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 offset of the (...

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Published in:Journal of Space Weather and Space Climate
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:English
Published: EDP Sciences 2021
Subjects:
Online Access:https://centaur.reading.ac.uk/95181/
https://centaur.reading.ac.uk/95181/8/swsc200083.pdf
https://centaur.reading.ac.uk/95181/1/390_Lockwood_Paper4n_Fa.pdf
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spelling ftunivreading:oai:centaur.reading.ac.uk:95181 2024-09-09T19:41:03+00:00 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. 2021-02-17 text https://centaur.reading.ac.uk/95181/ https://centaur.reading.ac.uk/95181/8/swsc200083.pdf https://centaur.reading.ac.uk/95181/1/390_Lockwood_Paper4n_Fa.pdf en eng EDP Sciences https://centaur.reading.ac.uk/95181/8/swsc200083.pdf https://centaur.reading.ac.uk/95181/1/390_Lockwood_Paper4n_Fa.pdf Lockwood, M. <https://centaur.reading.ac.uk/view/creators/90001127.html> orcid:0000-0002-7397-2172 , Haines, C., Barnard, L. A. <https://centaur.reading.ac.uk/view/creators/90005020.html> orcid:0000-0001-9876-4612 , Owens, M. J. <https://centaur.reading.ac.uk/view/creators/90003236.html> orcid:0000-0003-2061-2453 , Scott, C. J. <https://centaur.reading.ac.uk/view/creators/90003900.html> orcid:0000-0001-6411-5649 , Chambodut, A. and McWilliams, K. A. (2021) 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. Journal of Space Weather and Space Climate, 11. 15. ISSN 2115-7251 doi: https://doi.org/10.1051/swsc/2020077 <https://doi.org/10.1051/swsc/2020077> cc_by_4 Article PeerReviewed 2021 ftunivreading https://doi.org/10.1051/swsc/2020077 2024-06-25T15:04:04Z 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 of those in the northern hemisphere. Hemispheric differences have previously been discussed in terms of polar ionospheric conductivities generated by solar photoionization, effects which we allow for by looking at the dipole tilt effect on the 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 that is typically a 30% diurnal modulation for disturbed intervals rising to about 76% in quiet times. For the northern hemisphere these are 15% and 38% modulations. Motion towards/away from the Sun reduces/enhances the directly-driven ionospheric voltages and reduces/enhances the magnetic energy stored in the tail and we estimate that approximately 10% of the effect appears in directly driven ionospheric voltages and 90% in changes of the rate of energy storage or release in the near-Earth tail. The hemispheric asymmetry in the geomagnetic pole offsets from the rotational axis is shown to be the dominant factor in driving Universal Time (UT) variations and hemispheric differences in geomagnetic activity. 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 with time-of-year F and UT in the driving power input into the magnetosphere is converted into the equinoctial F - UT pattern in average ... Article in Journal/Newspaper Geomagnetic Pole CentAUR: Central Archive at the University of Reading Journal of Space Weather and Space Climate 11 15
institution Open Polar
collection CentAUR: Central Archive at the University of Reading
op_collection_id ftunivreading
language English
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 of those in the northern hemisphere. Hemispheric differences have previously been discussed in terms of polar ionospheric conductivities generated by solar photoionization, effects which we allow for by looking at the dipole tilt effect on the 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 that is typically a 30% diurnal modulation for disturbed intervals rising to about 76% in quiet times. For the northern hemisphere these are 15% and 38% modulations. Motion towards/away from the Sun reduces/enhances the directly-driven ionospheric voltages and reduces/enhances the magnetic energy stored in the tail and we estimate that approximately 10% of the effect appears in directly driven ionospheric voltages and 90% in changes of the rate of energy storage or release in the near-Earth tail. The hemispheric asymmetry in the geomagnetic pole offsets from the rotational axis is shown to be the dominant factor in driving Universal Time (UT) variations and hemispheric differences in geomagnetic activity. 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 with time-of-year F and UT in the driving power input into the magnetosphere is converted into the equinoctial F - UT pattern in average ...
format Article in Journal/Newspaper
author Lockwood, Mike
Haines, Carl
Barnard, Luke A.
Owens, Mathew J.
Scott, Chris J.
Chambodut, Aude
McWilliams, Kathryn A.
spellingShingle 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
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 EDP Sciences
publishDate 2021
url https://centaur.reading.ac.uk/95181/
https://centaur.reading.ac.uk/95181/8/swsc200083.pdf
https://centaur.reading.ac.uk/95181/1/390_Lockwood_Paper4n_Fa.pdf
genre Geomagnetic Pole
genre_facet Geomagnetic Pole
op_relation https://centaur.reading.ac.uk/95181/8/swsc200083.pdf
https://centaur.reading.ac.uk/95181/1/390_Lockwood_Paper4n_Fa.pdf
Lockwood, M. <https://centaur.reading.ac.uk/view/creators/90001127.html> orcid:0000-0002-7397-2172 , Haines, C., Barnard, L. A. <https://centaur.reading.ac.uk/view/creators/90005020.html> orcid:0000-0001-9876-4612 , Owens, M. J. <https://centaur.reading.ac.uk/view/creators/90003236.html> orcid:0000-0003-2061-2453 , Scott, C. J. <https://centaur.reading.ac.uk/view/creators/90003900.html> orcid:0000-0001-6411-5649 , Chambodut, A. and McWilliams, K. A. (2021) 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. Journal of Space Weather and Space Climate, 11. 15. ISSN 2115-7251 doi: https://doi.org/10.1051/swsc/2020077 <https://doi.org/10.1051/swsc/2020077>
op_rights cc_by_4
op_doi https://doi.org/10.1051/swsc/2020077
container_title Journal of Space Weather and Space Climate
container_volume 11
container_start_page 15
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