activity
20082023
most citedGONG Catalog of Solar Filament Oscillations Near Solar Maximum

59 citations · 218 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2023★ 10 cited

SPICE Connection Mosaics to link the Sun's surface and the heliosphere

T. Varesano, D. M. Hassler, N. Zambrana Prado +28

We present an analysis of the first connection mosaic made by the SPICE instrument on board of the ESA / NASA Solar Orbiter mission on March 2nd, 2022. The data will be used to map…

astro-ph.SR2023★ 4 cited

The Multiview Observatory for Solar Terrestrial Science (MOST)

N. Gopalswamy, S. Christe, S. F. Fung +54

We report on a study of the Multiview Observatory for Solar Terrestrial Science (MOST) mission that will provide comprehensive imagery and time series data needed to understand the…

astro-ph.SR2023★ 19 cited

Prospects of Detecting Non-thermal Protons in Solar Flares via Lyman Line Spectroscopy: Revisiting the Orrall-Zirker Effect

Graham S. Kerr, Joel C. Allred, Adam F. Kowalski +5

Solar flares are efficient particle accelerators, with a substantial fraction of the energy released manifesting as non-thermal particles. While the role that non-thermal electrons…

astro-ph.SR2023★ 5 cited

Nonlinear Fast Magnetosonic Waves in Solar Prominence Pillars

Leon Ofman, Therese A. Kucera, C. Richard DeVore

We investigate the properties of nonlinear fast magnetosonic (NFM) waves in a solar prominence, motivated by recent high-resolution and high-cadence Hinode/SOT observations of smal…

astro-ph.SR2021★ 30 cited

First observations from the SPICE EUV spectrometer on Solar Orbiter

A. Fludra, M. Caldwell, A. Giunta +28

We present first science observations taken during the commissioning activities of the Spectral Imaging of the Coronal Environment (SPICE) instrument on the ESA/NASA Solar Orbiter…

astro-ph.SR2020★ 2 cited

Untangling the global coronal magnetic field with multiwavelength observations

S. E. Gibson, A. Malanushenko, G. de Toma +16

Magnetism defines the complex and dynamic solar corona. Coronal mass ejections (CMEs) are thought to be caused by stresses, twists, and tangles in coronal magnetic fields that buil…