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astro-ph.SR2024
Spectroscopic Observations of the Solar Corona during the 2017 August 21 Total Solar Eclipse: Comparison of Spectral Line Widths and Doppler Shifts Between Open and Closed Magnetic Structures
Yingjie Zhu, Shadia R. Habbal, Adalbert Ding +5
The spectroscopic observations presented here were acquired during the 2017 August 21 total solar eclipse with a three-channel partially multiplexed imaging spectrometer (3PAMIS) o…
astro-ph.SR2023
Non-equilibrium Ionization Effects on Synthetic Spectra in the AWSoM Solar Corona
Judit Szente, Enrico Landi, Bart van der Holst
In this work we combined AWSoM's non-equilibrium ionization [NEI] calculations from (Szente:2022) with the synthetic spectral computations of SPECTRUM (Szente:2019), to predict non…
astro-ph.SR2012★ 27 cited
The role of radiative losses in the late evolution of pulse-heated coronal loops/strands
F. Reale, E. Landi
Radiative losses from optically thin plasma are an important ingredient for modeling plasma confined in the solar corona. Spectral models are continuously updated to include the em…