collaborators

6 papers

physics.space-ph2026

Advancing Heliophysics and Space Weather Modeling through Open Science

C. Corti, M. M. Kuznetsova, M. A. Reiss +85

We present a community-wide effort to develop a strategy and action plan to advance heliophysics and space weather modeling through open science. While open science has the potenti…

astro-ph.SR2026

Reevaluating thermal instability in a uniform plasma: an extended analysis of instability domains

Varsha Felsy, Ramon Oliver, Jaume Terradas +3

Thermal instability plays a crucial role in the dynamics of astrophysical plasmas. Building upon the foundational work of G. B. Field (1965) and the subsequent analysis by T. Water…

physics.space-ph2025

, outer boundary, and Biot-Savart in magnetosphere MHD simulations

Dean Thomas, Robert S. Weigel, Gary Quaresima +2

We examine the size of and outer surface boundary integrals in estimating the surface magnetic field from magnetohydrodynamic (M…

astro-ph.SR2025

Time evolution of white-light flare accompanied by probable postflare loops on M-type dwarf EV Lacertae

Shinnosuke Ichihara, Daisaku Nogami, Kosuke Namekata +6

White-light flares are explosive phenomena accompanied by brightening of continuum from near-ultraviolet to optical, which occur on the Sun and stars. In order to investigate the m…

astro-ph.SR2025

Prominence material observed by SoloHI beyond 0.5au

C. Mac Cormack, S. B. Shaik, P. Hess +2

With the combination of observations from in-situ and high-resolution remote sensing instruments, the Solar Orbiter (SolO) mission has become a particularly valuable mission for st…

astro-ph.SR2025

Understanding the complex morphology of a CME: multi-view analysis and numerical modeling

Cecilia Mac Cormack, Abril Sahade, Angelos Vourlidas +3

Although all coronal mass ejections (CMEs) that propagate into the heliosphere should contain a magnetic flux rope (MFR) component, the majority do not exhibit the expected white-l…