Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/39424
Title: Magnetospheric response and reconfiguration times following IMF B<inf>y</inf> reversals
Authors: Tenfjord, P.
Østgaard, N.
Strangeway, R.
Haaland, S.
Snekvik, K.
Laundal, K. M.
Reistad, J. P.
Milan, S. E.
First Published: 21-Jan-2017
Publisher: American Geophysical Union (AGU), Wiley
Citation: Journal of Geophysical Research: Space Physics, 2017, 122, 417–431
Abstract: The interaction between the interplanetary magnetic field (IMF) and the geomagnetic field at the dayside magnetopause leads to transfer of momentum and energy which changes the magnetospheric configuration, but only after a certain time. In this study we quantify this time, to advance our understanding of the causes for the delayed response of the magnetosphere. We study the response and reconfiguration time of the inner magnetosphere to IMF By reversals. A superposed epoch analysis of magnetic field measurements from four Geostationary Operational Environmental Satellite spacecraft at different local times both for negative to positive IMF By reversals and for positive to negative reversals is presented. The magnetospheric response time at geosynchronous orbit to the sudden change of IMF By is less than 15 (∼10) min from the bow shock (magnetopause) arrival time, while the reconfiguration time is less than 46 (∼41) min. These results are consistent with a By component induced on closed magnetic field lines due to the asymmetric loading of flux following asymmetric dayside reconnection when IMF By≠0. Our results also confirm our earlier studies that nightside reconnection is not required for generating a By component on closed field lines.
DOI Link: 10.1002/2016JA023018
ISSN: 2169-9380
eISSN: 2169-9402
Links: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023018/abstract
http://hdl.handle.net/2381/39424
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2016, American Geophysical Union (AGU), Wiley. Deposited with reference to the publisher’s open access archiving policy.
Description: The OMNI and GOES data are found here: http://cdaweb.gsfc.nasa.gov. SuperMAG data are available here: http://supermag.jhuapl.edu/. Scientists interested in other data used should contact the corresponding author.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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