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Published byAlyson Florence Harrington Modified over 8 years ago
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1 Joachim Birn LANL Karl Schindler Ruhr-Univ. Bochum Michael Hesse NASA/GSFC Thin Electron Current Sheets and Auroral Arcs Relationship between magnetospheric features and auroral electric fields and currents: role of flows, currents, electric potentials
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2 Auroral arc brightening Electron precipitation, Acceleration by E || J || Shear flow, for small scales carried by electron Hall current U shaped potential upward field-aligned current
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3 Relation between auroral arcs and shear flow j Hall
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4 x = -4x = 0 Vlasov model for thin embedded current sheet current in thin sheet carried by ExB drifting electrons pressure dominated by ions el. stat. potential
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5 Relation between thin current sheet and auroral arc current in thin sheet carried by eastward ExB drifting electrons rapid thinning provides Alfvenic pulse with field-aligned currents may lead to quasi-steady potential pattern
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6 thin current sheets dominated by electron flow (eastward ExB drift) but pressure dominated by ions potentials up to fraction of kT i /e bifurcation of current earthward of thin sheet double current sheet possible onset from rapid thinning in late growth phase or initial reconnection Alfvenic pulse with firl-aligned currents may lead to persisting potential precedes fast flow and dipolarization Summary: electron current sheets & arcs
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8 Vlasov equilibrium approach
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9 x = -4x = 0 Vlasov model for thin embedded current sheet
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10 Double electron current sheet
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11 2 min 4 min 6 min 8 min (300 km/s) (-200 km/s) Bubble propagation velocity v x depleted flux tube (reduced pressure or flux tube volume, entropy: pV ) Earthward motion from buoyancy, interchange (Pontius & Wolf, Chen & Wolf) Association with bursty bulk flows? (Sergeev et al.)
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12 twisted or sheared magnetic field field-aligned current flow Macro-scale field-aligned current generation Field-aligned currents at x = -1 Obs.: Nakamura et al.
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13 2 min 4 min 6 min 8 min 2 min 4 min 6 min 8 min pressure changevelocity v x
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14 2 min 4 min 6 min 8 min 2 min 4 min 6 min 8 min cross-tail current densitypressure change
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15 Relation between tail flows (“bubbles”), thin current sheets, and auroral arcs Earthward moving bubble Current layers
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16 Large scales: - ion & electron vorticity, shear flow (E B drift) field-aligned currents E E || Small scales: - perp. currents from enhanced p, reduced B - Hall current sheets electron E B drift E - closure of converging E E || U-shaped potentials - electron shear flow, vorticity field-aligned currents Summary: Bubble/BBF effects Summary: electron current sheets - current dominated by electrons - pressure dominated by ions - potentials up to fraction of kT i /e - bifurcation of current possible - double current sheet possible, cannot extend to z=0 inside plasma sheet
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