Description of model can be found in ./paper.pdf
git clone https://github.come/peijin94/SEMP.git
cd SEMP
python -m pip install .
demo in Jupyter notebook in demo-ipynb folder
CDF data format NASA online database.
cdflib is used for reading CDF files.
Download demo data:
run this to download the data to parent folder
cd ../
gdown --folder https://drive.google.com/drive/folders/1y7--cGBXU3gsYz2nZ_kI_5plRAHQY4MO
Step-by-step demo (matlab):
Install Matlab 2018b or newer then,
git clone https://github.com/peijin94/SEMP.git
cd SEMP/matlabsemp
Run the runMe_gui.m
- Load data files of CDF format
- Input the poistions of WIND and STEREO
- Select the time range which contains a event
- Select the frequency channels
- Mark the leading edge (fun part)
- Start the 'Best Model Finding Process' by click 'NextStep'
Click "import" button in the LoadData GUI, and click all the 'NextStep' way down to see the result
The final step may take a few minutes to find the best solution for the radio source trajectory, thank you for the patience.
(Please let me know if there is a problem using this code, contact me: pjer1316_AT_gmail.com)
Make sure to cite the paper if you use the idea or code in this repo:
@Article{Zhang2019,
author="Zhang, Peijin
and Wang, Chuanbing
and Ye, Lin
and Wang, Yuming",
title="Forward Modeling of the Type III Radio Burst Exciter",
journal="Solar Physics",
year="2019",
month="May",
day="22",
volume="294",
number="5",
pages="62",
issn="1573-093X",
doi="10.1007/s11207-019-1448-0",
url="https://doi.org/10.1007/s11207-019-1448-0"
}