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

International audience We use the am, an, as and the aσ 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....

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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.
Other Authors: Ecole et Observatoire des Sciences de la Terre (EOST), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2021
Subjects:
Online Access:https://hal-insu.archives-ouvertes.fr/insu-03707763
https://hal-insu.archives-ouvertes.fr/insu-03707763/document
https://hal-insu.archives-ouvertes.fr/insu-03707763/file/swsc200083.pdf
https://doi.org/10.1051/swsc/2020077
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spelling ftinsu:oai:HAL:insu-03707763v1 2023-06-18T03:40:41+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. Ecole et Observatoire des Sciences de la Terre (EOST) Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) 2021 https://hal-insu.archives-ouvertes.fr/insu-03707763 https://hal-insu.archives-ouvertes.fr/insu-03707763/document https://hal-insu.archives-ouvertes.fr/insu-03707763/file/swsc200083.pdf https://doi.org/10.1051/swsc/2020077 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2012.13324 info:eu-repo/semantics/altIdentifier/doi/10.1051/swsc/2020077 insu-03707763 https://hal-insu.archives-ouvertes.fr/insu-03707763 https://hal-insu.archives-ouvertes.fr/insu-03707763/document https://hal-insu.archives-ouvertes.fr/insu-03707763/file/swsc200083.pdf ARXIV: 2012.13324 BIBCODE: 2021JSWSC.11.15L doi:10.1051/swsc/2020077 http://creativecommons.org/licenses/by/ info:eu-repo/semantics/OpenAccess Journal of Space Weather and Space Climate https://hal-insu.archives-ouvertes.fr/insu-03707763 Journal of Space Weather and Space Climate, 2021, 11, ⟨10.1051/swsc/2020077⟩ magnetosphere geomagnetic activity Universal Time variations polar cap motions dipole tilt effects Physics - Space Physics Astrophysics - Earth and Planetary Astrophysics Physics - Geophysics [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 2021 ftinsu https://doi.org/10.1051/swsc/2020077 2023-06-05T20:26:36Z International audience We use the am, an, as and the aσ 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 ±76% in quiet times. For the northern hemisphere these are 15% and 38% modulations. Motion away from/towards 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 ... Article in Journal/Newspaper Geomagnetic Pole Institut national des sciences de l'Univers: HAL-INSU Journal of Space Weather and Space Climate 11 15
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic magnetosphere
geomagnetic activity
Universal Time variations
polar cap motions
dipole tilt effects
Physics - Space Physics
Astrophysics - Earth and Planetary Astrophysics
Physics - Geophysics
[SDU]Sciences of the Universe [physics]
spellingShingle magnetosphere
geomagnetic activity
Universal Time variations
polar cap motions
dipole tilt effects
Physics - Space Physics
Astrophysics - Earth and Planetary Astrophysics
Physics - Geophysics
[SDU]Sciences of the Universe [physics]
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 magnetosphere
geomagnetic activity
Universal Time variations
polar cap motions
dipole tilt effects
Physics - Space Physics
Astrophysics - Earth and Planetary Astrophysics
Physics - Geophysics
[SDU]Sciences of the Universe [physics]
description International audience We use the am, an, as and the aσ 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 ±76% in quiet times. For the northern hemisphere these are 15% and 38% modulations. Motion away from/towards 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 ...
author2 Ecole et Observatoire des Sciences de la Terre (EOST)
Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
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 HAL CCSD
publishDate 2021
url https://hal-insu.archives-ouvertes.fr/insu-03707763
https://hal-insu.archives-ouvertes.fr/insu-03707763/document
https://hal-insu.archives-ouvertes.fr/insu-03707763/file/swsc200083.pdf
https://doi.org/10.1051/swsc/2020077
genre Geomagnetic Pole
genre_facet Geomagnetic Pole
op_source Journal of Space Weather and Space Climate
https://hal-insu.archives-ouvertes.fr/insu-03707763
Journal of Space Weather and Space Climate, 2021, 11, ⟨10.1051/swsc/2020077⟩
op_relation info:eu-repo/semantics/altIdentifier/arxiv/2012.13324
info:eu-repo/semantics/altIdentifier/doi/10.1051/swsc/2020077
insu-03707763
https://hal-insu.archives-ouvertes.fr/insu-03707763
https://hal-insu.archives-ouvertes.fr/insu-03707763/document
https://hal-insu.archives-ouvertes.fr/insu-03707763/file/swsc200083.pdf
ARXIV: 2012.13324
BIBCODE: 2021JSWSC.11.15L
doi:10.1051/swsc/2020077
op_rights http://creativecommons.org/licenses/by/
info:eu-repo/semantics/OpenAccess
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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