scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...
scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...
scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...
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STP12 Abstracts<br />
Berlin, 12 - 16 July <strong>2010</strong><br />
SCOSTEP Symposium <strong>2010</strong><br />
High Latitude Thermal Cells Induced by Ion Drag Driven Gyres<br />
Walterscheid Richard 1 , Crowley Geoff 2<br />
1 The Aerospace Corporation, 2 ASTRA<br />
Un<strong>der</strong> typical conditions, the ions driven into motion by the high latitude electric field<br />
generates a pair of counter-rotating <strong>an</strong>ticyclonic <strong>an</strong>d cyclonic gyres in the neutral wind<br />
circulation. When viscous <strong>an</strong>d ion-drag forces are not too strong dynamical adjustment of the<br />
atmosphere acts to bring the winds into <strong>an</strong> approximate gradient wind bal<strong>an</strong>ce between the<br />
inertial forces (Coriolis <strong>an</strong>d centrifugal) <strong>an</strong>d the pressure gradient. These forces act in the<br />
same direction for cyclonic gyres <strong>an</strong>d in the opposite direction for <strong>an</strong>ticyclonic gyres. When<br />
the flow is not too strong or too curved the Coriolis force is domin<strong>an</strong>t <strong>an</strong>d dynamical<br />
adjustment gives a pair of high (warm) <strong>an</strong>d low (cold) pressure cells, associated respectively<br />
with the <strong>an</strong>ticyclonic <strong>an</strong>d cyclonic gyres. However, when the flow is sufficiently rapid the<br />
centrifugal force dominates <strong>an</strong>d both gyres give relatively cold low pressure cells. The<br />
thermal ch<strong>an</strong>ges induced by dynamics are adiabatic <strong>an</strong>d are in addition to the ch<strong>an</strong>ges induced<br />
by the diabatic heat sources.<br />
We have examined the bal<strong>an</strong>ce of forces with a 3-D general circulation model of the upper<br />
atmosphere (TIME-GCM). We infer the bal<strong>an</strong>ce of forces normal to the motion (centrifugal,<br />
Coriolis <strong>an</strong>d pressure gradient) forces. We have examined the bal<strong>an</strong>ce of forces <strong>an</strong>d the<br />
pressure <strong>an</strong>d thermal response to these forces during quiet <strong>an</strong>d active times.<br />
The quiet-time structure is radically ch<strong>an</strong>ged when the atmosphere is spun up into rapid<br />
motion during active periods. During active periods structures form that are more<br />
complicated th<strong>an</strong> the structure of the forcing itself. Centers of relative low density air are<br />
found on both the dawn <strong>an</strong>d dusk sides with a trough of low density air over the pole<br />
connecting them. The intrusion of low density air over the pole splits the region of high<br />
density air that exists un<strong>der</strong> quiet conditions giving two high density centers, one toward the<br />
midnight side <strong>an</strong>d other toward the noon side. This gives the four cell pattern simulated by<br />
Crowley et al., 1989, 1996. We find that this structure evolves when the flow is too rapid to<br />
sustain the quiet-time warm high-pressure <strong>an</strong>ticyclonic cells.<br />
Crowley, G., B. A. Emery, R. G. Roble, H. C. Carlson, <strong>an</strong>d D. J. Knipp (1989),<br />
Thermospheric dynamics during September 18 – 19, 1984: 1. Model simulations, J. Geophys.<br />
Res., 94, 16,925– 16,944.<br />
Crowley, G., J. Schoendorf, R. G. Roble, <strong>an</strong>d F. A. Marcos (1996), Cellular structures in the<br />
high-latitude thermosphere, J. Geophys. Res., 101, 211–223, doi:10.1029/95JA02584.