From the 1 of 3 linked papers with an AI index.
3 papers
Inferring 3D Coronal Magnetic Fields through Seismology-assisted Inversions of -only Spectropolarimetric Observations
Alin Razvan Paraschiv, Alin RÄzvan Paraschiv
The paper presents a new inversion method that combines Stokes IQU spectropolarimetric data of coronal emission lines with coronal‑seismology derived plane‑of‑sky magnetic‑field es…
Ubiquitous high-frequency waves and disturbances in the active region corona observed with DKIST/Cryo-NIRSP
Momchil E. Molnar, Richard Morton, Alin Paraschiv +4
The plasma of the solar corona harbors a multitude of coronal wave modes, some of which could be dissipated to provide the required energy and momentum to heat the corona and accel…
Mapping the Sun's coronal magnetic field using the Zeeman effect
Thomas A. Schad, Gordon J. D. Petrie, Jeffrey R. Kuhn +9
Regular remote sensing of the magnetic field embedded within the million-degree solar corona is severely lacking. This reality impedes fundamental investigations of the nature of c…