Kavli Affiliate: J. Todd Hoeksema
| First 5 Authors: Alexander Kosovichev, Sarbani Basu, Yuto Bekki, Juan Camilo Buitrago-Casas, Theodosios Chatzistergos
| Summary:
High-resolution helioseismology observations with the Helioseismic and
Magnetic Imager (HMI) onboard 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.
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