activity
20172026
most citedMapping the Sun's coronal magnetic field using the Zeeman effect

33 citations · 94 across the 12 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2026

Inferring 3D Coronal Magnetic Fields through Seismology-assisted Inversions of -only Spectropolarimetric Observations

Alin Razvan Paraschiv

The routine measurement of the Stokes signals of emission lines in the solar corona is still a challenging endeavor, particularly for observations using small-aperture instr…

astro-ph.SR2025

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…

astro-ph.SR2024★ 33 cited

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…

astro-ph.SR2024

Coronagraphic observations of Si X 1430 nm acquired by DKIST/Cryo-NIRSP with methods for telluric absorption correction

T. A. Schad, A. Fehlmann, G. I. Dima +6

We report commissioning observations of the Si X 1430 nm solar coronal line observed coronagraphically with the Cryogenic Near-Infrared Spectropolarimeter (Cryo-NIRSP) at the Natio…

astro-ph.SR2022★ 4 cited

A Machine Learning Enhanced Approach for Automated Sunquake Detection in Acoustic Emission Maps

Vanessa Mercea, Alin Razvan Paraschiv, Daniela Adriana Lacatus +2

Sunquakes are seismic emissions visible on the solar surface, associated with some solar flares. Although discovered in 1998, they have only recently become a more commonly detecte…

astro-ph.SR2022★ 9 cited

Optimal spectral lines for measuring chromospheric magnetic fields

P. Judge, P. Bryans, R. Casini +4

This paper identifies spectral lines from X-ray to infrared wavelengths which are optimally suited to measuring vector magnetic fields as high as possible in the solar atmosphere.…