activity
20242026
collaborators

5 papers

astro-ph.SR2026

Diversity of morphology of type II spicules in MURaM-ChE simulations

Sanghita Chandra, Robert Cameron, Damien Przybylski +1

Spicules are ubiquitous, small-scale features in the solar atmosphere, exhibiting a jet-like appearance most clearly identified by their apparent motion in off-limb observations. W…

astro-ph.SR2026

A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy

Valeriy Vasilyev, Alexander I. Shapiro, Nadiia Kostogryz +10

TRAPPIST-1 is an ultra-cool dwarf that flares frequently. These flares shape the surrounding planets' high-energy irradiation environments, with consequences for atmospheric chemis…

astro-ph.SR2025

Statistical properties of spicules in MURaM-ChE

Sanghita Chandra, Robert Cameron, Damien Przybylski +1

Numerical simulations of the solar chromosphere have progressed towards reproducing spicules, which are transient features observed at the solar limb using spectral lines such as H…

astro-ph.SR2025

Probing chromospheric fine structures with a Hα proxy using MURaM-ChE

Sanghita Chandra, Robert Cameron, Damien Przybylski +3

H observations of the solar chromosphere reveal dynamic small-scale structures known as spicules at the limb and rapid blue and red shifted excursions (RBEs/RREs) on-disk. We w…

astro-ph.SR2024

3D Radiative MHD Simulations of Starspots II: Large-scale Structure

Tanayveer Singh Bhatia, Mayukh Panja, Robert Cameron +1

We compute realistic 3D radiative MHD near-surface models of starspots with substantial penumbrae on cool main-sequence stars using the MURaM simulation code. This work is an impro…