Published August 13, 2019 | Version v1

Magnetospheric `penetration' of IMF By viewed through the lens of an empirical RBF modeling

  • 1. Saint-Petersburg State University

Description

(1) The model sample source code (fortran), named B_calculation_sample_source_code.for

(2) Two data files for IMF Bz>0 and Bz<0 with self-explanatory filenames Bz_gt_0_All_By.dat and Bz_lt_0_All_By.dat 

(3) A text file, named Data_format.txt, with a description of the data format of the above data files. 
(4) A file Kurihara_3D_grid.dat containing coordinates of the RBF grid nodes (required as input to the model source code)

(5) Two model input parameter files, named Parameters_Negative_IMF_Bz.par and Parameters_Positive_IMF_Bz.par

(6)  A file TA15_Model_description.pdf  with details on the interplanetary N- and B-indices, included in the data files

Notes

The authors acknowledge the support of Russian Fund for Basic Research (RFBR) 17-05-00415

Files

Data_format.txt

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