How Well Can We Estimate Pedersen Conductance From the THEMIS White-Light All-Sky Cameras?

摘要

We show that a white-light all-sky imager can estimate Pedersen conductance with an uncertainty of 3 mho or 40%. Using a series of case studies over a wide range of geomagnetic activity, we compare estimates of Pedersen conductance from the backscatter spectrum of the Poker Flat Incoherent Scatter Radar with auroral intensities. We limit this comparison to an area bounding the radar measurements and within a limited area close to (but off) imager zenith. We confirm a linear relationship between conductance and the square root of auroral intensity predicted from a simple theoretical approximation. Hence, we extend a previous empirical result found for green-line emissions to the case of white-light off-zenith emissions. The difference between the radar conductance and the best-fit relationship has a mean of -0.76 ± 4.8 mho and a relative mean difference of 21% ± 78%. The uncertainties are reducedto-0.72±3.3mhoand0%±40%byaveraging conductance over 10 min,whichweattribute to the time that auroral features take to move across the imager field being greater than the 1-min resolution of the radar data. Our results demonstrate and calibrate the use of Time History of Events and Macroscale Interactions during Substorms all-sky imagers for estimating Pedersen conductance. This technique allows the extension of estimates of Pedersen conductance from Incoherent Scatter Radars to derive continental-scale estimates on scales of ~1-10 min and ~100 km~2. It thus complements estimates from low-altitude satellites, satellite auroral imagers, and ground-based magnetometers.