Inversion techniques of the radiative transfer equation for polarized light are presented as one of the best current procedures to infer the vector magnetic...
Structure and Dynamics of the Sun's Interior Revealed by the Helioseismic and Magnetic Imager
High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) provide a unique three...
SUNRISE III: Overview of Observatory and Instruments
In July 2024, SUNRISE completed its third successful science flight. The SUNRISE III observatory had been upgraded significantly after the two previous...
The Taiwan Oscillation Network (TON) is a ground-based network to measure solar intensity oscillations to study the internal structure of the Sun. K-line full...
The density matrix approach to polarized radiative transfer
The density matrix approach to polarized radiative transfer is reviewed, with particular emphasis on the physical assumptions that are at the basis of the...
The dynamics of the solar radiative interior are still poorly constrained by comparison to the convective zone. This disparity is even more marked when we...