arXiv · 2503.07880
Structure and Dynamics of the Sun's Interior Revealed by Helioseismic and Magnetic Imager
Abstract
High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard 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.
Explore related subjects
Keep this discovery
Alexander Kosovichev, Sarbani Basu, Yuto Bekki, Juan Camilo Buitrago-Casas, Theodosios Chatzistergos, Ruizhu Chen, Joergen Christensen-Dalsgaard, Alina Donea, Bernhard Fleck, Damien Fournier, Rafael A. Garcia, Alexander Getling, Laurent Gizon, Douglas O. Gough, Shravan Hanasoge, Chris S. Hanson, Shea A. Hess Webber, J. Todd Hoeksema, Rachel Howe, Kiran Jain, Spiridon Kasapis, Samarth G. Kashyap, Irina Kitiashvili, Rudolf Komm, Sylvain Korzennik, Natalie A. Krivova, Jeff Kuhn, Zhi-Chao Liang, Charles Lindsey, Sushant S. Mahajan, Krishnendu Mandal, Prasad Mani, Juan Carlos Martinez Oliveros, Savita Mathur, M. Cristina Rabello Soares, S. Paul Rajaguru, Johann Reiter, Edward J. Rhodes, Jr., Jean-Pierre Rozelot, Philip H. Scherrer, Sami K. Solanki, John Stefan, Juri Toomre, Sushanta C. Tripathy, Lisa A. Upton, Junwei Zhao. 2025-03-10. Structure and Dynamics of the Sun's Interior Revealed by Helioseismic and Magnetic Imager. https://arxiv.org/abs/2503.07880
Cite the original work for its findings. Save a collection to share your selection of sources.