Structure and Dynamics of the Sun's Interior Revealed by the Helioseismic and Magnetic Imager

Bibcode
2025SoPh..300...70K
DOI
10.1007/s11207-025-02480-6
Kosovichev, Alexander G.; Basu, Sarbani; Bekki, Yuto; Buitrago-Casas, Juan Camilo; Chatzistergos, Theodosios; Chen, Ruizhu; Christensen-Dalsgaard, Jørgen; Donea, Alina; Fleck, Bernhard; Fournier, Damien; García, Rafael A.; Getling, Alexander V.; Gizon, Laurent; Gough, Douglas O.; Hanasoge, Shravan; Hanson, Chris S.; Hess Webber, Shea A.; Hoeksema, J. Todd; Howe, Rachel; Jain, Kiran; Kasapis, Spiridon; Kashyap, Samarth G.; Kitiashvili, Irina N.; Komm, Rudolf; Korzennik, Sylvain G.; Krivova, Natalie A.; Kuhn, Jeffrey R.; Liang, Zhi-Chao; Lindsey, Charles; Mahajan, Sushant S.; Mandal, Krishnendu; Mani, Prasad; Martinez Oliveros, Juan Carlos; Mathur, Savita; Rabello Soares, M. Cristina; Rajaguru, S. Paul; Reiter, Johann; Rhodes, Edward J.; Rozelot, Jean-Pierre; Scherrer, Philip H.; Solanki, Sami K.; Stefan, John T.; Toomre, Juri; Tripathy, Sushanta C.; Upton, Lisa A.; Zhao, Junwei
Bibliographical reference

Solar Physics

Advertised on:
5
2025
Journal
Solar Physics
Number of authors
46
IAC number of authors
1
Citations
0
Refereed citations
0
Description
High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) provide a unique three-dimensional view of the solar interior structure and dynamics, revealing a tremendous complexity of the physical processes inside the Sun. We present an overview of the results of the HMI helioseismology program and discuss their implications for modern theoretical models and simulations of the solar interior.
Type
Refereed
Helioseismology
Magnetic fields
Sunspots

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