Description: An efficient algorithm for identification of PIL on Solar Dynamic Observatory (SDO) Helioseismic and Magnetic Imager (HMI) magnetograms.
Detailed description will appear in the paper: Volobuev, D.M.
Polarity-Inversion Line Preceding X-class Flare, Solar Physics,
Initial data (65 megabyte .fits magnetograms) can be downloaded from http://hmi.stanford.edu/
- Model_test_PIL_Open.m script - calculates parameters of the example(simulated S-curve)
- SDO_PIL_Open.m script - identifies PIL on SDO magnetogram and calculates its parameters
- 5 functions are used within these scripts
To Search:
File list (Check if you may need any files):
KMvD.m
Model_test_PIL_Open.m
PIL_Open.m
SDO_PIL_Open.m
dilate_n.m
license.txt
min_dist.m
select_dipoles.m
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