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
3
Número de citas referidas
3
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.
Proyectos relacionados
Helio y Astroseismología
Sismología Solar y Estelar y Búsqueda de Exoplanetas
Los objetivos principales de este proyecto son: 1) estudiar la estructura y la dinámica del interior solar, 2) ampliar este estudio a otros tipos de estrellas y 3) buqueda de planetas extrasolares utilizando métodos fotométricos y su caracterización con información complementaria (espectrometría). Para alcanzar el primer objetivo, utilizamos la
Savita
Mathur
En ejecución
Tipo
Con árbitro
Física estelar e interestelar (FEEI)
Heliosismología
Campos magnéticos
Manchas solares

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