Influence of short-term solar disturbances on the fair weather conduction current

The fair weather atmospheric electrical current (Jz) couples the ionosphere to the lower atmosphere and thus provides a route by which changes in solar activity can modify processes in the lower troposphere. This paper examines the temporal variations and spectral characteristics of continuous measu...

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Main Authors: Elhalel Gal, Yair Yoav, Nicoll Keri, Price Colin, Reuveni Yuval, Harrison R. Giles
Format: Article
Language:English
Published: EDP Sciences 2014-01-01
Series:Journal of Space Weather and Space Climate
Online Access:https://www.swsc-journal.org/articles/swsc/full_html/2014/01/swsc130033/swsc130033.html
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spelling doaj-2a55c1de363c4a36a13e1d384568d68d2021-02-02T05:35:53ZengEDP SciencesJournal of Space Weather and Space Climate2115-72512014-01-014A2610.1051/swsc/2014022swsc130033Influence of short-term solar disturbances on the fair weather conduction currentElhalel GalYair YoavNicoll KeriPrice ColinReuveni YuvalHarrison R. GilesThe fair weather atmospheric electrical current (Jz) couples the ionosphere to the lower atmosphere and thus provides a route by which changes in solar activity can modify processes in the lower troposphere. This paper examines the temporal variations and spectral characteristics of continuous measurements of Jz conducted at the Wise Observatory in Mitzpe-Ramon, Israel (30°35′ N, 34°45′ E), during two large CMEs, and during periods of increased solar wind density. Evidence is presented for the effects of geomagnetic storms and sub-storms on low latitude Jz during two coronal mass ejections (CMEs), on 24–25th October 2011 and 7–8th March 2012, when the variability in Jz increased by an order of magnitude compared to normal fair weather conditions. The dynamic spectrum of the increased Jz fluctuations exhibit peaks in the Pc5 frequency range. Similar low frequency characteristics occur during periods of enhanced solar wind proton density. During the October 2011 event, the periods of increased fluctuations in Jz lasted for 7 h and coincided with fluctuations of the inter-planetary magnetic field (IMF) detected by the ACE satellite. We suggest downward mapping of ionospheric electric fields as a possible mechanism for the increased fluctuations.https://www.swsc-journal.org/articles/swsc/full_html/2014/01/swsc130033/swsc130033.html
collection DOAJ
language English
format Article
sources DOAJ
author Elhalel Gal
Yair Yoav
Nicoll Keri
Price Colin
Reuveni Yuval
Harrison R. Giles
spellingShingle Elhalel Gal
Yair Yoav
Nicoll Keri
Price Colin
Reuveni Yuval
Harrison R. Giles
Influence of short-term solar disturbances on the fair weather conduction current
Journal of Space Weather and Space Climate
author_facet Elhalel Gal
Yair Yoav
Nicoll Keri
Price Colin
Reuveni Yuval
Harrison R. Giles
author_sort Elhalel Gal
title Influence of short-term solar disturbances on the fair weather conduction current
title_short Influence of short-term solar disturbances on the fair weather conduction current
title_full Influence of short-term solar disturbances on the fair weather conduction current
title_fullStr Influence of short-term solar disturbances on the fair weather conduction current
title_full_unstemmed Influence of short-term solar disturbances on the fair weather conduction current
title_sort influence of short-term solar disturbances on the fair weather conduction current
publisher EDP Sciences
series Journal of Space Weather and Space Climate
issn 2115-7251
publishDate 2014-01-01
description The fair weather atmospheric electrical current (Jz) couples the ionosphere to the lower atmosphere and thus provides a route by which changes in solar activity can modify processes in the lower troposphere. This paper examines the temporal variations and spectral characteristics of continuous measurements of Jz conducted at the Wise Observatory in Mitzpe-Ramon, Israel (30°35′ N, 34°45′ E), during two large CMEs, and during periods of increased solar wind density. Evidence is presented for the effects of geomagnetic storms and sub-storms on low latitude Jz during two coronal mass ejections (CMEs), on 24–25th October 2011 and 7–8th March 2012, when the variability in Jz increased by an order of magnitude compared to normal fair weather conditions. The dynamic spectrum of the increased Jz fluctuations exhibit peaks in the Pc5 frequency range. Similar low frequency characteristics occur during periods of enhanced solar wind proton density. During the October 2011 event, the periods of increased fluctuations in Jz lasted for 7 h and coincided with fluctuations of the inter-planetary magnetic field (IMF) detected by the ACE satellite. We suggest downward mapping of ionospheric electric fields as a possible mechanism for the increased fluctuations.
url https://www.swsc-journal.org/articles/swsc/full_html/2014/01/swsc130033/swsc130033.html
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