Evidence of Alfvenic Poynting Flux as the Primary Driver of Auroral Motion During a Geomagnetic Substorm
Author ORCID Identifier
Ferradas, Cristian http://orcid.org/0000-0002-6931-1793 Larsen, Brian A-7822-2011 http://orcid.org/0000-0003-4515-0208 Reeves, Geoffrey E-8101-2011 http://orcid.org/0000-0002-7985-8098 Igl, Alexander http://orcid.org/0000-0002-2844-5613
Geomagnetic substorms are major energy transfer events where energy stored in the Earth's magnetotail is released into the ionosphere. Substorm phenomena, including auroral activities, earthward Poynting flux, magnetic field dipolarization, etc, have been extensively studied. However, the complex interplay among them is not fully understood. In a fortuitous event on June 7, 2013, the twin Van Allen Probes (separated by 0.4 h in local time) observed bursts of earthward Alfvenic Poynting flux in the vicinity of the plasma sheet boundary layer (PSBL). The Poynting flux bursts correlate with enhancements of auroral brightness around the footpoints of both spacecraft. This indicates a temporal and spatial correlation between the auroral brightening and Poynting flux bursts, and that the auroral motion is directly linked to the perpendicular expansion of the Alfven wave. These observations suggest that the Alfvenic Poynting flux is a primary driver for the auroral electron acceleration. Around the time of auroral brightening, a dipolarization was seen to propagate more than 4 h in local time during a 20 min period. The azimuthal phase speed of this dipolarization (2 deg/min) is too small to explain the azimuthal motion of the aurora (13.6 deg/min), but the dipolarization could be related to the generation of the Alfvenic Poynting flux through phase mixing at strong density gradients like those in the PSBL.
Publication Source (Journal or Book title)
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
Tian, S., Colpitts, C. A., Wygant, J. R., Cattell, C. A., Ferradas, C. P., Igl, A. B., Larsen, B. A., Reeves, G. D., & Donovan, E. F. (2021). Evidence of Alfvenic Poynting Flux as the Primary Driver of Auroral Motion During a Geomagnetic Substorm. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 126 (5) https://doi.org/10.1029/2020JA029019