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

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.

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Publication Details

Journal
Solar Physics
Published
2025-05-01
DOI
https://doi.org/10.1007/s11207-025-02480-6
Citations
7
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
8.08
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Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager

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article

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

Junwei Zhao, Spiridon Kasapis, Irina Kitiashvili, J. T. Hoeksema, R. Howe, J. R. Kuhn, J. Christensen‐Dalsgaard, S. Mathur, C. Lindsey, Lisa Upton, Kiran Jain, B. Fleck, Shravan Hanasoge, Zhi–Chao Liang, Yuto Bekki, Prasad Mani, Juri Toomre, John T. Stefan, S. K. Solanki, Theodosios Chatzistergos, Sushant S. Mahajan, А. Г. Косовичев, Samarth G. Kashyap, Alina Donea, M. C. Rabello‐Soares, Chris S. Hanson, S. P. Rajaguru, Krishnendu Mandal, Ruizhu Chen, Juan Carlos Martínez Oliveros, А. В. Гетлинг, S. C. Tripathy, J. P. Rozelot, D. O. Gough, L. Gizon, S. G. Korzennik, Juan Camilo Buitrago‐Casas, N. A. Krivova, Sarbani Basu, E. J. Rhodes, Shea A. Hess Webber, P. H. Scherrer, R. A. García, D. Fournier, Rudolf Komm, Johann Reiter
article en
7 citations

Abstract

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.

Solar PhysicsVol. 300(5)
University of Southern California (US), New Jersey Institute of Technology (US), Tata Institute of Fundamental Research (IN), New York University Abu Dhabi (AE), Ames Research Center (US), Southwest Research Institute (US), Centre National de la Recherche Scientifique (FR), The University of Sydney (AU), University of Hawaii System (US), Joint Institute for Laboratory Astrophysics (US), Indian Institute of Astrophysics (IN), Universidad de La Laguna (ES), Lomonosov Moscow State University (RU), Aarhus University (DK), Université Paris Cité (FR), University of Cambridge (GB), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Yale University (US), Astrophysique, Instrumentation et Modélisation (FR), National Solar Observatory (US), Max Planck Institute for Solar System Research (DE), Center for Astrophysics Harvard & Smithsonian (US), Observatoire de la Côte d’Azur (FR), CEA Paris-Saclay (FR), Instituto de Astrofísica de Canarias (ES), Astrophysics Science Division (US), Northwest Research Associates (US), Monash University (AU), Technical University of Munich (DE), University of Birmingham (GB), University of California, Berkeley (US), Stanford University (US)
Openalex Percentile: Top 3%
Solar and Space Plasma Dynamics
8.08
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