[IGPP Everyone] TOMORROW: Space Physics Seminar, Friday June 5th- Spontaneous Reconnection Onset in the Magnetotail: Wagging the Dog (M.I. Sitnov, JHU APL)

Thu Aug 6 14:39:12 PDT 2015

Hi Marco, 

Sorry, was in a bad accident on Tuesday, car totaled, out till Tuesday. You'll need to specify the room and time, please go ahead. ;) 

-E 

P.S. did you sort out everything with your conference with Gloria? Assuming you won't need me until afterwards, but best clear the payment issues with her just to be sure it's all in place so no UC funny business. Good luck. 

TO: everyone at epss.ucla.edu; everyone at igpp.ucla.edu 
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SPACE PHYSICS SEMINAR 

DEPARTMENT OF EARTH, PLANETARY, AND SPACE SCIENCES 

DEPARTMENT OF ATMOSPHERIC AND OCEANIC SCIENCES 

UNIVERSITY OF CALIFORNIA, LOS ANGELES 

(EPSS M288A, AOS M275A ) 

Mikhail I. Sitnov 

JHU APL 

Spontaneous Reconnection Onset in the Magnetotail: Wagging the Dog 

Bursty reconnection in the Earth¹s magnetotail has important features that distinguish it from similar processes in other space plasma regions and the simplest theoretical models. First, its possibility has long been questioned because of the stabilizing effect of electrons magnetized by the north-south (Bz) magnetic field component. Second, reconnection in the tail competes with non-reconnection ballooning/interchange and flapping motions. Third, it is distinguished by the so-called dipolarization fronts, kinetic-scale shock-like plasma structures which dominate the energy conversion. We discuss the kinetic and MHD theory of the magnetotail reconnection onset to identify the equilibria for which the spontaneous reconnection is possible. It shows that a necessary condition for the reconnection onset is a tailward gradient of the Bz field, which is indeed observed in the late substorm growth phase. 3D PIC simulations show that, when such an instability develops, it starts from the generation of an earthward plasma bulk flow with a dipolarization front at its leading edge and is followed by a magnetic topology change. These processes are accompanied by interchange and flapping motions that result in structuring of the tail activity in the local time but do not destroy the global reconnection-dominated picture. Simulations show that, in contrast to simple models, the energy conversion in the tail is largely provided by dipolarization fronts and the corresponding ion and electron temperature increases are consistent with THEMIS observations. We discuss virtual satellite observations, which reveal the potential of the MMS observations in resolving the primary plasma modes associated with the magnetotail reconnection. We also discuss the role of the dipole magnetic field in the tail structure and dynamics. 

. 

Friday, June 5, 2015 

Room 6704 Geology 

3:30 - 5:00 PM 

Refreshments served after the seminar in Room 6850. 

In-Charge 
M. Velli 

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