Scholarlink

<p>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.</p>

错误：搜索内容不能为空，请输入英文关键词
错误：关键词超出字数限制，请精简
高级检索

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

  • 期刊论文

  • 出版模式：

    开放获取

  • 发表日期：

    2025年5月26日

查看全文
  • 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

摘要

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.