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

IF 2.7 3区物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS

Solar Physics Pub Date : 2025-05-26 DOI:10.1007/s11207-025-02480-6

Alexander G. Kosovichev, Sarbani Basu, Yuto Bekki, Juan Camilo Buitrago-Casas, Theodosios Chatzistergos, Ruizhu Chen, Jørgen Christensen-Dalsgaard, Alina Donea, Bernhard Fleck, Damien Fournier, Rafael A. García, Alexander V. 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 N. Kitiashvili, Rudolf Komm, Sylvain G. Korzennik, Natalie A. Krivova, Jeffrey R. 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 T. Stefan, Juri Toomre, Sushanta C. Tripathy, Lisa A. Upton, Junwei Zhao

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引用次数: 0

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.

查看原文本刊更多论文

日震和磁成像仪揭示的太阳内部结构和动力学

太阳动力学观测站（SDO）搭载的日震和磁成像仪（HMI）提供了太阳内部结构和动力学的独特三维视图，揭示了太阳内部物理过程的巨大复杂性。我们概述了HMI日震学计划的结果，并讨论了它们对现代理论模型和太阳内部模拟的影响。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

Solar Physics 地学天文-天文与天体物理

CiteScore

5.10

自引率

17.90%

发文量

146

审稿时长

1 months

期刊介绍： Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.