Journal
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
Volume 124, Issue 6, Pages 4710-4724Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2018JA026245
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Funding
- Canadian Space Agency's Geospace Observatory (GO Canada) continuation initiative
- Italian National Research Council
- National Program for Antarctic Research
- NSERC Discovery grant
- NSERC USRA
- CSA
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Cross-track ion drifts measured by the Swarm A satellite are compared with colocated line-of-sight Super Dual Auroral Radar Network (SuperDARN) velocities in approximately the same directions. More than 200 Swarm A passes over four polar cap SuperDARN radars in the Northern and Southern Hemispheres are considered. Overall, the Swarm-based velocities are larger than the SuperDARN velocities; the slope of the best fit line to the data is similar to 0.67. Somewhat stronger differences are found when Swarm A measurements for the entire year 2016 are compared with SuperDARN vector data from global-scale convection maps. Swarm ion drift data demonstrate known features of the high-latitude convection patterns, for example, reverse convection cells at interplanetary magnetic field B-z > 0. The latitudes of the convection reversal boundary inferred from SuperDARN are found to be in reasonable agreement with those determined from Swarm A and Swarm B, with Swarm-based latitudes occurring roughly 1 degrees more equatorward, typically.
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