Author ORCID Identifier
James McAteer:
https://orcid.org/0000-0003-1493-101X
Vik Dhillon:
https://orcid.org/0000-0003-4236-9642
Aney Tlatov:
https://orcid.org/0000-0003-1545-2125
Paolo Romano:
https://orcid.org/0000-0001-7066-6674
Yuming Wang:
https://orcid.org/0000-0002-8887-3919
Francesca Zuccarello:
https://orcid.org/0000-0003-1853-2550
Astrid Veronig:
https://orcid.org/0000-0003-2073-002X
robertus erdelyi:
https://orcid.org/0000-0003-3439-4127
Steven Wrathmall:
https://orcid.org/0000-0003-1770-9721
Ifan Hughes:
https://orcid.org/0000-0001-6322-6435
Sarah Matthews:
https://orcid.org/0000-0001-9346-8179
Santiago Vargas Domínguez:
https://orcid.org/0000-0002-5999-4842
Yihua Yan:
https://orcid.org/0000-0002-7106-6029
Martin Dyer:
https://orcid.org/0000-0003-3665-5482
Marianna Korsos:
https://orcid.org/0000-0002-0049-4798
David Kuridze:
https://orcid.org/0000-0003-2760-2311
Danielle Pizzey:
https://orcid.org/0000-0002-9025-8608
Document Type
Journal Article
Journal Article Version
Final Version / Publisher's PDF (peer-reviewed)
Publication Date
1-26-2022
Abstract
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.
Published in
Journal of Space Weather and Space Climate
DOI
10.1051/swsc/2021025
Keywords
Sun, precursors, flares
Department / Organizational Unit
Astronomy
Copyright Notice
© 2022 R. Erdelyi, M. Korsos, X. Huang, et al., reuse allowed according to Creative Commons license.
License for Reuse

This work is licensed under a Creative Commons Attribution 4.0 International License.
Recommended Citation
Erdelyi, R., Korsos, M. B., Huang, X., Yang, Y., Pizzey, D., Wrathmall, S. A., Hughes, I. G., Dyer, M. J., Dhillon, V. S., Belucz, B., Brajsa, R., Chatterjee, P., Cheng, X., Deng, Y., Vargas Dominguez, S., Joya, R., Gomory, P., Gyenge, N. G., Hanslmeier, A., ... Zuccarello, F. (2022). The Solar Activity Monitor Network - SAMNet. Journal of Space Weather and Space Climate, 12. https://doi.org/10.1051/swsc/2021025
Comments
Additional authors: Roman Brajsa; Piyali Chatterjee; Xuewu Cheng; Yuanyong Deng; Santiago Vargas Dominguez; Raul Joya; Peter Gomory; Norbert G. Gyenge; Arnold Hanslmeier; Ales Kucera; David Kuridze; Faquan Li; Zhong Liu; Long Xu; Mihalis Mathioudakis; Sarah Matthews; James R. T. McAteer; Alexei A. Pevtsov; Werner Potzi; Paolo Romano; Jinhua Shen; Janos Temesvary; Andrey G. Tlatov; Charles Triana; Dominik Utz; Astrid M. Veronig; Yuming Wang; Yihua Yan; Teimuraz Zaqarashvili; Francesca Zuccarello