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Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study

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@article{IJASEIT1177,
   author = {Marhamah Mohd Shafie and Roslan Umar and Nor Hazmin Sabri and Nur Zulaikha Mohd Afandi and Zainol Abidin Ibrahim},
   title = {Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study},
   journal = {International Journal on Advanced Science, Engineering and Information Technology},
   volume = {7},
   number = {4},
   year = {2017},
   pages = {1441--1447},
   keywords = {radio frequency interference; solar radio burst; e-CALLISTO; spectrum survey},
   abstract = {Solar radio burst study is one of the new researches done in radio astronomy field in Malaysia. Solar radio burst is associated with Coronal Mass Ejections (CMEs). It occurs when magnetic storm collides with Earth’s magnetosphere. In this paper, we present the level of radio frequency interference (RFI) at selected sites in Malaysia; ESERI (ECE), Balai Cerap KUSZA (BCK), Sungai Chantek (SGC) and Hentian Serdang (HSRDG) focusing on wideband (30kHz-1000 MHz. The threshold for all selected sites is -76.3741 dBm (7.3887), -74.4022 dBm (9.8143), -73.736 dBm (9.4494) and -66.4082 dBm (13.4290) respectively. This study was done to survey the status of frequency allocation in Malaysia for radio astronomy study. In this frequency ranges, radio astronomical sources found are pulsar, deuterium line (DI) and solar radio burst. These radio astronomical sources can be studied best at BCK compared to other sites. This is important to radio astronomer in Malaysia especially in solar burst detection to identify the best site for observation. This study also may provide RFI database to radio astronomers to refer to before conducting an observation.},
   issn = {2088-5334},
   publisher = {INSIGHT - Indonesian Society for Knowledge and Human Development},
   url = {http://ijaseit.insightsociety.org/index.php?option=com_content&view=article&id=9&Itemid=1&article_id=1177},
   doi = {10.18517/ijaseit.7.4.1177}
}

EndNote

%A Shafie, Marhamah Mohd
%A Umar, Roslan
%A Sabri, Nor Hazmin
%A Mohd Afandi, Nur Zulaikha
%A Ibrahim, Zainol Abidin
%D 2017
%T Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study
%B 2017
%9 radio frequency interference; solar radio burst; e-CALLISTO; spectrum survey
%! Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study
%K radio frequency interference; solar radio burst; e-CALLISTO; spectrum survey
%X Solar radio burst study is one of the new researches done in radio astronomy field in Malaysia. Solar radio burst is associated with Coronal Mass Ejections (CMEs). It occurs when magnetic storm collides with Earth’s magnetosphere. In this paper, we present the level of radio frequency interference (RFI) at selected sites in Malaysia; ESERI (ECE), Balai Cerap KUSZA (BCK), Sungai Chantek (SGC) and Hentian Serdang (HSRDG) focusing on wideband (30kHz-1000 MHz. The threshold for all selected sites is -76.3741 dBm (7.3887), -74.4022 dBm (9.8143), -73.736 dBm (9.4494) and -66.4082 dBm (13.4290) respectively. This study was done to survey the status of frequency allocation in Malaysia for radio astronomy study. In this frequency ranges, radio astronomical sources found are pulsar, deuterium line (DI) and solar radio burst. These radio astronomical sources can be studied best at BCK compared to other sites. This is important to radio astronomer in Malaysia especially in solar burst detection to identify the best site for observation. This study also may provide RFI database to radio astronomers to refer to before conducting an observation.
%U http://ijaseit.insightsociety.org/index.php?option=com_content&view=article&id=9&Itemid=1&article_id=1177
%R doi:10.18517/ijaseit.7.4.1177
%J International Journal on Advanced Science, Engineering and Information Technology
%V 7
%N 4
%@ 2088-5334

IEEE

Marhamah Mohd Shafie,Roslan Umar,Nor Hazmin Sabri,Nur Zulaikha Mohd Afandi and Zainol Abidin Ibrahim,"Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study," International Journal on Advanced Science, Engineering and Information Technology, vol. 7, no. 4, pp. 1441-1447, 2017. [Online]. Available: http://dx.doi.org/10.18517/ijaseit.7.4.1177.

RefMan/ProCite (RIS)

TY  - JOUR
AU  - Shafie, Marhamah Mohd
AU  - Umar, Roslan
AU  - Sabri, Nor Hazmin
AU  - Mohd Afandi, Nur Zulaikha
AU  - Ibrahim, Zainol Abidin
PY  - 2017
TI  - Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study
JF  - International Journal on Advanced Science, Engineering and Information Technology; Vol. 7 (2017) No. 4
Y2  - 2017
SP  - 1441
EP  - 1447
SN  - 2088-5334
PB  - INSIGHT - Indonesian Society for Knowledge and Human Development
KW  - radio frequency interference; solar radio burst; e-CALLISTO; spectrum survey
N2  - Solar radio burst study is one of the new researches done in radio astronomy field in Malaysia. Solar radio burst is associated with Coronal Mass Ejections (CMEs). It occurs when magnetic storm collides with Earth’s magnetosphere. In this paper, we present the level of radio frequency interference (RFI) at selected sites in Malaysia; ESERI (ECE), Balai Cerap KUSZA (BCK), Sungai Chantek (SGC) and Hentian Serdang (HSRDG) focusing on wideband (30kHz-1000 MHz. The threshold for all selected sites is -76.3741 dBm (7.3887), -74.4022 dBm (9.8143), -73.736 dBm (9.4494) and -66.4082 dBm (13.4290) respectively. This study was done to survey the status of frequency allocation in Malaysia for radio astronomy study. In this frequency ranges, radio astronomical sources found are pulsar, deuterium line (DI) and solar radio burst. These radio astronomical sources can be studied best at BCK compared to other sites. This is important to radio astronomer in Malaysia especially in solar burst detection to identify the best site for observation. This study also may provide RFI database to radio astronomers to refer to before conducting an observation.
UR  - http://ijaseit.insightsociety.org/index.php?option=com_content&view=article&id=9&Itemid=1&article_id=1177
DO  - 10.18517/ijaseit.7.4.1177

RefWorks

RT Journal Article
ID 1177
A1 Shafie, Marhamah Mohd
A1 Umar, Roslan
A1 Sabri, Nor Hazmin
A1 Mohd Afandi, Nur Zulaikha
A1 Ibrahim, Zainol Abidin
T1 Radio Environment Analysis at Balai Cerap KUSZA for Solar Burst Study
JF International Journal on Advanced Science, Engineering and Information Technology
VO 7
IS 4
YR 2017
SP 1441
OP 1447
SN 2088-5334
PB INSIGHT - Indonesian Society for Knowledge and Human Development
K1 radio frequency interference; solar radio burst; e-CALLISTO; spectrum survey
AB Solar radio burst study is one of the new researches done in radio astronomy field in Malaysia. Solar radio burst is associated with Coronal Mass Ejections (CMEs). It occurs when magnetic storm collides with Earth’s magnetosphere. In this paper, we present the level of radio frequency interference (RFI) at selected sites in Malaysia; ESERI (ECE), Balai Cerap KUSZA (BCK), Sungai Chantek (SGC) and Hentian Serdang (HSRDG) focusing on wideband (30kHz-1000 MHz. The threshold for all selected sites is -76.3741 dBm (7.3887), -74.4022 dBm (9.8143), -73.736 dBm (9.4494) and -66.4082 dBm (13.4290) respectively. This study was done to survey the status of frequency allocation in Malaysia for radio astronomy study. In this frequency ranges, radio astronomical sources found are pulsar, deuterium line (DI) and solar radio burst. These radio astronomical sources can be studied best at BCK compared to other sites. This is important to radio astronomer in Malaysia especially in solar burst detection to identify the best site for observation. This study also may provide RFI database to radio astronomers to refer to before conducting an observation.
LK http://ijaseit.insightsociety.org/index.php?option=com_content&view=article&id=9&Itemid=1&article_id=1177
DO  - 10.18517/ijaseit.7.4.1177