2 papers
astro-ph.SR2026
From simulations to observations of cool plasma: What we can learn from synthetic spectra
V. JerÄiÄ, T. A. Kucera, A. G. M. Pietrow +2
The paper generates synthetic Mg II h&k spectra from a non‑adiabatic 2.5D MHD simulation of coronal rain and compares them with IRIS observations to assess how well the model repro…
astro-ph.SR2025
Secondary small-scale dynamics of a Rayleigh-Taylor unstable solar prominence
Madhurjya Changmai, Jack M. Jenkins, Rony Keppens
Quiescent solar prominences show distinct small-scale dynamics in observations. Their internal density contrasts with the surrounding corona make them susceptible to Rayleigh-Taylo…