output
20082025
most citedNew Insights into White-Light Flare Emission from Radiative-Hydrodynamic Modeling of a Chromospheric Condensation

96 citations

21 papers

physics.space-ph2025

Magnitude of Short-Wavelength Electric Field Fluctuations in Simulations of Collisionless Plasma Shocks

Vadim Roytershteyn, Lynn B. Wilson, Li-Jen Chen +2

Large-amplitude electrostatic fluctuations are routinely observed by spacecraft upon traversal of collisionless shocks in the heliosphere. Kinetic simulations of shocks have strugg…

astro-ph.SR2023★ 4 cited

Trajectories of Coronal Mass Ejection from Solar-type Stars

Fabian Menezes, Adriana Valio, Yuri Netto +3

The Sun and other solar-type stars have magnetic fields that permeate their interior and surface, extends through the interplanetary medium, and is the main driver of stellar activ…

physics.space-ph2023★ 25 cited

On the seed population of solar energetic particles in the inner heliosphere

Nicolas Wijsen, Gang Li, Zheyi Ding +5

Particles measured in large gradual solar energetic particle (SEP) events are believed to be predominantly accelerated at shocks driven by coronal mass ejections (CMEs). Ion charge…

astro-ph.EP2023★ 13 cited

Absence of extended atmospheres in low-mass star radius-gap planets GJ 9827 b, GJ 9827 d and TOI-1235 b

Vigneshwaran Krishnamurthy, Teruyuki Hirano, Eric Gaidos +20

\textit{Kepler} showed a paucity of planets with radii of 1.5 - 2 around solar mass stars but this radius-gap has not been well studied for low-mass star plane…

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★ 4 cited

The Transition Region of Solar Flare Loops

C. Gontikakis, S. K. Antiochos, P. R. Young

The transition region between the Sun's corona and chromosphere is important to the mass and energy transfer from the lower atmosphere to the corona; consequently, this region has…