Interhemispheric Asymmetries in the Ground Magnetic Response to Interplanetary Shocks: The Role of Shock Impact Angle
dc.contributor.author | Xu, Z. | en |
dc.contributor.author | Hartinger, Michael D. | en |
dc.contributor.author | Oliveira, Denny M. | en |
dc.contributor.author | Coyle, Shane | en |
dc.contributor.author | Clauer, C. Robert | en |
dc.contributor.author | Weimer, Daniel R. | en |
dc.contributor.author | Edwards, T. R. | en |
dc.contributor.department | Electrical and Computer Engineering | en |
dc.date.accessioned | 2021-01-06T13:38:20Z | en |
dc.date.available | 2021-01-06T13:38:20Z | en |
dc.date.issued | 2020-03 | en |
dc.description.abstract | Interplanetary (IP) shocks drive magnetosphere-ionosphere (MI) current systems that in turn are associated with ground magnetic perturbations. Recent work has shown that IP shock impact angle plays a significant role in controlling the subsequent geomagnetic activity and magnetic perturbations; for example, highly inclined shocks drive asymmetric MI responses due to interhemispherical asymmetric magnetospheric compressions, while almost head-on shocks drive more symmetric MI responses. However, there are few observations confirming that inclined shocks drive such asymmetries in the high-latitude ground magnetic response. We use data from a chain of Antarctic magnetometers, combined with magnetically conjugate stations on the west coast of Greenland, to test these model predictions (Oliveira & Raeder, 2015, https://doi.org/10.1002/2015JA021147; Oliveira, 2017, https://doi.org/10.1007/s13538-016-0472-x). We calculate the time derivative of the magnetic field (partial derivative B/partial derivative t) in each hemisphere separately. Next, we examine the ratio of Northern to Southern Hemisphere partial derivative B/partial derivative t intensities and the time differences between the maximum. partial derivative B/partial derivative t immediately following the impact of IP shocks. We order these results according to shock impact angles obtained from a recently published database with over 500 events and discuss how shock impact angles affect north-south hemisphere asymmetries in the ground magnetic response. We find that the hemisphere the shock strikes first usually has (1) the first response in partial derivative B/partial derivative t and (2) the most intense response in partial derivative B/partial derivative t. Additionally, we show that highly inclined shocks can generate high-latitude ground magnetic responses that differ significantly from predictions based on models that assume symmetric driving conditions. | en |
dc.description.notes | Z. Xu and M.D. Hartinger were supported by NSF1543364 and 1744828. D.M. Oliveira acknowledges the NASA Grant HISFM18-HIF (Heliophysics Innovation Fund). All data used in the analysis are publicly available at the following repositories: AALPIP magnetometer at mist.nianet.org or NASA CDAWeb, DTU 10s Greenland magnetometer data the Tromso Geophysical Observatory at http://flux.phys.uit.no/geomag.html.The shock database is available in the supporting information of publications cited in the text. | en |
dc.description.sponsorship | NASANational Aeronautics & Space Administration (NASA) [HISFM18-HIF]; [NSF1543364]; [1744828]; Directorate For GeosciencesNational Science Foundation (NSF)NSF - Directorate for Geosciences (GEO) [1744828] Funding Source: National Science Foundation; Office of Polar Programs (OPP)National Science Foundation (NSF)NSF - Directorate for Geosciences (GEO) [1744828] Funding Source: National Science Foundation | en |
dc.format.mimetype | application/pdf | en |
dc.identifier.doi | https://doi.org/10.1029/2019SW002427 | en |
dc.identifier.eissn | 1542-7390 | en |
dc.identifier.issue | 3 | en |
dc.identifier.other | e2019SW002427 | en |
dc.identifier.uri | http://hdl.handle.net/10919/101759 | en |
dc.identifier.volume | 18 | en |
dc.language.iso | en | en |
dc.rights | Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International | en |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | en |
dc.title | Interhemispheric Asymmetries in the Ground Magnetic Response to Interplanetary Shocks: The Role of Shock Impact Angle | en |
dc.title.serial | Space Weather-The International Journal of Research And Applications | en |
dc.type | Article - Refereed | en |
dc.type.dcmitype | Text | en |
dc.type.dcmitype | StillImage | en |
Files
Original bundle
1 - 1 of 1
Loading...
- Name:
- 2019SW002427.pdf
- Size:
- 5.67 MB
- Format:
- Adobe Portable Document Format
- Description: