摘要: Ground-based synoptic solar observations provide critical contextual data
used to model the large-scale state of the heliosphere. The next decade will
see a combination of ground-based telescopes and space missions that will study
our Sun's atmosphere microscopic processes with unprecedented detail. This
white paper describes contextual observations from a ground-based network
needed to fully exploit this new knowledge of the underlying physics that leads
to the magnetic linkages between the heliosphere and the Sun. This combination
of a better understanding of small-scale processes and the appropriate global
context will enable a physics-based approach to Space Weather comparable to
Terrestrial Weather forecasting.
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分类:
天文学
>>
天文学
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引用:
ChinaXiv:202303.02712
(或此版本
ChinaXiv:202303.02712V1)
DOI:10.12074/202303.02712V1
CSTR:32003.36.ChinaXiv.202303.02712.V1
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科创链TXID:
814ecd0f-b0f3-4f20-aaa6-fe648d5f6ae0
- 推荐引用方式:
Sanjay Gosain,V. Martinez Pillet,A. Pevtsov,H. Gilbert,S. Gibson,A. G. de Wijn,J. Burkepile,A. Asai,H. M. Bain,C. J. Henney,Y. Katsukawa,H. Lin,W. Manchester,J. McAteer,K. Muglach,M. Rast,M. Roth,J. Zhang.Ground-based Synoptic Studies of the Sun.中国科学院科技论文预发布平台.[ChinaXiv:202303.02712V1]
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