activity
20142024
most citedMulti-Passband Observations of A Solar Flare over the He I 10830 Å line

9 citations · 9 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2024

Forecasting SEP Events During Solar Cycles 23 and 24 Using Interpretable Machine Learning

Spiridon Kasapis, Irina N. Kitiashvili, Paul Kosovich +4

Prediction of the Solar Energetic Particle (SEP) events garner increasing interest as space missions extend beyond Earth's protective magnetosphere. These events, which are, in mos…

astro-ph.SR2024

Investigating Performance Trends of Simulated Real-time Solar Flare Predictions: The Impacts of Training Windows, Data Volumes, and the Solar Cycle

Griffin T. Goodwin, Viacheslav M. Sadykov, Petrus C. Martens

This study explores the behavior of machine learning-based flare forecasting models deployed in a simulated operational environment. Using Georgia State University's Space Weather…

astro-ph.SR2023

Spectro-Polarimetric Properties of Sunquake Sources in X1.5 Flare and Evidence for Electron and Proton Beam Impacts

Alexander G. Kosovichev, Viacheslav M. Sadykov, John T. Stefan

The first significant sunquake event of Solar Cycle 25 was observed during the X1.5 flare of May 10, 2022, by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics…

astro-ph.SR20219 cited

Multi-Passband Observations of A Solar Flare over the He I 10830 Å line

Yan Xu, Xu Yang, Graham S. Kerr +5

This study presents a C3.0 flare observed by the BBSO/GST and IRIS, on 2018-May-28 around 17:10 UT. The Near Infrared Imaging Spectropolarimeter (NIRIS) of GST was set to spectral…

astro-ph.SR2014

Using MHD simulations to model H-alpha and UV spectral lines for interpretation of IRIS and NST data

Viacheslav M. Sadykov, Alexander G. Kosovichev

We present results of non-LTE modeling of H-alpha 6563 A and Mg II k&h 2796 A and 2803 A lines. This modeling is important for interpretation of coordinated observations from the r…