First direct observations of interplanetary shock impact angle effects on actual geomagnetically induced currents: The case of the Finnish natural gas pipeline system

dc.contributor.authorOliveira, Denny
dc.contributor.authorZesta, Eftyhia
dc.contributor.authorVidal-Luengo, Sergio
dc.date.accessioned2024-08-07T14:07:11Z
dc.date.available2024-08-07T14:07:11Z
dc.date.issued2024-07-09
dc.description.abstractThe impact of interplanetary (IP) shocks on the Earth’s magnetosphere can greatly disturb the geomagnetic field and electric currents in the magnetosphere-ionosphere system. At high latitudes, the current systems most affected by the shocks are the auroral electrojet currents. These currents then generate ground geomagnetically induced currents that couple with and are highly detrimental to ground artificial conductors including power transmission lines, oil/gas pipelines, railways, and submarine cables. Recent research has shown that the shock impact angle, the angle the shock normal vector performs with the Sun-Earth line, plays a major role in controlling the subsequent geomagnetic activity. More specifically, due to more symmetric magnetospheric compressions, nearly frontal shocks are usually more geoeffective than highly inclined shocks. In this study, we utilize a subset (332 events) of a shock list with more than 600 events to investigate, for the first time, shock impact angle effects on the subsequent GICs right after shock impact (compression effects) and several minutes after shock impact (substorm-like effects). We use GIC recordings from the Finnish natural gas pipeline performed near the Mäntsälä compression station in southern Finland. We find that GIC peaks (> 5 A) occurring after shock impacts are mostly caused by nearly frontal shocks and occur in the post-noon/dusk magnetic local time sector. These GIC peaks are presumably triggered by partial ring current intensifications in the dusk sector. On the other hand, more intense GIC peaks (> 20 A) generally occur several minutes after shock impacts and are located around the magnetic midnight terminator. These GIC peaks are most likely caused by intense energetic particle injections from the magnetotail which frequently occur during substorms. The results of this work are relevant to studies aiming at predicting GICs following solar wind driving under different levels of asymmetric solar wind forcing.
dc.description.sponsorshipThe author(s) declare that financial support was received for the research, authorship, and/or publication of this article. DMO and EZ thank the financial support provided by the NASA HGIO program through grant 80NSSC22K0756. DMO and SVL acknowledge the financial support provided by NASA LWS program through grant NNH22ZDA001N-LWS.
dc.description.urihttps://www.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2024.1392697/full
dc.format.extent18 pages
dc.genrejournal articles
dc.identifierdoi:10.13016/m2v2p4-mzjk
dc.identifier.citationOliveira, Denny M., Eftyhia Zesta, and Sergio Vidal-Luengo. “First Direct Observations of Interplanetary Shock Impact Angle Effects on Actual Geomagnetically Induced Currents: The Case of the Finnish Natural Gas Pipeline System.” Frontiers in Astronomy and Space Sciences 11 (July 10, 2024). https://doi.org/10.3389/fspas.2024.1392697.
dc.identifier.urihttps://doi.org/10.3389/fspas.2024.1392697
dc.identifier.urihttp://hdl.handle.net/11603/35172
dc.language.isoen
dc.publisherFrontiers
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsCC BY 4.0 Deed ATTRIBUTION 4.0 INTERNATIONAL
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectionospheric response
dc.subjectgeospace response
dc.subjectGeomagnetic activity
dc.subjectshock geometry
dc.subjectinterplanetary shocks
dc.subjectGeomagnetically induced currents
dc.titleFirst direct observations of interplanetary shock impact angle effects on actual geomagnetically induced currents: The case of the Finnish natural gas pipeline system
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0003-2078-7229

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