AWSoM Magnetohydrodynamic Simulation of a Solar Active Region. II. Statistical Analysis of Alfvén Wave Dissipation and Reflection, Scaling Laws, and Energy …
T Shi, W Manchester, E Landi… - The Astrophysical …, 2024 - iopscience.iop.org
The coronal heating problem has been a major challenge in solar physics, and a
tremendous amount of effort has been made over the past several decades to solve it. In this …
tremendous amount of effort has been made over the past several decades to solve it. In this …
Nonequilibrium Ionization Effects on Synthetic Spectra in the AWSoM Solar Corona
J Szente, E Landi, B van der Holst - The Astrophysical Journal …, 2023 - iopscience.iop.org
In this work, we combined AWSoM's nonequilibrium ionization (NEI) calculations from
Szente et al. with the synthetic spectral computations of SPECTRUM to predict …
Szente et al. with the synthetic spectral computations of SPECTRUM to predict …
Solar wind modeling with the Alfvén Wave Solar atmosphere Model driven by HMI-based Near-Real-Time maps by the National Solar Observatory
We explore the performance of the Alfvén Wave Solar atmosphere Model with near-real-time
(NRT) synoptic maps of the photospheric vector magnetic field. These maps, produced by …
(NRT) synoptic maps of the photospheric vector magnetic field. These maps, produced by …
3D Nonequilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. I. Comparison with Hinode/EIS Observations
EM Wraback, E Landi, WB Manchester… - The Astrophysical …, 2025 - iopscience.iop.org
High-resolution EUV spectroscopy provides an informative diagnostic tool for the early
evolution of coronal mass ejections (CMEs) since it can directly measure many physical …
evolution of coronal mass ejections (CMEs) since it can directly measure many physical …
Spectroscopic Observations of the Solar Corona during the 2017 August 21 Total Solar Eclipse: Comparison of Spectral Line Widths and Doppler Shifts between …
Y Zhu, SR Habbal, A Ding, B Yamashiro… - The Astrophysical …, 2024 - iopscience.iop.org
The spectroscopic observations presented here were acquired during the 2017 August 21
total solar eclipse (TSE) with a three-channel partially multiplexed imaging spectrometer …
total solar eclipse (TSE) with a three-channel partially multiplexed imaging spectrometer …
Three‐dimensional structure of the corona during WHPI campaign rotations CR‐2219 and CR‐2223
DG Lloveras, AM Vasquez, FA Nuevo… - Journal of …, 2022 - Wiley Online Library
Differential emission measure tomography (DEMT) and white light (WL) tomography were
applied to study the three‐dimensional (3D) structure of the global solar corona for two …
applied to study the three‐dimensional (3D) structure of the global solar corona for two …
Constraining the inner boundaries of COCONUT through plasma β and Alfvén speed
Context. Space weather modelling has been gaining importance due to our increasing
dependency on technology sensitive to space weather effects, such as satellite services, air …
dependency on technology sensitive to space weather effects, such as satellite services, air …
Simulating Compressive Stream Interaction Regions during Parker Solar Probe's First Perihelion Using Stream-aligned Magnetohydrodynamics
EM Wraback, AP Hoffmann… - The Astrophysical …, 2024 - iopscience.iop.org
We used the stream-aligned magnetohydrodynamics (SA-MHD) model to simulate
Carrington rotation 2210, which contains Parker Solar Probe's (PSP) first perihelion at 36.5 …
Carrington rotation 2210, which contains Parker Solar Probe's (PSP) first perihelion at 36.5 …
Physics-Based Simulation of the 2013 April 11 SEP Event
Solar energetic particles (SEPs) can pose hazardous radiation risks to both humans in
space and spacecraft electronics. Numerical modeling based on first principles offers …
space and spacecraft electronics. Numerical modeling based on first principles offers …