The SunPy project: Open source development and status of the version 1.0 core package

WT Barnes, MG Bobra, SD Christe, N Freij… - The Astrophysical …, 2020 - iopscience.iop.org
The goal of the SunPy project is to facilitate and promote the use and development of
community-led, free, and open source data analysis software for solar physics based on the …

Magnetic connectivity of the ecliptic plane within 0.5 au: potential field source surface modeling of the first Parker solar probe encounter

ST Badman, SD Bale, JCM Oliveros… - The Astrophysical …, 2020 - iopscience.iop.org
We compare magnetic field measurements taken by the FIELDS instrument on board Parker
Solar Probe (PSP) during its first solar encounter to predictions obtained by potential field …

On the formation of solar wind and switchbacks, and quiet sun heating

V Upendran, D Tripathi - The Astrophysical Journal, 2022 - iopscience.iop.org
The solar coronal heating in quiet Sun (QS) and coronal holes (CHs), including solar wind
formation, are intimately tied by magnetic field dynamics. Thus, a detailed comparative study …

Understanding heating in active region cores through machine learning. I. Numerical modeling and predicted observables

WT Barnes, SJ Bradshaw, NM Viall - The Astrophysical Journal, 2019 - iopscience.iop.org
To adequately constrain the frequency of energy deposition in active region cores in the
solar corona, systematic comparisons between detailed models and observational data are …

Understanding Heating in Active Region Cores through Machine Learning. II. Classifying Observations

WT Barnes, SJ Bradshaw, NM Viall - The Astrophysical Journal, 2021 - iopscience.iop.org
Constraining the frequency of energy deposition in magnetically closed active region cores
requires sophisticated hydrodynamic simulations of the coronal plasma and detailed forward …

Properties of the C ii 1334 Å line in coronal hole and quiet Sun as observed by IRIS

V Upendran, D Tripathi - The Astrophysical Journal, 2021 - iopscience.iop.org
Coronal holes (CHs) have subdued intensity and net blueshifts when compared to the quiet
Sun (QS) at coronal temperatures. At transition region temperatures, such differences are …

[HTML][HTML] Sunspot Rotation in High-and Low-Flaring Active Regions

R Grimes, B Pintér - Solar Physics, 2022 - Springer
Sunspot rotations are closely linked with flaring activity. They are thought to contribute to the
accumulation of helicity in magnetic flux tubes and to triggering magnetic reconnection in …

[PDF][PDF] Investigating the Solar Wind with Parker Solar Probe

R Laker, TS Horbury, JP Eastwood - 2019 - ronanlaker.com
Since the start of the space age, various spacecraft have supplied direct and remote
observations of the solar wind. This has proved critical to our understanding of its structure …