Updated Fortran program for modeling ULF waves in a three-dimensional magnetosphere

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Updated Fortran program for modeling ULF waves in a three-dimensional magnetosphere

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2022-05-19

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Lysak, Robert L
lysak001@umn.edu

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Abstract

This is the update of a three-dimensional code in dipole geometry for modeling Ultra-Low-Frequency (ULF) waves. The previous version is at https://doi.org/10.13020/d1g7-c676. This code has been used in a study of so-called Pi2 pulsations in the magnetosphere, which are waves with a period of 1-2 minutes that are commonly observed during substorms. This code has been used in conjunction with analysis of data from the Van Allen Probes mission.

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Fortran source code for modeling ULF waves in the magnetosphere

Referenced by

Takahashi, K., Lysak, R. L., Vellante, M., Wygant, J. R., Kletzing, C. (2022). A Statistical Study of Pi2 Pulsations Observed by Van 2 Allen Probes, submitted to Journal of Geophysical Research: Space Physics
https://doi.org/10.1029/2022ja030674

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NSF Grant AGS 1840891

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Lysak, Robert L. (2022). Updated Fortran program for modeling ULF waves in a three-dimensional magnetosphere. Retrieved from the Data Repository for the University of Minnesota (DRUM), https://doi.org/10.13020/kbp7-dd42.
View/Download file
File View/OpenDescriptionSize
alfdip3d.f90Fortran Source Code54.34 KB
alf3d.datInput data file for alfdip3d1.09 KB
newalfdip.proIDL routines21.36 KB
archive.zipData files used to create the figures in the referenced paper11.35 MB
alfdipupdate.txtCode updates and file descriptions3.33 KB
README.txtDescription of data1.84 KB

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