Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect

We use the am, an, as and the a-sigma geomagnetic indices to the explore a previously overlooked factor in magnetospheric electrodynamics, namely the inductive effect of diurnal motions of the Earth's magnetic poles toward and away from the Sun caused by Earth's rotation. Because the offse...

Full description

Bibliographic Details
Main Authors: Lockwood, Mike, Haines, Carl, Barnard, Luke A., Owens, Mathew J., Scott, Chris J., Chambodut, Aude, McWilliams, Kathryn A.
Format: Article in Journal/Newspaper
Language:unknown
Published: arXiv 2020
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.2012.13324
https://arxiv.org/abs/2012.13324
id ftdatacite:10.48550/arxiv.2012.13324
record_format openpolar
spelling ftdatacite:10.48550/arxiv.2012.13324 2023-05-15T16:19:42+02:00 Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect Lockwood, Mike Haines, Carl Barnard, Luke A. Owens, Mathew J. Scott, Chris J. Chambodut, Aude McWilliams, Kathryn A. 2020 https://dx.doi.org/10.48550/arxiv.2012.13324 https://arxiv.org/abs/2012.13324 unknown arXiv Creative Commons Attribution Non Commercial No Derivatives 4.0 International https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode cc-by-nc-nd-4.0 CC-BY-NC-ND Space Physics physics.space-ph Earth and Planetary Astrophysics astro-ph.EP Geophysics physics.geo-ph FOS Physical sciences Article CreativeWork article Preprint 2020 ftdatacite https://doi.org/10.48550/arxiv.2012.13324 2022-03-10T15:14:38Z We use the am, an, as and the a-sigma geomagnetic indices to the explore a previously overlooked factor in magnetospheric electrodynamics, namely the inductive effect of diurnal motions of the Earth's magnetic poles toward and away from the Sun caused by Earth's rotation. Because the offset of the (eccentric dipole) geomagnetic pole from the rotational axis is roughly twice as large in the southern hemisphere compared to the northern, the effects there are predicted to be roughly twice the amplitude. Hemispheric differences have previously been discussed in terms of polar ionospheric conductivities, effects which we allow for by studying the dipole tilt effect on time-of-year variations of the indices. The electric field induced in a geocentric frame is shown to also be a significant factor and gives a modulation of the voltage applied by the solar wind flow in the southern hemisphere of typically a 30% diurnal modulation for disturbed intervals rising to 76% in quiet times. Motion towards/away from the Sun reduces/enhances the directly-driven ionospheric voltages and reduces/enhances the magnetic energy stored in the near-Earth tail: 10% of the effect being directly-driven and 90% being in tail energy storage/release. Combined with the effect of solar wind dynamic pressure and dipole tilt on the pressure balance in the near-Earth tail, the effect provides an excellent explanation of how the observed Russell-McPherron pattern in the driving power input into the magnetosphere is converted into the equinoctial pattern in average geomagnetic activity (after correction is made for dipole tilt effects on ionospheric conductivity), added to a pronounced UT variation with minimum at 02-10UT. In addition, we show that the predicted and observed UT variations in average geomagnetic activity has implications for the occurrence of the largest events that also show the nett UT variation. : Accepted for publication in J. Space Weather Space Clim., contains 23 Figures plus has an Appendix containing 4 Figures Article in Journal/Newspaper Geomagnetic Pole DataCite Metadata Store (German National Library of Science and Technology)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Space Physics physics.space-ph
Earth and Planetary Astrophysics astro-ph.EP
Geophysics physics.geo-ph
FOS Physical sciences
spellingShingle Space Physics physics.space-ph
Earth and Planetary Astrophysics astro-ph.EP
Geophysics physics.geo-ph
FOS Physical sciences
Lockwood, Mike
Haines, Carl
Barnard, Luke A.
Owens, Mathew J.
Scott, Chris J.
Chambodut, Aude
McWilliams, Kathryn A.
Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect
topic_facet Space Physics physics.space-ph
Earth and Planetary Astrophysics astro-ph.EP
Geophysics physics.geo-ph
FOS Physical sciences
description We use the am, an, as and the a-sigma geomagnetic indices to the explore a previously overlooked factor in magnetospheric electrodynamics, namely the inductive effect of diurnal motions of the Earth's magnetic poles toward and away from the Sun caused by Earth's rotation. Because the offset of the (eccentric dipole) geomagnetic pole from the rotational axis is roughly twice as large in the southern hemisphere compared to the northern, the effects there are predicted to be roughly twice the amplitude. Hemispheric differences have previously been discussed in terms of polar ionospheric conductivities, effects which we allow for by studying the dipole tilt effect on time-of-year variations of the indices. The electric field induced in a geocentric frame is shown to also be a significant factor and gives a modulation of the voltage applied by the solar wind flow in the southern hemisphere of typically a 30% diurnal modulation for disturbed intervals rising to 76% in quiet times. Motion towards/away from the Sun reduces/enhances the directly-driven ionospheric voltages and reduces/enhances the magnetic energy stored in the near-Earth tail: 10% of the effect being directly-driven and 90% being in tail energy storage/release. Combined with the effect of solar wind dynamic pressure and dipole tilt on the pressure balance in the near-Earth tail, the effect provides an excellent explanation of how the observed Russell-McPherron pattern in the driving power input into the magnetosphere is converted into the equinoctial pattern in average geomagnetic activity (after correction is made for dipole tilt effects on ionospheric conductivity), added to a pronounced UT variation with minimum at 02-10UT. In addition, we show that the predicted and observed UT variations in average geomagnetic activity has implications for the occurrence of the largest events that also show the nett UT variation. : Accepted for publication in J. Space Weather Space Clim., contains 23 Figures plus has an Appendix containing 4 Figures
format Article in Journal/Newspaper
author Lockwood, Mike
Haines, Carl
Barnard, Luke A.
Owens, Mathew J.
Scott, Chris J.
Chambodut, Aude
McWilliams, Kathryn A.
author_facet Lockwood, Mike
Haines, Carl
Barnard, Luke A.
Owens, Mathew J.
Scott, Chris J.
Chambodut, Aude
McWilliams, Kathryn A.
author_sort Lockwood, Mike
title Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect
title_short Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect
title_full Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect
title_fullStr Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect
title_full_unstemmed Semi-annual, annual and Universal Time variations in the magnetosphere and in geomagnetic activity: 4. Polar Cap motions and origins of the Universal Time effect
title_sort semi-annual, annual and universal time variations in the magnetosphere and in geomagnetic activity: 4. polar cap motions and origins of the universal time effect
publisher arXiv
publishDate 2020
url https://dx.doi.org/10.48550/arxiv.2012.13324
https://arxiv.org/abs/2012.13324
genre Geomagnetic Pole
genre_facet Geomagnetic Pole
op_rights Creative Commons Attribution Non Commercial No Derivatives 4.0 International
https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
cc-by-nc-nd-4.0
op_rightsnorm CC-BY-NC-ND
op_doi https://doi.org/10.48550/arxiv.2012.13324
_version_ 1766006104270045184