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Published byMagdalene Caroline Phelps Modified over 8 years ago
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MHD Simulations of magnetotail reconnection (J. Birn) Observations MHD simulation: overview Propagation of dipolarization signals Generation of pulsations: bouncing, “breathing” Field-aligned current generation Role of entropy reduction Ackn.: Thanks to M. Henderson, M. Hesse, R. Nakamura, E. Panov Focus on “bursty bulk flows” and “dipolarization”
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Observations of flow bursts and “dipolarization fronts” Sergeev et al., 1996 North Sun Dusk Sergeev et al., 2010 time field-aligned currents auroral streamer
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Observations of flow bursts and dipolarization fronts Runov et al., 2009 Nakamura et al., 2009
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Observations of flow bursts: bouncing and vorticity Panov et al., 2010 Ohtani et al., 2009
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flow bursts = depleted flux tubes (“bubbles”)? reduced S from reconnection (Fig. after Forsyth et al., 2008) Kim et al., 2010 Pontius & Wolf, 1990: reduced “entropy” or slippage? ( Wolf et al., 2009)
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Schindler, Birn Voigt Lee&Wolf
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MHD Simulations: Overview (Static equilibrium: p = j B) 1. INITIAL (GROWTH) PHASE: SPATIALLY AND TEMPORALLY LIMITED INFLOW, COMPRESSION, THIN CURRENT SHEET FORMATION 2. DYNAMIC (EXPANSIVE) PHASE: ANOM. RESISTIVITY CAUSES RECONNECTION, PLASMOID EJECTION 3. ENERGETIC PARTICLES: TEST PARTICLES IN MHD FIELDS Time-dependent simulations: Initial State addition of dipole, + relaxation into equilibrium Initial Phase
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Pre-onset phase: Adiabatic deformation thin current sheet formation, loss of equilibrium y 2-D quasi-static theory 3-D MHD simulation JyJy JyJy x x y z
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3D MHD Simulation of Tail Reconnection
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Magnetic Field B z in the x,z plane z x 0-2-4-6-8-10-12 B z (x,z)
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Electric Field E y in the x,z plane z x
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Electric Field E y and velocity in the x,y plane y x E y (x,y)
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Local characteristics as function of x
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3D MHD Simulations & Observations THEMIS observations (Panov et al., 2010) MHD simulations (Birn et al., 2011) Bouncing, pulsating, dipolarization sequences
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Field-aligned current generation t = 128 t = 132 (equilibrium) -120 0 -6-6 6 y -6-6 6 y
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Onset Timing E y at x-point J || at x = 0 integrated J || (region 1) max. J || t = 61: finite resistivity t = 90: neutral line formation t = 120: onset of fast reconnection
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Onset of fast reconnection
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Entropy function in the x,y plane -15 -10 -5 0 x y -10 -5 B z contours 5 1010
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Comparison 2D vs. 3D, enthalpy flux H x = 2.5pv x 2D3D
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Comparison 2D vs. 3D
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y x Test particle simulations (electrons) α = 35° at x=1.5, y=0,z=0
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Test particle simulations (electrons) pitch angle averaged passage of dipolarization front x = 3, y = 0, z = 0
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Summary: MHD Simulations of Tail Reconnection Reconnection enables ballooning/interchange Ballooning enables - fast reconnection, significant energy release - cross-tail structure, leading to Fast flows and dipolarization fronts - propagating earthward - stopping & tailward expansion - bouncing, vorticity, & breathing - field-aligned currents Localized electric field accelerates particles
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