activity
20102026
most citedMapping the Sun's coronal magnetic field using the Zeeman effect

33 citations · 47 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2026

Spectroscopic analysis and RHD modeling of the first Ca II H and H-epsilon flare spectra from DKIST/ViSP

Cole Tamburri, Adam Kowalski, Gianna Cauzzi +7

We analyze decay phase observations of the GOES class C6.7 flare SOL2022-08-19T20:31 by the Visible Spectropolarimeter (ViSP) on the National Science Foundation's Daniel K. Inouye…

astro-ph.SR2025

Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST

Cole A. Tamburri, Maria D. Kazachenko, Gianna Cauzzi +8

We present the highest-resolution H observations of a solar flare to date, collected during the decay phase of an X1.3-class flare on 8 August 2024 at 20:12 UT. Observations wit…

astro-ph.SR2025

First coordinated observations between Solar Orbiter and the Daniel K. Inouye Solar Telescope

Krzysztof Barczynski, Miho Janvier, Chris J. Nelson +8

Solar Orbiter and the Daniel K. Inouye Solar Telescope (DKIST) are two of the newest facilities available to the solar physics community. The first coordinated observations of the…

astro-ph.SR2025

Intersecting frontiers for ground and space-based solar missions: symbiotic coordination between DKIST, PSP, and Solar Orbiter

Thomas A. Schad, Alexandra Tritschler, Gianna Cauzzi

Three uniquely powerful solar and heliospheric facilities are now operational at the same time. The US National Science Foundation's Daniel K Inouye Solar Telescope, NASA's Parker…

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★ 5 cited

Magnetic diffusion in Solar atmosphere produces measurable electric fields

Tetsu Anan, Roberto Casini, Han Uitenbroek +13

The efficient release of magnetic energy in astrophysical plasmas, such as during solar flares, can in principle be achieved through magnetic diffusion, at a rate determined by the…

astro-ph.SR2010★ 9 cited

Line shape effects on intensity measurements of solar features: Brightness correction to SoHO MDI continuum images

S. Criscuoli, I. Ermolli, D. Del Moro +4

Continuum intensity observations obtained with the Michelson Doppler Imager (MDI) on-board the SoHO mission provide long time series of filtergrams that are ideal for studying the…