activity
20172026
most citedRecord-breaking coronal magnetic field in solar active region 12673

47 citations · 145 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Determination of the Height-Temperature Profile Above a Solar Active Region from Multi-Frequency Radio Observations

T. I. Kaltman, A. G. Stupishin, G. A. Makoev

An iterative method is presented for reconstructing the height-temperature profile of the solar atmosphere above a sunspot using multi-frequency spectro-polarimetric microwave obse…

astro-ph.SR2023★ 28 cited

Data-Constrained Solar Modeling with GX Simulator

Gelu M. Nita, Gregory D. Fleishman, Alexey A. Kuznetsov +6

To facilitate the study of solar active regions and flaring loops, we have created a modeling framework, the freely distributed GX Simulator IDL package, that combines 3D magnetic…

astro-ph.SR2021★ 12 cited

Coronal Heating Law Constrained by Microwave Gyroresonant Emission

Gregory D. Fleishman, Sergey A. Anfinogentov, Alexey G. Stupishin +2

The question why the solar corona is much hotter than the visible solar surface still puzzles solar researchers. Most theories of the coronal heating involve a tight coupling betwe…

astro-ph.SR2019★ 47 cited

Record-breaking coronal magnetic field in solar active region 12673

Sergey A. Anfinogentov, Alexey G. Stupishin, Ivan I. Mysh'yakov +1

At the Sun, the strongest magnetic fields are routinely detected at dark sunspots. The magnitude of the field is typically about 3000 G, with only a few exceptions that reported th…

astro-ph.SR2018★ 22 cited

Force-Free Field Reconstructions Enhanced by Chromospheric Magnetic Field Data

Gregory Fleishman, Ivan Mysh'yakov, Alexey Stupishin +2

3D picture of the coronal magnetic field remains an outstanding problem in solar physics, particularly, in active regions. Nonlinear force-free field reconstructions that employ ro…

astro-ph.SR2017★ 36 cited

Casting the Coronal Magnetic Field Reconstruction Tools in 3D Using MHD Bifrost Model

Gregory D. Fleishman, Sergey Anfinogentov, Maria Loukitcheva +2

Quantifying coronal magnetic field remains a central problem in solar physics. Nowadays the coronal magnetic field is often modelled using nonlinear force-free field (NLFFF) recons…