collaborators

6 papers

physics.space-ph2025

NASA/NOAA MOU Annex Final Report: Evaluating Model Advancements for Predicting CME Arrival Time

M. L. Mays, P. J. MacNeice, A. Taktakishvili +11

The purpose of this project was to assess improvements in CME arrival time forecasts at Earth using the Air Force Data Assimilative Photospheric Flux Transport (ADAPT) model driven…

astro-ph.SR2025

Why do solar wind models get it wrong: understanding the capabilities of time-dependent solar wind simulations

Evangelia Samara, Elena Provornikova, C. Nick Arge +2

We explore the capabilities of time-dependent (TD) magnetohydrodynamics (MHD) solar wind simulations with the coupled WSA model of the solar corona and GAMERA model of the inner he…

astro-ph.SR2025

Incorporating Magnetic Field Characteristics into EUV-Based Automated Segmentation of Coronal Holes

Jeremy A. Grajeda, Laura E. Boucheron, Michael S. Kirk +3

Coronal holes (CHs) are magnetically open regions that allow hot coronal plasma to escape from the Sun and form the high-speed solar wind. This wind can interact with Earth's magne…

astro-ph.SR2025

Improved Tomographic Reconstruction of 3D Global Coronal Density from STEREO/COR1 Observations

Tongjiang Wang, C. Nick Arge, Shaela I. Jones

Tomography is a powerful technique for recovering the three-dimensional (3D) density structure of the global solar corona. In this work, we present an improved tomography method by…

astro-ph.SR2025

Magnetic Field-Constrained Ensemble Image Segmentation of Coronal Holes in Chromospheric Observations

Jaime A. Landeros, Michael S. Kirk, C. Nick Arge +5

Coronal Holes (CHs) are large-scale, low-density regions in the solar atmosphere which may expel high-speed solar wind streams that incite hazardous, geomagnetic storms. Coronal an…

astro-ph.SR2024

Quantifying the Consistency and Characterizing the Confidence of Coronal Holes Detected by Active Contours without Edges (ACWE)

Jeremy A. Grajeda, Laura E. Boucheron, Michael S. Kirk +2

Coronal Holes (CHs) are regions of open magnetic field lines, resulting in high speed solar wind. Accurate detection of CHs is vital for space weather prediction. This paper presen…