Measurement of the stochasticity of low-latitude geomagnetic temporal variations

Ground magnetometer measurements of total magnetic field strength from 6 stations at low latitudes were analyzed using power spectrum and Hurst range scaling techniques. The Hurst exponents for most of these time-series were near 0.5, which indicates stochasticity, with the highest latitude...

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Main Authors: J. A. Wanliss, M. A. Reynolds
Format: Article
Language:English
Published: Copernicus Publications 2003-09-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/21/2025/2003/angeo-21-2025-2003.pdf
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author J. A. Wanliss
M. A. Reynolds
author_facet J. A. Wanliss
M. A. Reynolds
author_sort J. A. Wanliss
collection DOAJ
description Ground magnetometer measurements of total magnetic field strength from 6 stations at low latitudes were analyzed using power spectrum and Hurst range scaling techniques. The Hurst exponents for most of these time-series were near 0.5, which indicates stochasticity, with the highest latitude stations exhibiting some persistence with Hurst exponents greater than 0.6. Although no definite correlations are evident, the relative increase of the Hurst exponent with latitude suggests the possibility that the underlying dynamics of the magnetosphere change with latitude. This result may help quantify the dynamics of the inner magnetosphere itself without the direct presence of the solar wind driver.<br><br><b>Key words. </b>Magnetospheric physics (magnetospheric configuration and dynamics; plasmasphere) – Space plasma physics (nonlinear phenomena)
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spelling doaj.art-3ce53715bcf04be6946249ef319c68872022-12-22T03:37:00ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762003-09-01212025203010.5194/angeo-21-2025-2003Measurement of the stochasticity of low-latitude geomagnetic temporal variationsJ. A. Wanliss0M. A. ReynoldsDepartment of Physical Sciences, Embry-Riddle Aeronautical University, 600 S. Clyde Morris Blvd., Daytona Beach, FL 32114, USAGround magnetometer measurements of total magnetic field strength from 6 stations at low latitudes were analyzed using power spectrum and Hurst range scaling techniques. The Hurst exponents for most of these time-series were near 0.5, which indicates stochasticity, with the highest latitude stations exhibiting some persistence with Hurst exponents greater than 0.6. Although no definite correlations are evident, the relative increase of the Hurst exponent with latitude suggests the possibility that the underlying dynamics of the magnetosphere change with latitude. This result may help quantify the dynamics of the inner magnetosphere itself without the direct presence of the solar wind driver.<br><br><b>Key words. </b>Magnetospheric physics (magnetospheric configuration and dynamics; plasmasphere) – Space plasma physics (nonlinear phenomena)https://www.ann-geophys.net/21/2025/2003/angeo-21-2025-2003.pdf
spellingShingle J. A. Wanliss
M. A. Reynolds
Measurement of the stochasticity of low-latitude geomagnetic temporal variations
Annales Geophysicae
title Measurement of the stochasticity of low-latitude geomagnetic temporal variations
title_full Measurement of the stochasticity of low-latitude geomagnetic temporal variations
title_fullStr Measurement of the stochasticity of low-latitude geomagnetic temporal variations
title_full_unstemmed Measurement of the stochasticity of low-latitude geomagnetic temporal variations
title_short Measurement of the stochasticity of low-latitude geomagnetic temporal variations
title_sort measurement of the stochasticity of low latitude geomagnetic temporal variations
url https://www.ann-geophys.net/21/2025/2003/angeo-21-2025-2003.pdf
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AT mareynolds measurementofthestochasticityoflowlatitudegeomagnetictemporalvariations