This readme was generated on 2025-11-4 by djcalve2

# GENERAL INFORMATION

Title: Turbulence in Core-Collapse Supernovae

This data set accompanies the following publication:
https://doi.org/10.3847/1538-4357/ae1475
in The Astrophysical Journal


## Contact Information
Name: Carla Frohlich
ORCID: 0000-0003-0191-2477
Institution: North Carolina State University, Raleigh, NC, USA
Email: cfrohli@ncsu.edu



# SHARING/ACCESS INFORMATION

License: Creative Commons Attribution No Derivatives 4.0 International
DOI (data): 10.5281/zenodo.17555447
DOI (publication): 10.3847/1538-4357/ae1475


# DATA AND FILE OVERVIEW

## Data Files

Files: s153050kedata.txt, s153050kr.txt, s201620kedata.txt, s201620kr.txt, s201950kedata.txt, s201950kr.txt, s202260kedata.txt, s202260kr.txt, s202670kedata.txt, s202670kr.txt, s202940kedata.txt, s202940kr.txt, s232130kedata.txt, s232130kr.txt, s272210kedata.txt, s272210kr.txt, sphericalavgs153050kedata.txt, sphericalavgs153050kr.txt, sphericalavgs272210kedata.txt, sphericalavgs272210kr.txt

Format: csv

Data description:
- kedata files (s153050kedata.txt, s201620kedata.txt, etc.): Single column containing kinetic energy values in erg
    *Columns:
    - Integrated specific kinetic energy power spectrum in the gain region for a given wavenumber [cm^6/s^2]

- kr files (s153050kr.txt, s201620kr.txt, etc.): 
    *Columns:
    -Radial wavenumbers k_r [cm^-1]

## Python script for analysis:

Figure_7.py

Python packages required:
- numpy
- matplotlib
- cmasher


(EOF)
