Distributions of Birkeland current density observed by AMPERE are heavy-tailed or long-tailed
Distributions of Birkeland current density observed by AMPERE are heavy-tailed or long-tailed
We analyze probability distributions of Birkeland current densities measured by the Active Magnetosphere and Planetary Electrodynamics Response Experiment. We find that the distributions are leptokurtic rather than normal and they are sometimes heavy-tailed. We fit q-exponential functions to the distributions and use these to estimate where the largest currents are likely to occur. The shape and scale parameters of the fitted q-exponential distribution vary with location: The scale parameter maximizes for current densities with the same polarity and in the same location as the average Region 1 current, whereas the shape parameter maximizes for current densities with the same polarity and in the same location as the average Region 2 current. We find that current densities |J| ≥ 0.2 μA m−2 are most likely to occur in the average Region 1 current region, and second most likely to occur in the average Region 2 current region. However, for extreme currents (|J| ≥ 4.0 μA m−2), we find that the most likely location is colocated with the average Region 2 current region on the dayside, at a colatitude of 18°−22°.
Birkeland currents, distributions, field-aligned currents, q-exponential, space weather, Tsallis statistics
Coxon, John C.
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Chisham, Gareth
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Freeman, Mervyn P.
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Anderson, Brian J.
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Fear, Robert C.
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23 January 2022
Coxon, John C.
566baea5-6a30-4855-bde3-a09c115efde4
Chisham, Gareth
25a4afbd-b568-49c4-a881-206da96f8425
Freeman, Mervyn P.
dc974e00-a73d-4d41-a2a8-3c5aebd7a5b5
Anderson, Brian J.
c30e4de5-7757-4c54-a05d-43369e879c0c
Fear, Robert C.
8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
Coxon, John C., Chisham, Gareth, Freeman, Mervyn P., Anderson, Brian J. and Fear, Robert C.
(2022)
Distributions of Birkeland current density observed by AMPERE are heavy-tailed or long-tailed.
Journal of Geophysical Research: Space Physics, 127 (2), [e2021JA029801].
(doi:10.1029/2021JA029801).
Abstract
We analyze probability distributions of Birkeland current densities measured by the Active Magnetosphere and Planetary Electrodynamics Response Experiment. We find that the distributions are leptokurtic rather than normal and they are sometimes heavy-tailed. We fit q-exponential functions to the distributions and use these to estimate where the largest currents are likely to occur. The shape and scale parameters of the fitted q-exponential distribution vary with location: The scale parameter maximizes for current densities with the same polarity and in the same location as the average Region 1 current, whereas the shape parameter maximizes for current densities with the same polarity and in the same location as the average Region 2 current. We find that current densities |J| ≥ 0.2 μA m−2 are most likely to occur in the average Region 1 current region, and second most likely to occur in the average Region 2 current region. However, for extreme currents (|J| ≥ 4.0 μA m−2), we find that the most likely location is colocated with the average Region 2 current region on the dayside, at a colatitude of 18°−22°.
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JGR Space Physics - 2022 - Coxon - Distributions of Birkeland Current Density Observed by AMPERE are Heavy‐Tailed or
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Accepted/In Press date: 10 January 2022
Published date: 23 January 2022
Keywords:
Birkeland currents, distributions, field-aligned currents, q-exponential, space weather, Tsallis statistics
Identifiers
Local EPrints ID: 491410
URI: http://eprints.soton.ac.uk/id/eprint/491410
ISSN: 2169-9380
PURE UUID: bb616526-91ef-4359-bf06-a4299830b730
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Date deposited: 21 Jun 2024 17:07
Last modified: 22 Jun 2024 01:47
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Author:
Gareth Chisham
Author:
Mervyn P. Freeman
Author:
Brian J. Anderson
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