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

Lysak, Robert L
2022-05-19
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https://doi.org/10.13020/kbp7-dd42
 https://hdl.handle.net/11299/227516
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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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University of Minnesota School of Physics and Astronomy Space Physics Group

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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.

Description

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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A previous version of the code is available here:
 https://doi.org/10.13020/d1g7-c676

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Attribution-NonCommercial-NoDerivs 3.0 United States
 http://creativecommons.org/licenses/by-nc-nd/3.0/us/

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Data Repository for U of M (DRUM)

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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.

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alfdip3d.f90
Fortran Source Code
(54.34 KB)

alf3d.dat
Input data file for alfdip3d
(1.09 KB)

newalfdip.pro
IDL routines
(21.36 KB)

archive.zip
Data files used to create the figures in the referenced paper
(11.35 MB)

alfdipupdate.txt
Code updates and file descriptions
(3.33 KB)

README.txt
Description of data
(1.84 KB)

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