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

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; Jean Pierre Rozelot; Philip H. Scherrer; Sami K. Solanki; John T. Stefan; Juri Toomre; Sushanta C. Tripathy; Lisa A. Upton; Junwei Zhao

doi:10.1007/s11207-025-02480-6

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

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 JainSpiridon 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, Jean Pierre Rozelot, Philip H. Scherrer, Sami K. Solanki, John T. Stefan, Juri Toomre, Sushanta C. Tripathy, Lisa A. Upton, Junwei Zhao

Research output: Contribution to journal › Review article › peer-review

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.

Original language	English (US)
Article number	70
Journal	Solar Physics
Volume	300
Issue number	5
DOIs	https://doi.org/10.1007/s11207-025-02480-6
State	Published - May 2025

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Active regions
Flares
Helioseismology
Interior
Magnetic fields
Oscillations
Rotation
Sunspots
Turbulence
Velocity field

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Kosovichev, A. G., Basu, S., Bekki, Y., Buitrago-Casas, J. C., Chatzistergos, T., Chen, R., Christensen-Dalsgaard, J., Donea, A., Fleck, B., Fournier, D., García, R. A., Getling, A. V., Gizon, L., Gough, D. O., Hanasoge, S., Hanson, C. S., Hess Webber, S. A., Hoeksema, J. T., Howe, R., ... Zhao, J. (2025). Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager. Solar Physics, 300(5), Article 70. https://doi.org/10.1007/s11207-025-02480-6

@article{1abf6e73df324f9ab39dc1a5f8895018,

title = "Structure and Dynamics of the Sun{\textquoteright}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.",

keywords = "Active regions, Flares, Helioseismology, Interior, Magnetic fields, Oscillations, Rotation, Sunspots, Turbulence, Velocity field",

author = "Kosovichev, \{Alexander G.\} and Sarbani Basu and Yuto Bekki and Buitrago-Casas, \{Juan Camilo\} and Theodosios Chatzistergos and Ruizhu Chen and J{\o}rgen Christensen-Dalsgaard and Alina Donea and Bernhard Fleck and Damien Fournier and Garc{\'i}a, \{Rafael A.\} and Getling, \{Alexander V.\} and Laurent Gizon and Gough, \{Douglas O.\} and Shravan Hanasoge and Hanson, \{Chris S.\} and Hess Webber, \{Shea A.\} and Hoeksema, \{J. Todd\} and Rachel Howe and Kiran Jain and Spiridon Kasapis and Kashyap, \{Samarth G.\} and Kitiashvili, \{Irina N.\} and Rudolf Komm and Korzennik, \{Sylvain G.\} and Krivova, \{Natalie A.\} and Kuhn, \{Jeffrey R.\} and Liang, \{Zhi Chao\} and Charles Lindsey and Mahajan, \{Sushant S.\} and Krishnendu Mandal and Prasad Mani and Martinez Oliveros, \{Juan Carlos\} and Savita Mathur and Rabello Soares, \{M. Cristina\} and Rajaguru, \{S. Paul\} and Johann Reiter and Rhodes, \{Edward J.\} and Rozelot, \{Jean Pierre\} and Scherrer, \{Philip H.\} and Solanki, \{Sami K.\} and Stefan, \{John T.\} and Juri Toomre and Tripathy, \{Sushanta C.\} and Upton, \{Lisa A.\} and Junwei Zhao",

note = "Publisher Copyright: {\textcopyright} The Author(s) 2025.",

year = "2025",

month = may,

doi = "10.1007/s11207-025-02480-6",

language = "English (US)",

volume = "300",

journal = "Solar Physics",

issn = "0038-0938",

publisher = "Springer Netherlands",

number = "5",

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Kosovichev, AG, Basu, S, Bekki, Y, Buitrago-Casas, JC, Chatzistergos, T, Chen, R, Christensen-Dalsgaard, J, Donea, A, Fleck, B, Fournier, D, García, RA, Getling, AV, Gizon, L, Gough, DO, Hanasoge, S, Hanson, CS, Hess Webber, SA, Hoeksema, JT, Howe, R, Jain, K, Kasapis, S, Kashyap, SG, Kitiashvili, IN, Komm, R, Korzennik, SG, Krivova, NA, Kuhn, JR, Liang, ZC, Lindsey, C, Mahajan, SS, Mandal, K, Mani, P, Martinez Oliveros, JC, Mathur, S, Rabello Soares, MC, Rajaguru, SP, Reiter, J, Rhodes, EJ, Rozelot, JP, Scherrer, PH, Solanki, SK, Stefan, JT, Toomre, J, Tripathy, SC, Upton, LA & Zhao, J 2025, 'Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager', Solar Physics, vol. 300, no. 5, 70. https://doi.org/10.1007/s11207-025-02480-6

TY - JOUR

T1 - Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager

AU - Kosovichev, Alexander G.

AU - Basu, Sarbani

AU - Bekki, Yuto

AU - Buitrago-Casas, Juan Camilo

AU - Chatzistergos, Theodosios

AU - Chen, Ruizhu

AU - Christensen-Dalsgaard, Jørgen

AU - Donea, Alina

AU - Fleck, Bernhard

AU - Fournier, Damien

AU - García, Rafael A.

AU - Getling, Alexander V.

AU - Gizon, Laurent

AU - Gough, Douglas O.

AU - Hanasoge, Shravan

AU - Hanson, Chris S.

AU - Hess Webber, Shea A.

AU - Hoeksema, J. Todd

AU - Howe, Rachel

AU - Jain, Kiran

AU - Kasapis, Spiridon

AU - Kashyap, Samarth G.

AU - Kitiashvili, Irina N.

AU - Komm, Rudolf

AU - Korzennik, Sylvain G.

AU - Krivova, Natalie A.

AU - Kuhn, Jeffrey R.

AU - Liang, Zhi Chao

AU - Lindsey, Charles

AU - Mahajan, Sushant S.

AU - Mandal, Krishnendu

AU - Mani, Prasad

AU - Martinez Oliveros, Juan Carlos

AU - Mathur, Savita

AU - Rabello Soares, M. Cristina

AU - Rajaguru, S. Paul

AU - Reiter, Johann

AU - Rhodes, Edward J.

AU - Rozelot, Jean Pierre

AU - Scherrer, Philip H.

AU - Solanki, Sami K.

AU - Stefan, John T.

AU - Toomre, Juri

AU - Tripathy, Sushanta C.

AU - Upton, Lisa A.

AU - Zhao, Junwei

PY - 2025/5

Y1 - 2025/5

N2 - 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.

AB - 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.

KW - Active regions

KW - Flares

KW - Helioseismology

KW - Interior

KW - Magnetic fields

KW - Oscillations

KW - Rotation

KW - Sunspots

KW - Turbulence

KW - Velocity field

UR - http://www.scopus.com/inward/record.url?scp=105006424735&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=105006424735&partnerID=8YFLogxK

U2 - 10.1007/s11207-025-02480-6

DO - 10.1007/s11207-025-02480-6

M3 - Review article

AN - SCOPUS:105006424735

SN - 0038-0938

VL - 300

JO - Solar Physics

JF - Solar Physics

IS - 5

M1 - 70

ER -

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

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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