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Magnetotail Current Sheet IKI 26-30 September 2011 Magnetic Reconnection in the Current Sheet: Geotail Observations Wednesday 28 September 2011, 1220-1300 T. Nagai Tokyo Institute of Technology. The basic physical components on the magnetic reconnection site
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Magnetotail Current Sheet IKI 26-30 September 2011 Magnetic Reconnection in the Current Sheet: Geotail Observations Wednesday 28 September 2011, 1220-1300 T. Nagai Tokyo Institute of Technology
The basic physical components on the magnetic reconnection site • The central electron current layer – the (electron) diffusion region • The ion-electron decoupling region – the Hall physics region • Inflows and Outflows – the MHD region
MHD Picture of Magnetic Reconnection inflow outflow Bz > 0 Bz < 0
Particle Picture of Magnetic Reconnection Ion flows Electron flows unit ViA unit VeA
Outflows Ve Ve Vi Vi Bz > 0Bz < 0 MHD Ion-electron decoupling MHD
electron current layer - Vey Bz > 0Bz < 0
The basic physical components on the magnetic reconnection site • The central electron current layer – the (electron) diffusion region • The ion-electron decoupling region – the Hall physics region • Inflows and Outflows – the MHD region
electron Vx ion Vx ion Vy electron Vy
electron Vx ion Vx ion Vy electron Vy electron Vperp x electron Vperp y 2 10 nA/m
ion Vx ion Vy electron Vx electron Vy
electron Vx electron Vy electron Vperp x electron Vperp y 2 20 nA/m
electron Vx ion Vx ion Vy electron Vy
Geotail Observations in the Plasma Sheet (plasma b > 1) in 1994-2010 X = -18 to -30 RE Y = -20 to +20 RE
MHD flows Vi = Ve Errors are small when energetic electrons are rich. electron Vx ion Vx electron Vy ion Vy
Physical Size of the Magnetic Reconnection Site in the X direction in the Y direction ?
15 May 2003 near 1055 UT the spacecraft Geotail at 28 RE in situ observations of magnetic reconnection Geotail
Bz < 0 Bz > 0 Earthward flows Bz > 0Bz < 0 Tailward flows Ion Et Earthward flows Tailward flows
Main Targets of This Paper • Detect the central intense electron current layer • Get scales of magnetic reconnection • with Geotail observations • VA = 2,200 km/s • li = 1,200 km (ion inertial length) • Geotail MGF 16 vectors /s • LEP 12 s • electron g-factor 4x10 • DT 5.5x10 -4 -3
Bz < 0 Bz > 0 Earthward flows 5 minutes Bz > 0Bz < 0 Tailward flows Ion Et Earthward flows Tailward flows
Ion observations Bz > 0Bz < 0 Bz < 0 Bz > 0 Earthward flows 1000 km/s ion flow VA = 2200 km/s Tailward flows
Ion flows vs. electron flows Ion Et Bz > 0Bz < 0 Bz < 0 Bz > 0 Vi Vx > 3000 km/s electron flows Vy > 6000 km/s electron flows Ve Ve
Ion and electron flows perpendicular to the magnetic field Bz > 0Bz < 0 Bz < 0 Bz > 0 V Earthward flows Vx > 2000 km/s electron flows Vy > 3000 km/s electron flows Ve Tailward flows Ve
Electron observations acceleration and heating electron Et Bz > 0Bz < 0 Bz < 0 Bz > 0 V Vx > 2000 km/s electron flows Vy > 3000 km/s electron flows Ve Ve
Bz > 0Bz < 0 Earthward flows Tailward flows 1057:44 1053:44 UT time Earth tail Bz > 0Bz < 0 > 8.47 keV electron directional fluxes
Bz > 0Bz < 0 Earthward flows Tailward flows 1057:44 1053:44 UT time Earth tail Bz > 0Bz < 0 electron velocity distribution function In the equatorial plane Vy < 0 dawnward Vy > 0 duskward
Bz > 0Bz < 0 Earthward flows Tailward flows 1057:44 1053:44 UT time Earth tail Bz > 0Bz < 0 electron velocity distribution function Hall electrons
Bz > 0Bz < 0 Earthward flows Tailward flows 1057:44 1053:44 UT time Earth tail Bz > 0Bz < 0 ion velocity distribution functions
Bz > 0Bz < 0 Earthward flows Tailward flows time Bz > 0Bz < 0
Bz > 0Bz < 0 Earthward flows Tailward flows time counter-streaming inflows Bz > 0Bz < 0 ion velocity distribution functions
Important Questions ion-electron decoupling Ve >> Vi MHD MHD large Vey 1057:44 1053:44 UT intense electron current layer spatial scales?
Asymmetric outflows MHD flows +450 km/s -650 km/s Earthward flow speed tailward flow speed
MHD flows +550 km/s -550 km/s (+450 km/s) (-650 km/s) -100 km/s tailward velocity of reconnection site
Bz > 0Bz < 0 Earthward flows Tailward flows time counter-streaming inflows Bz > 0Bz < 0 ion velocity distribution functions
Asymmetric inflows inflows Vx = +64 km/s Vx= -269 km/s
inflows Cluster results -100 km/s Baker et al. 2002 Imada et al. 2007 Vx = +164 km/s Vx= -169 km/s (+264 km/s -269 km/s) -100 km/s tailward velocity of reconnection site
ion-electron decoupling region MHD MHD 1 li Earth tail central electron current layer 8 li Vx peak Flux peak Ion ele ele ion 8 li = 1.5 RE 1 li = 1200 km
the X-line position PIC simulation results the northern earthward side of the reconnection site (upper-left quadrant)
observation simulation at TΩi = 35 Vix / Vex 0.2-0.3 0.1 Vey / Vex 1.25 1.4 Vix 0.5 VA 0.3 VA the full extent of the central 1 li 1 li electron current layer the full extent of 8 li 8 li the ion-electron decoupling region
8 li = 1.5 RE ion-electron decoupling region Geotail Survey of Tailward Flows with Bz < 0 in 1995-2003 209 events Nagai et al., 2005
Geotail Reconnection Events = Observations of Ion-Electron Decoupling Region 34 events 34/208 = 0.16 reconnection events at 20-30 RE Nagai et al., 1998; 2001