THEMIS SWG, Annapolis, Sept. 14, 2011 Supported by NSF grant #

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Presentation transcript:

THEMIS SWG, Annapolis, Sept. 14, 2011 Supported by NSF grant # 1044495 THEMIS observations of mid-tail reconnection and dipolarization fronts A. Runov, X.Z. Zhou, V. Angelopoulos IGPP/ESS UCLA Supported by NSF grant # 1044495

Transient Magnetotial RX Scenario 1: DF is a consequence of transient reconnection (RX) in the mid-magnetotail. Timing between RX and DF should be consistent with reconnection outflow velocity. Ballooning/interchange may lead to azimuthal structuring and further steepening of the front (M.Nakamura et al., 2002; Pritchett & Coroniti, 2010). Scenario 2: DF appears as a consequence of local thinning (min Bz) of the magnetotail plasma sheet leading to ballooning (e.g., Zhu et al., 2009, Pritchett & Coroniti, 2010, Birn et al, 2011) or “melon seed” (Sitnov et al., 2011, submitted) instability prior to fast mid-tail reconnection. RX itself is complex process, including “slow” and “fast” phases. THEMIS major conjunction events with signatures of RX and DF Timing of RX and DF 2008-02-26 Angelopoulos et al., Science, 2008 2009-02-07 Oka et al. GRL submitted 2008-03-01 – this work Transient Magnetotial RX and DF Formation Transient RX, Semenov et al., 1984 Bz E* Kiehas et al., 2009 PIC simulations of TRX, Sitnov et al, 2009

08-03-01/02:15:00 (Kp = 5+) Bz Vz 0214 UT MHD simulations discrete IONOSPHERE discrete diffuse El-Alaoui et al., JGR, 2009

P3, P4 P1: TW flow with Bz<0 (RX) P2: Bx oscillations @ PS; RX PS  PSBL; Vz > 0 P3,P4: decrease in Bz indicates CS stretching, Duskward/Earthward flow: CS thinning; Dipolarization front (DF) Opposite flows at P3 and P4 behind DF. Timing: P4  P3 G-10,-12: jump in Bz (DF); |Be| < 5 nT prior to DF; anti-correlation in Bz behind the front. Timing: G10  G12 RX ?? DF 0214 P3, P4

Timing: Cumulative Flux Transfer 3D MHD simulations of RX in the magnetotail Φ=-∫[V x B]y dt J.Liu et al., JGR, 2011 Birn et al, JGR, 2011 2-step process: “slow” regime  “fast” (or “burst”) regime P2: “Slow” FT 0210 UT, “Fast” FT 0214:45 UT P1: “Fast” FT 0215:08, P4: DF 0215:06 Timing: DF was formed before fast regime start at P2

P2 Observations at Cumulative Flux Transport Onset (0210UT) Bx oscillations Positive-negative E-field variations Mainly northward ion Vx after 0210 UT Decrease in HEi+ and increase in HE e- fluxes during “plus” intervals Increase-decrease in i+ and e- NS flux MVA normal vectors Rapid current sheet flapping: surface waves (ripples) on the current sheet

Reconstruction of Flapping Current Sheet Structure Vdz=EyBx/B S=∫Vdz dt Flapping: a set of folds on CS Flapping amplitude ~1000 km Embedded TCS with H~400 km (~c/ωpi) Local jy max at the CS periphery “Triple-peak” structure in the center (?)

P3/P4 & GOES 10/12 Observations in the near-Earth PS THM P3/4 – GOES 10/12 timing: earthward propagation of the front P3 – P4 timing: -6 s G10-G12 timing: 25 s G10 Be = 66 nT G12 Be = 51 nT P3/4 & G10/12 timing: non-planar front and earthward-dawnward propagation Bulk flow in XY plane: opposite direction at P3 (duskward) and P4 (mainly dawnward) behind the front Vortex motion or gradP-drift? G10 G12 P3 P4 Similar results in simulations: Birn et al., 2011, Merkin et al., (submitted)

P3 & P4 Observations

Summary & Open Questions Midtail: Signatures ofreconnection (Vx<0 & Bz<0) at X≈-22 RE; Near PS: Earthward-moving dipolarization front between X≈-10 & -5 RE; Activity started at X≈-16 RE gradual increase in the magnetic flux transfer rate (Φ); In ~5 min  burst-like enhancement in Φ; Flapping waves on CS surface with amplitude of 1000 km Non-Harris CS structure: embedded TCS (tripple-peak?) in the center & a peak at the perephery Dipolarization front in the Near-Earth PS: Appeared in ~5 minutes after the initial flux transfer increase; Simultaneously ( within 0.5 min) with fast flux transfer onset => appeared on slow phase  Scenario 2 seems possible. Earthward and dawnward propagation of the dipolarization front; Non-planarity of the front; Vortical bulk flow behind/around the front (?) Difference in filed and particle signatures at two points separated by <1 RE in Y RX & Flapping (kinking): what drives what? What does flapping CS structure tell us about RX? Comprehensive 3D modeling is needed. What are mechanisms of front formation on “slow” RX phase? Is ballooning in a play? Comprehensive 3D modeling is needed.

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Flapping model: TCS “double-gradient” instability Erkaev et al., JGR, 2009