The Solar Activity Monitor Network - SAMNet
文献类型：期刊论文
| 作者 | Erdelyi, Robertus12,13,14; Korsos, Marianna B.13,14,15; Huang, Xin16; Yang, Yong17; Pizzey, Danielle18; Wrathmall, Steven A.18; Hughes, Ifan G.18; Dyer, Martin J.19; Dhillon, Vikram S.19,20; Belucz, Bernadett13,14 |
| 刊名 | Journal of Space Weather and Space Climate
 |
| 出版日期 | 2022 |
| 卷号 | 12页码:212 |
| ISSN号 | 2115-7251 |
| 关键词 | Sun flares precursors magneto-optical filter space weather flare doppler fields instrument prediction velocity line sun Astronomy & Astrophysics Geochemistry & Geophysics Meteorology & Atmospheric Sciences |
| DOI | 10.1051/swsc/2021025 |
| 产权排序 | 27 |
| 文献子类 | Article |
| 英文摘要 | The Solar Activity Magnetic Monitor (SAMM) Network (SAMNet) is a future UK-led international network of ground-based solar telescope stations. SAMNet, at its full capacity, will continuously monitor the Sun's intensity, magnetic, and Doppler velocity fields at multiple heights in the solar atmosphere (from photosphere to upper chromosphere). Each SAMM sentinel will be equipped with a cluster of identical telescopes each with a different magneto-optical filter (MOFs) to take observations in K I, Na D, and Ca I spectral bands. A subset of SAMM stations will have white-light coronagraphs and emission line coronal spectropolarimeters. The objectives of SAMNet are to provide observational data for space weather research and forecast. The goal is to achieve an operationally sufficient lead time of e.g., flare warning of 2-8 h and provide many sought-after continuous synoptic maps (e.g., LoS magnetic and velocity fields, intensity) of the lower solar atmosphere with a spatial resolution limited only by seeing or diffraction limit, and with a cadence of 10 min. The individual SAMM sentinels will be connected to their master HQ hub where data received from all the slave stations will be automatically processed and flare warning issued up to 26 h in advance. |
| 语种 | 英语 |
| WOS记录号 | WOS:000746925900001 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/5131]  |
| 专题 | 太阳物理研究室_太阳物理研究团组 |
| 作者单位 | 1.School of Natural Sciences and Medicine, Ilia State Univ., Cholokashvili Ave. 3/5, Tbilisi 0162, Georgia; 2.School of Astronomy and Space Science, Univ. of Chinese Acad. of Sciences, Beijing 100049, PR China; 3.CAS Center for Excellence in Comparative Planetology, USTC, Hefei 230026, PR China; 4.CAS Key Laboratory of Geospace Environment, School of Earth and Space Sciences, Univesity of Science and Technology of China, Hefei 230026, PR China; 5.Instituto de Astrofsica de Andaluca, Granada 18008, Spain; 6.Xinjiang Astromomical Observatory, CAS, 150 Science 1-Street, Urumqi 830011, PR China; 7.Kislovodsk Solar Mountain Astronomical Station, Central Astronomical Observatory of the Russian Academy of Sciences, Kislovodsk 357700, Russia; 8.Observatorio AstroExplor, Cra 58C 152B-22, Bogota, Colombia; 9.Pulkovo Astronomical Observatory, Russian Academy of Sciences, Saint Petersburg 196140, Russian Federation; 10.Kanzelhöhe Observatory for Solar and Environmental Research, University of Graz, Kanzelhöhe 19, Treffen 9521, Austria; |
| 推荐引用方式 GB/T 7714 | Erdelyi, Robertus,Korsos, Marianna B.,Huang, Xin,et al. The Solar Activity Monitor Network - SAMNet[J]. Journal of Space Weather and Space Climate,2022,12:212. |
| APA | Erdelyi, Robertus.,Korsos, Marianna B..,Huang, Xin.,Yang, Yong.,Pizzey, Danielle.,...&Zuccarello, Francesca.(2022).The Solar Activity Monitor Network - SAMNet.Journal of Space Weather and Space Climate,12,212. |
| MLA | Erdelyi, Robertus,et al."The Solar Activity Monitor Network - SAMNet".Journal of Space Weather and Space Climate 12(2022):212. |
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