A new auroral feature: The nightside gap

Details A new auroral feature: The nightside gap A new auroral feature: The nightside gap

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998georl..25.3747c&link_type=abstract

Geophysical Research Letters, Volume 25, Issue 20, p. 3747-3750

Physics

Plasma Physics

6

Space Plasma Physics: Discontinuities, Magnetospheric Physics: Auroral Phenomena, Magnetospheric Physics: Storms And Substorms, Magnetospheric Physics: Magnetosphere/Ionosphere Interactions

Scientific paper

Using images from the Ultraviolet Imager (UVI) aboard the Polar spacecraft, we identify an unusual morphological feature of the auroral oval marked by roughly a factor of four decrease in auroral luminosity near local midnight during some substorms. This feature has not been previously described in detail. The nightside gap appears in roughly 7% of the substorms observed by UVI during our study period from December, 1996 to February, 1997. Two nightside gap events from this period are characterized in detail as case studies of this phenomenon. We suggest that the nightside gap may be due to a significant reduction in field-aligned currents along with an insufficient ionospheric potential to accelerate precipitating electrons within the gap region, perhaps associated with the Harang discontinuity.

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