Structure and dynamics of the sun’s interior revealed by the helioseismic and magnetic Imager

Kosovichev, A. G; Basu, S; Bekki, Y; Buitrago-Casas, Juan Camilo; Chatzistergos, Theodosios; Chen, Ruizhu; Christensen-Dalsgaard, J; Donea, Alina; Fleck, Bernhard; Fournier, Damien; Garcia, R. A; Getling, Alexander V; Gizon, L; Gough, Douglas O; Hanasoge, S. M; Hanson, Chris S; Webber, Shea A. Hess; Hoeksema, J. Todd; Howe, Rachel; Jain, K; Kasapis, Spiridon; Kashyap, Samarth G; Kitiashvili, I. N; Komm, R; Korzennik, S. G; Krivova, Natalie A; Kuhn, Jeffrey R; Liang, Zhi-Chao; Lindsey, Charles; Mahajan, Sushant S; Mandal, K; Mani, Prasad; Oliveros, Juan Carlos Martinez; Mathur, S; Soares, M. Cristina Rabello; Rajaguru, S. P; Reiter, Johann; Rhodes Jr., Edward J; Rozelot, J. P; Scherrer, P. H; Solanki, S. K; Stefan, John T; Toomre, Juri; Tripathy, S. C; Upton, Lisa A; Zhao, Junwei

Home
→
IIAP Publications
→
IIAP Publications
→
View Item

Structure and dynamics of the sun’s interior revealed by the helioseismic and magnetic Imager

Kosovichev, A. G; Basu, S; Bekki, Y; Buitrago-Casas, Juan Camilo; Chatzistergos, Theodosios; Chen, Ruizhu; Christensen-Dalsgaard, J; Donea, Alina; Fleck, Bernhard; Fournier, Damien; Garcia, R. A; Getling, Alexander V; Gizon, L; Gough, Douglas O; Hanasoge, S. M; Hanson, Chris S; Webber, Shea A. Hess; Hoeksema, J. Todd; Howe, Rachel; Jain, K; Kasapis, Spiridon; Kashyap, Samarth G; Kitiashvili, I. N; Komm, R; Korzennik, S. G; Krivova, Natalie A; Kuhn, Jeffrey R; Liang, Zhi-Chao; Lindsey, Charles; Mahajan, Sushant S; Mandal, K; Mani, Prasad; Oliveros, Juan Carlos Martinez; Mathur, S; Soares, M. Cristina Rabello; Rajaguru, S. P; Reiter, Johann; Rhodes Jr., Edward J; Rozelot, J. P; Scherrer, P. H; Solanki, S. K; Stefan, John T; Toomre, Juri; Tripathy, S. C; Upton, Lisa A; Zhao, Junwei

URI: http://hdl.handle.net/2248/8727

Date: 2025-05

Abstract:

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.