Semi Analytical Method for simulating Solar Atmospheric GAmma-ray flux
In the repo, please find our poster here. We are glad to share that the poster Proton Motion obtained Best Poster Award 3rd Prize in SURIP 2021 in CUHK Physics!
This repository simulates the SAγ flux with a semi-analytical method to reduce the time cost of a full simulation. We combined the observational data of solar magnetic field and the simulation on cosmic-ray protons' motion.
Please run the following to compute the simulate the trajectory of cosmic-ray protons' motion in the Sun:
# Build docker image
make build
# After modifying config/config.yml for configuration of simulation
# Start docker container
make start
# If you want to check the available Carrington Rotations
make args="--show" start
# If you need to download HMI map data
make email=<your email> start
# Remove all docker container
make cleanPlease run the following to set up the Jupyter server for development or data visualization:
# Set up Jupyter server (default port=8888 if no input)
# This is for development or data visualization
make port=<port> jupyter_up
# Kill Jupyter server
make jupyter_downAfter set up the server, you can go to here and the password is samsaga.