The Solar Activity Monitor Network – SAMNet
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 atmospher...
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EDP Sciences
2022-01-01
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Series: | Journal of Space Weather and Space Climate |
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Online Access: | https://www.swsc-journal.org/articles/swsc/full_html/2022/01/swsc200065/swsc200065.html |
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author | Erdélyi Robertus Korsós Marianna B. Huang Xin Yang Yong Pizzey Danielle Wrathmall Steven A. Hughes Ifan G. Dyer Martin J. Dhillon Vikram S. Belucz Bernadett Brajša Roman Chatterjee Piyali Cheng Xuewu Deng Yuanyong Domínguez Santiago Vargas Joya Raúl Gömöry Peter Gyenge Norbert G. Hanslmeier Arnold Kucera Ales Kuridze David Li Faquan Liu Zhong Xu Long Mathioudakis Mihalis Matthews Sarah McAteer James R.T. Pevtsov Alexei A. Pötzi Werner Romano Paolo Shen Jinhua Temesváry János Tlatov Andrey G. Triana Charles Utz Dominik Veronig Astrid M. Wang Yuming Yan Yihua Zaqarashvili Teimuraz Zuccarello Francesca |
author_facet | Erdélyi Robertus Korsós Marianna B. Huang Xin Yang Yong Pizzey Danielle Wrathmall Steven A. Hughes Ifan G. Dyer Martin J. Dhillon Vikram S. Belucz Bernadett Brajša Roman Chatterjee Piyali Cheng Xuewu Deng Yuanyong Domínguez Santiago Vargas Joya Raúl Gömöry Peter Gyenge Norbert G. Hanslmeier Arnold Kucera Ales Kuridze David Li Faquan Liu Zhong Xu Long Mathioudakis Mihalis Matthews Sarah McAteer James R.T. Pevtsov Alexei A. Pötzi Werner Romano Paolo Shen Jinhua Temesváry János Tlatov Andrey G. Triana Charles Utz Dominik Veronig Astrid M. Wang Yuming Yan Yihua Zaqarashvili Teimuraz Zuccarello Francesca |
author_sort | Erdélyi Robertus |
collection | DOAJ |
description | 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. |
first_indexed | 2024-12-20T14:58:18Z |
format | Article |
id | doaj.art-bb3757f31cdd4bd883696c991a0a4d01 |
institution | Directory Open Access Journal |
issn | 2115-7251 |
language | English |
last_indexed | 2024-12-20T14:58:18Z |
publishDate | 2022-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | Journal of Space Weather and Space Climate |
spelling | doaj.art-bb3757f31cdd4bd883696c991a0a4d012022-12-21T19:36:45ZengEDP SciencesJournal of Space Weather and Space Climate2115-72512022-01-0112210.1051/swsc/2021025swsc200065The Solar Activity Monitor Network – SAMNetErdélyi Robertus0https://orcid.org/0000-0003-3439-4127Korsós Marianna B.1https://orcid.org/0000-0001-8696-9856Huang Xin2https://orcid.org/0000-0003-0569-5932Yang YongPizzey Danielle3https://orcid.org/0000-0002-9025-8608Wrathmall Steven A.4https://orcid.org/0000-0003-1770-9721Hughes Ifan G.5https://orcid.org/0000-0001-6322-6435Dyer Martin J.6https://orcid.org/0000-0003-3665-5482Dhillon Vikram S.7https://orcid.org/0000-0003-4236-9642Belucz Bernadett8Brajša Roman9Chatterjee Piyali10Cheng XuewuDeng Yuanyong11Domínguez Santiago Vargas12https://orcid.org/0000-0002-5999-4842Joya Raúl13https://orcid.org/0000-0001-6264-4467Gömöry Peter14https://orcid.org/0000-0002-0473-4103Gyenge Norbert G.15Hanslmeier Arnold16Kucera Ales17Kuridze David18Li FaquanLiu Zhong19Xu Long20https://orcid.org/0000-0002-9286-2876Mathioudakis Mihalis21Matthews Sarah22https://orcid.org/0000-0001-9346-8179McAteer James R.T.23https://orcid.org/0000-0003-1493-101XPevtsov Alexei A.24https://orcid.org/0000-0003-0489-0920Pötzi Werner25https://orcid.org/0000-0003-4811-0543Romano Paolo26https://orcid.org/0000-0001-7066-6674Shen Jinhua27Temesváry János28Tlatov Andrey G.29https://orcid.org/0000-0003-1545-2125Triana Charles30https://orcid.org/0000-0001-6961-0454Utz Dominik31Veronig Astrid M.32https://orcid.org/0000-0003-2073-002XWang Yuming33Yan Yihua34https://orcid.org/0000-0002-7106-6029Zaqarashvili Teimuraz35Zuccarello Francesca36https://orcid.org/0000-0003-1853-2550Solar Physics & Space Plasma Research Center (SP2RC), School of Mathematics and Statistics, University of SheffieldDepartment of Astronomy, Eötvös Loránd Univ.CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of SciencesJoint Quantum Centre (JQC) Durham-Newcastle, Department of Physics, Durham UniversityJoint Quantum Centre (JQC) Durham-Newcastle, Department of Physics, Durham UniversityJoint Quantum Centre (JQC) Durham-Newcastle, Department of Physics, Durham UniversityDepartment of Physics and Astronomy, University of SheffieldDepartment of Physics and Astronomy, University of SheffieldDepartment of Astronomy, Eötvös Loránd Univ.Hvar Observatory, Faculty of Geodesy, Univ. of ZagrebIndian Institute of Astrophysics (IIA)CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of SciencesObservatorio Astronómico Nacional, Universidad Nacional de ColombiaObservatorio Astronómico, Universidad Sergio ArboledaAstronomical Institute, Slovak Academy of SciencesSolar Physics & Space Plasma Research Center (SP2RC), School of Mathematics and Statistics, University of SheffieldInstitute of Physics, University of GrazAstronomical Institute, Slovak Academy of SciencesDepartment of Physics, Aberystwyth UniversityYunnan Observatories, Chinese Academy of SciencesCAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of SciencesAstrophysics Research Centre, School of Mathematics and Physics, Queen’s University BelfastUCL-Mullard Space Science Lab.Department of Astronomy, New Mexico State UnivNational Solar ObservatoryKanzelhöhe Observatory for Solar and Environmental Research, University of GrazINAF Osservatorio Astrofisico di CataniaXinjiang Astromomical Observatory, CASGyula Bay Zoltán Solar Observatory (GSO), Hungarian Solar Physics Foundation (HSPF)Kislovodsk Solar Mountain Astronomical Station, Central Astronomical Observatory of the Russian Academy of SciencesObservatorio AstroExplorInstitute of Physics, University of GrazInstitute of Physics, University of GrazCAS Key Laboratory of Geospace Environment, School of Earth and Space Sciences, Univesity of Science and Technology of ChinaCAS Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of SciencesInstitute of Physics, University of GrazDipartimento di Fisica e Astronomia “Ettore Majorana”, Universitá di CataniaThe 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.https://www.swsc-journal.org/articles/swsc/full_html/2022/01/swsc200065/swsc200065.htmlsun-flares-precursors |
spellingShingle | Erdélyi Robertus Korsós Marianna B. Huang Xin Yang Yong Pizzey Danielle Wrathmall Steven A. Hughes Ifan G. Dyer Martin J. Dhillon Vikram S. Belucz Bernadett Brajša Roman Chatterjee Piyali Cheng Xuewu Deng Yuanyong Domínguez Santiago Vargas Joya Raúl Gömöry Peter Gyenge Norbert G. Hanslmeier Arnold Kucera Ales Kuridze David Li Faquan Liu Zhong Xu Long Mathioudakis Mihalis Matthews Sarah McAteer James R.T. Pevtsov Alexei A. Pötzi Werner Romano Paolo Shen Jinhua Temesváry János Tlatov Andrey G. Triana Charles Utz Dominik Veronig Astrid M. Wang Yuming Yan Yihua Zaqarashvili Teimuraz Zuccarello Francesca The Solar Activity Monitor Network – SAMNet Journal of Space Weather and Space Climate sun-flares-precursors |
title | The Solar Activity Monitor Network – SAMNet |
title_full | The Solar Activity Monitor Network – SAMNet |
title_fullStr | The Solar Activity Monitor Network – SAMNet |
title_full_unstemmed | The Solar Activity Monitor Network – SAMNet |
title_short | The Solar Activity Monitor Network – SAMNet |
title_sort | solar activity monitor network samnet |
topic | sun-flares-precursors |
url | https://www.swsc-journal.org/articles/swsc/full_html/2022/01/swsc200065/swsc200065.html |
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