Westward traveling surges: Sliding along boundary arcs and distinction from onset arc brightening. Issue 12 (12th December 2013)

• Record Type: Journal Article
• Authors: Lyons, L. R.; Nishimura, Y.; Gallardo‐Lacourt, B.; Zou, Y.; Donovan, E.; Mende, S.; Angelopoulos, V.; M. Ruohoniemi, J.; McWilliams, K.
• Is Part Of: Journal of geophysical research. Volume 118:Issue 12(2013:Dec.)
• Page Start: 7643
• Page End: 7653
• Publication Date: 2013-12-12
• Subjects: Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2013JA019334
• Languages: English
• ISSNs: 2169-9380

Abstract

<abstract abstract-type="main"> <title> <x xml:space="preserve">Abstract</x> </title> <p>[1] After onset, auroral brightening rapidly spreads azimuthally along the onset arc, typically, but not always, extending substantially farther westward than eastward. Expansion‐phase auroras also expand poleward and can contact an arc along the auroral poleward boundary. For such events, we find that poleward expansion of the region of active aurora accelerates after contact, forming a bulge region that protrudes into the preexisting polar cap and expands westward as the westward traveling surge. This westward motion is slower than, and initiates later than, the azimuthal spreading of the onset arc brightening. The poleward boundary arc remains connected to the surge as the surge slides along the equatorward moving edge of the boundary arc, and this connection appears to set off the westward traveling, poleward protruding activity of the surge via localized polar cap flow adjacent to the boundary arc. Ground magnetic signatures show a relatively weak <italic>H</italic> component depression moving westward with the onset arc brightening, and a delayed substantially larger depression moving with the westward propagating surge that must be associated with a substantially larger westward ionospheric current. The clear distinction between onset arc brightening and the westward traveling surge seen in auroral and magnetometer current signatures implies that their underlying processes are very different. Evidence suggests that flow channels adjacent to the boundary arc possibly feed surge development. These results are consistent with current wedge formation being more associated with post‐onset activity than with onset, and with flow channels from the polar cap being important for surge/bulge development.</p> </abstract>