activity
20032026
most citedA Comparison of Flare Forecasting Methods, I: Results from the "All-Clear" Workshop

228 citations · 1.1k across the 29 of their papers we have counts for

collaborators

30 papers

astro-ph.SR2026

Unipolarity of the solar magnetic field in equatorial coronal holes

Khagendra Katuwal, R. T. James McAteer

A study of the unbalanced magnetic polarity distribution of 70 coronal holes was performed. Data from the Helioseismic and Magnetic Imager (HMI) were used to examine the photospher…

astro-ph.IM2023★ 1 cited

The case for studying other planetary magnetospheres and atmospheres in Heliophysics

Ian J. Cohen, Chris Arridge, Abigail Azari +37

Heliophysics is the field that "studies the nature of the Sun, and how it influences the very nature of space - and, in turn, the atmospheres of planetary bodies and the technology…

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…

astro-ph.IM2023★ 1 cited

Improving Multi-Dimensional Data Formats, Access, and Assimilation Tools for the Twenty-First Century

Daniel B. Seaton, Amir Caspi, Roberto Casini +12

Heliophysics image data largely relies on a forty-year-old ecosystem built on the venerable Flexible Image Transport System (FITS) data standard. While many in situ measurements us…

astro-ph.IM2023★ 5 cited

COMPLETE: A flagship mission for complete understanding of 3D coronal magnetic energy release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

COMPLETE is a flagship mission concept combining broadband spectroscopic imaging and comprehensive magnetography from multiple viewpoints around the Sun to enable tomographic recon…

astro-ph.SR2020★ 3 cited

Spatial and temporal analysis of 3-minute oscillations in the chromosphere associated with the X2.2 Solar Flare on 2011 February 15

Laurel Farris, R. T. James McAteer

3-minute oscillations in the chromosphere are attributed to both slow magnetoacoustic waves propagating from the photosphere, and to oscillations generated within the chromosphere…