Decimetric and metric digital solar radio spectrometers of the Yunnan Astronomical Observatories and the first-light results | |
Gao GN(高冠男)1,2,3; Wang M(汪敏)1,3,4; Dong L(董亮)1,4; Wu, N5; Lin J(林隽)1 | |
刊名 | NEW ASTRONOMY |
2014-07 | |
卷号 | 30页码:68-78 |
关键词 | Instrument: radio spectrometer Sun: radio bursts Sun: fine structures |
ISSN号 | 1384-1076 |
通讯作者 | Gao, G (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | Based on an old decimetric solar radio spectrometer working in the frequency range of 625-1500 MHz of the Yunnan Astronomical Observatories (YNAO) during the last solar cycle, we designed a fully digital Fast Fourier Transform (FFT) spectrometer to upgrade the old one. The new digital spectrometer has the spectral resolution of 200 kHz, much higher than the old one (about 1.3 MHz). In addition, we also established a new metric solar radio telescope working in the frequency range of 70-700 MHz located at the Fuxian Solar Observatory of YNAO, deploying the same type of the digital FFT spectrometer. The two instruments have begun to operate in a daily survey mode since September 2009 and March 2012, respectively, and many solar radio bursts have been observed. In these events, various types of decimetric and metric fine structures with fairly meticulous spectral features were recognized. These features were never resolved in previous observation and studies. We have introduced these two instruments with their detailed technological components, as well as a set of observational data obtained during the first-light of the instruments. The information revealed by these data can improve our knowledge and understanding of the physics of the energy conversion, particle acceleration and transportation during the solar eruption. (C) 2014 Elsevier B.V. All rights reserved. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | FINE-STRUCTURES ; MAGNETIC RECONNECTION ; II BURSTS ; CHROMOSPHERIC EVAPORATION ; INTERPLANETARY SPACE ; ZEBRA PATTERNS ; DECEMBER 1 ; FLARE ; EMISSION ; BAND |
收录类别 | SCI |
原文出处 | http://www.sciencedirect.com/science/article/pii/S1384107614000153 |
语种 | 英语 |
WOS记录号 | WOS:000333493100009 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5630] |
专题 | 云南天文台_射电天文研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.Yunnan Observatory, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 2.University of Chinese Academy of Sciences, Beijing 100049, China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatory, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 4.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 5.School of Tourism and Geography, Yunnan Normal University, Kunming, Yunnan 650031, China |
推荐引用方式 GB/T 7714 | Gao GN,Wang M,Dong L,et al. Decimetric and metric digital solar radio spectrometers of the Yunnan Astronomical Observatories and the first-light results[J]. NEW ASTRONOMY,2014,30:68-78. |
APA | Gao GN,Wang M,Dong L,Wu, N,&Lin J.(2014).Decimetric and metric digital solar radio spectrometers of the Yunnan Astronomical Observatories and the first-light results.NEW ASTRONOMY,30,68-78. |
MLA | Gao GN,et al."Decimetric and metric digital solar radio spectrometers of the Yunnan Astronomical Observatories and the first-light results".NEW ASTRONOMY 30(2014):68-78. |
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