The SunPy project: Open source development and status of the version 1.0 core package
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 …
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
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 …
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 …
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 …
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 …
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 …
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 …
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 …
observations of the solar wind. This has proved critical to our understanding of its structure …