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
Referencia bibliográfica

Solar Physics

Fecha de publicación:
5
2025
Revista
Solar Physics
Número de autores
46
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Con árbitro
Heliosismología
Campos magnéticos
Manchas solares

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