This package processes SDO data to recover trends in the center-to-limbv ariability of the solar radial velocity. v0.x.y is described in Palumbo et al. (2024b). The results of this paper can be reproduced using the showyourwork workflow from this repo.
The sdo-clv-pipeline package can be trivially installed using the uv tool:
git clone https://github.com/palumbom/sdo-clv-pipeline.git
cd sdo-clv-pipeline
uv syncThen in Python, simply:
import sdo_clv_pipeline
If you use this code in your research, please cite the relevant software release and paper.
This repo is maintained by Michael Palumbo. You may may contact him via his email - mpalumbo@flatironinstitute.org