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

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https://doi.org/10.13020/kbp7-dd42
https://hdl.handle.net/11299/227516

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Keywords

ULF Waves

Magnetosphere-Ionosphere Coupling

Cavity Modes

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

Published Date

2022-05-19

Authors

Lysak, Robert L

Group

University of Minnesota School of Physics and Astronomy Space Physics Group

Author Contact

Lysak, Robert L
lysak001@umn.edu

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Dataset

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

Related to

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

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License

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)

Funding information

NSF Grant AGS 1840891

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Previously Published Citation

Suggested citation

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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