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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8727
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dc.contributor.authorKosovichev, A. G-
dc.contributor.authorBasu, S-
dc.contributor.authorBekki, Y-
dc.contributor.authorBuitrago-Casas, Juan Camilo-
dc.contributor.authorChatzistergos, Theodosios-
dc.contributor.authorChen, Ruizhu-
dc.contributor.authorChristensen-Dalsgaard, J-
dc.contributor.authorDonea, Alina-
dc.contributor.authorFleck, Bernhard-
dc.contributor.authorFournier, Damien-
dc.contributor.authorGarcia, R. A-
dc.contributor.authorGetling, Alexander V-
dc.contributor.authorGizon, L-
dc.contributor.authorGough, Douglas O-
dc.contributor.authorHanasoge, S. M-
dc.contributor.authorHanson, Chris S-
dc.contributor.authorWebber, Shea A. Hess-
dc.contributor.authorHoeksema, J. Todd-
dc.contributor.authorHowe, Rachel-
dc.contributor.authorJain, K-
dc.contributor.authorKasapis, Spiridon-
dc.contributor.authorKashyap, Samarth G-
dc.contributor.authorKitiashvili, I. N-
dc.contributor.authorKomm, R-
dc.contributor.authorKorzennik, S. G-
dc.contributor.authorKrivova, Natalie A-
dc.contributor.authorKuhn, Jeffrey R-
dc.contributor.authorLiang, Zhi-Chao-
dc.contributor.authorLindsey, Charles-
dc.contributor.authorMahajan, Sushant S-
dc.contributor.authorMandal, K-
dc.contributor.authorMani, Prasad-
dc.contributor.authorOliveros, Juan Carlos Martinez-
dc.contributor.authorMathur, S-
dc.contributor.authorSoares, M. Cristina Rabello-
dc.contributor.authorRajaguru, S. P-
dc.contributor.authorReiter, Johann-
dc.contributor.authorRhodes Jr., Edward J-
dc.contributor.authorRozelot, J. P-
dc.contributor.authorScherrer, P. H-
dc.contributor.authorSolanki, S. K-
dc.contributor.authorStefan, John T-
dc.contributor.authorToomre, Juri-
dc.contributor.authorTripathy, S. C-
dc.contributor.authorUpton, Lisa A-
dc.contributor.authorZhao, Junwei-
dc.date.accessioned2025-06-19T05:37:11Z-
dc.date.available2025-06-19T05:37:11Z-
dc.date.issued2025-05-
dc.identifier.citationSolar Physics, Vol. 300, No. 5, 70en_US
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/8727-
dc.descriptionRestricted Accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractHigh-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.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.relation.urihttps://doi.org/10.1007/s11207-025-02480-6-
dc.rights© The Author(s), under exclusive licence to Springer Nature B.V. 2025-
dc.subjectActive regionsen_US
dc.subjectFlaresen_US
dc.subjectHelioseismologyen_US
dc.subjectInterioren_US
dc.subjectMagnetic fieldsen_US
dc.subjectOscillationsen_US
dc.subjectRotationen_US
dc.subjectSunspotsen_US
dc.subjectTurbulenceen_US
dc.subjectVelocity fielden_US
dc.titleStructure and dynamics of the sun’s interior revealed by the helioseismic and magnetic Imageren_US
dc.typeArticleen_US
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