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Found 3 entries in the Bibliography.
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OVATION Prime-2013: Extension of auroral precipitation model to higher disturbance levels
OVATION Prime (OP) is an auroral precipitation model parameterized by solar wind driving. Distinguishing features of the model include an optimized solar wind-magnetosphere coupling function (dΦMP/dt) which predicts auroral power significantly better than\ Kpor other traditional parameters, the separation of aurora into categories (diffuse aurora, monoenergetic, broadband, and ion), the inclusion of seasonal variations, and separate parameter fits for each magnetic latitude (MLA ...
Newell, P.; Liou, K.; Zhang, Y.; Sotirelis, T.; Paxton, L.; Mitchell, E.;
Published by: Space Weather Published on: Jan-06-2014
YEAR: 2014   DOI: 10.1002/swe.v12.610.1002/2014SW001056
Local Geomagnetic Indices and the Prediction of Auroral Power
The aurora has been related to magnetometer observations for centuries, and to geomagnetic indices for decades. As the number of stations and data processing power increases, just how auroral power (AP) relates to geomagnetic observations becomes a more tractable question. This paper compares Polar UVI AP observations during 1997 with a variety of indices. Local time (LT) versions of the SuperMAG auroral electrojet (SME) are introduced and examined, along with the corresponding upper and lower envelopes (SMU< ...
Published by: Journal of Geophysical Research: Space Physics Published on: 11/2014
YEAR: 2014   DOI: 10.1002/2014JA020524
Aurora; indices; auroral electrojet; Pedersen current; prediction
Does the polar cap disappear under an extended strong northward IMF?
Zhang, Yongliang; Paxton, Larry; Newell, Patrick; Meng, Ching-I.;
Published by: Journal of Atmospheric and Solar-Terrestrial Physics Published on: Jan-12-2009
YEAR: 2009   DOI: 10.1016/j.jastp.2009.09.005