How can we create flare-prolific active regions on the Sun?

Toriumi, Shin

doi:10.57757/IUGG23-1342

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Conference Paper

How can we create flare-prolific active regions on the Sun?

Authors

Toriumi, Shin
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Toriumi, S. (2023): How can we create flare-prolific active regions on the Sun?, XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG) (Berlin 2023).
https://doi.org/10.57757/IUGG23-1342

Cite as: https://gfzpublic.gfz.de/pubman/item/item_5017257

Abstract

Solar flares and coronal mass ejections, especially the stronger ones, are known to occur in active regions of the Sun. Therefore, understanding how such source regions are created and evolve is important not only for solar and heliophysics but also in view of space weather forecasting. In this presentation, we review the key observations and state-of-the-art numerical modeling of emergence and evolution of flare-prolific active regions. We also discuss what science can be achieved on this issue by the next-generation missions in the 2020s, represented by JAXA's SOLAR-C mission.