Analysis of radio astronomy bands using CALLISTO spectrometer at Malaysia-UKM station

被引：3

作者：

Zavvari, Azam ^{[1
]}

Islam, Mohammad Tariqul ^{[1
]}

Anwar, Radial ^{[2
]}

Abidin, Zamri Zainal ^{[3
]}

Asillam, Mhd Fairos ^{[4
]}

Monstein, Christian ^{[5
]}

机构：

[1] Univ Kebangsaan Malaysia, Fac Engn & Built Environm, Dept Elect Elect & Syst Engn, Bangi 43600, Selangor, Malaysia

[2] Univ Kebangsaan Malaysia, Inst Climate Change, Ctr Space Sci, Bangi 43600, Selangor, Malaysia

[3] Univ Malaya, Fac Sci Bldg, Dept Phys, Kuala Lumpur 50603, Selangor, Malaysia

[4] Natl Space Agcy Malaysia ANGKASA, Lot 2233,Kg Sungai Lang, Banting 42700, Selangor, Malaysia

[5] Swiss Fed Inst Technol, Inst Astron, HIT G13-2,Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland

来源：

EXPERIMENTAL ASTRONOMY | 2016年 / 41卷 / 1-2期

关键词：

e-CALLISTO network; Radio astronomy; Sun; Solar radio burst;

D O I：

10.1007/s10686-015-9480-z

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The e-CALLISTO system is a worldwide network that aims to observe solar radio emission for astronomical science. CALLISTO instruments have been deployed worldwide in various locations that together can provide continuous observation of the solar radio spectrum for 24 h per day year-round. Malaysia-UKM is a strategic equatorial location and can observe the Sun 12 h per day. This paper gives an overview of the spectrum allocation for radio astronomy, which falls in the specified operating frequency band of the CALLISTO spectrometer. The radio astronomy bands are analyzed at the Malaysia-UKM station according to the International Telecommunication Union recommendations. Some observational results are also presented in this paper.

引用

页码：185 / 195

页数：11

共 15 条

[1] Analysis of radio astronomy bands using CALLISTO spectrometer at Malaysia-UKM station
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Radial Anwar
Zamri Zainal Abidin
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Christian Monstein
Experimental Astronomy, 2016, 41 : 185 - 195
[2] CALLISTO Radio Spectrometer Construction at Universiti Kebangsaan Malaysia
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