) for those sites. The averaged RFI level above noise level at the three group sites are 19.0 (±1.79) dBm, 19.5 (±3.71) dBm and 17.0 (±3.71) dBm and the averaged RFI level above noise level for without main peaks are 20.1 (±1.77) dBm, 19.6 (±3.65) dBm and 17.2 (±1.43) dBm respectively. © 2012 American Institute of Physics.
publisher American Institute of Physics Inc.
issn 0094243X
language English
format Conference paper
accesstype
record_format scopus
collection Scopus
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