Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/45137
Title: Separation and Quantification of Ionospheric Convection Sources: 2. The Dipole Tilt Angle Influence on Reverse Convection Cells During Northward IMF
Authors: Reistad, JP
Laundal, KM
Østgaard, N
Ohma, A
Thomas, EG
Haaland, S
Oksavik, K
Milan, SE
First Published: 4-Jul-2019
Publisher: American Geophysical Union (AGU), Wiley
Citation: Journal of Geophysical Research: Space Physics, 2019, 124
Abstract: This paper investigates the influence of Earth's dipole tilt angle on the reverse convection cells (sometimes referred to as lobe cells) in the Northern Hemisphere ionosphere during northward IMF, which we relate to high-latitude reconnection. Super Dual Auroral Radar Network plasma drift observations in 2010–2016 are used to quantify the ionospheric convection. A novel technique based on Spherical Elementary Convection Systems (SECS) that was presented in our companion paper (Reistad et al., 2019, https://doi.org/10.1029/2019JA026634) is used to isolate and quantify the reverse convection cells. We find that the dipole tilt angle has a linear influence on the reverse cell potential. In the Northern Hemisphere the reverse cell potential is typically two times higher in summer than in winter. This change is interpreted as the change in interplanetary magnetic field-lobe reconnection rate due to the orientation of the dipole tilt. Hence, the dipole tilt influence on reverse ionospheric convection can be a significant modification of the more known influence from vswBz. These results could be adopted by the scientific community as key input parameters for lobe reconnection coupling functions.
DOI Link: 10.1029/2019JA026641
ISSN: 2169-9380
eISSN: 2169-9402
Links: https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2019JA026641
http://hdl.handle.net/2381/45137
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © the authors, 2019. This is an open-access article distributed under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives License (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.
Description: This article is a companion to Reistad et al. (2019), https://doi.org/10.1029/2019JA026634. http://hdl.handle.net/2381/45136
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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