Simulation data from "Mass Flows in Expanding Coronal Loops"
<p>24 HYDRAD hydrodynamic simulations from the paper "Mass Flows in Expanding Coronal Loops" by Reep, Scott, Chhabra, Unverferth & Knizhnik, accepted for publication in the Astrophysical Journal, 2024 (https://arxiv.org/abs/2403.12358). Each of Figures 1, 2, 3, and 9 have six simulations with varying cross-sectional area expansion factors. These simulations were used to generate the plots in the paper.</p> <p>The output of the simulation data can be found in the ./Results/ folder of each simulation's directory. The source code was modified to hard code the expansion factors in ./HYDRAD/source/eqns.cpp, under the functions double CEquations::CalculateMagneticField and double CEquations::CalculateCrossSection, rather than using polynomial fits as is standard in HYDRAD. </p> <p> </p>
ShareScore
32/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 4
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 8
- Engagement
- 0