Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager
А. Г. Косовичев, Sarbani Basu, Yuto Bekki, Juan Camilo Buitrago‐Casas, Theodosios Chatzistergos, Ruizhu Chen, J. Christensen‐Dalsgaard, Alina Donea, B. Fleck, D. Fournier, R. A. García, А. В. Гетлинг, L. Gizon, D. O. Gough, Shravan Hanasoge, Chris S. Hanson, Shea A. Hess Webber, J. T. Hoeksema, R. Howe, Kiran Jain, Spiridon Kasapis, Samarth G. Kashyap, Irina Kitiashvili, Rudolf Komm, S. G. Korzennik, N. A. Krivova, J. R. Kuhn, Zhi–Chao Liang, C. Lindsey, Sushant S. Mahajan, Krishnendu Mandal, Prasad Mani, Juan Carlos Martínez Oliveros, S. Mathur, M. C. Rabello‐Soares, S. P. Rajaguru, Johann Reiter, E. J. Rhodes, J. P. Rozelot, P. H. Scherrer, S. K. Solanki, John T. Stefan, Juri Toomre, S. C. Tripathy, Lisa Upton, Junwei Zhao
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.