From the 1 of 3 linked papers with an AI index.
3 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…
astro-ph.SR2024
Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths
A. G. M. Pietrow, V. Liakh, C. M. J. Osborne +2
We present synthetic spectra corresponding to a 2.5D magnetohydrodynamical simulation of a rotating prominence in the Ca II 8542 Ã , H, Ca II K, Mg II k, Ly , and Ly l…