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CMSO Workshop on Flow Driven Instabilities and Turbulence in High Beta Plasmas
 


Astrophysical Background:

Charge: Review of the physical process and where topic is important in Astrophysics. What parameter regimes and/or geometry are necessary to learn something important? What needs to be measured?

Experimental or Numerical Modeling Scenario:

Charge: Conceptual design of plasma experiment (in MPDX or otherwise) and feasibility. Hardware implementation, geometry, and required plasma parameters. What can be measured?

Speakers

Day I - Tue. Dec 15 
8:30-9:15Welcome and IntroductionCary Forest

9:15-10:00MHD Dynamos Stas Boldyrev
From a pure MHD standpoint, how do we optimize the experiment for studying outstanding questions in dynamos? What flow topologies are optimal? Can time dependent (Galloway Proctor flows) be devised in a sphere? How does compressibility and/or high Pm possible in plasma change outlook.

10:00-10:30Break 

10:30-11:30Plasma Dynamos Steve Cowley
Where and when do two fluid or kinetic effects become important in astrophysical dynamos? What parameter regime and geometry is optimal for studying this in experiment? Hall effects; firehose, mirror

11:30-12:15DiscussionHantao Ji

12:15-1:30Lunch (provided) 

1:30-3:30Plasma MRIGreg Hammett (45 min)
Hantao Ji (30 min)
Cami Collins (15 min)
Fatima Ebrahami+Ivan Khalzov (30 min)
Standard MRI flow; what will Hall (both MHD and neutral collisions) effects, anisotropic pressure and collisionless MRI look like. What do we need to diagnose it.

3:30-4:00Break 

4:00-5:00Rotating Convection:Ben Brown
compressibility and stratification
Compositional/temperature/magnetic buoyancy driven instabilities in stratified, rotating plasmas; ECH applied to boundary provides heating and buoyancy; Role of Reynolds stress on rotation profile; stratification; Magnetic buoyancy

5:00-6:00Discussion Fausto Cattaneo

7:00-9:30Group Dinner 
   
Day II - Wed. Dec 16 
8:30-9:15Plasma Turbulence at High Beta
Troy Carter
See MRI and Plasma Dynamos; Self-excitation not critical; chaotic stirring is. Turbulence in near equipartition. Ion heating. Inertial range; transition from unmagnetized to magnetized (anisotropy)   

9:15-10:00Jets and DisksJohn Everett
Plasma Gun array injecting into high beta plasma; equilibrium, loss of equilibrium, collimation; focus on steady state aspects and role of external plasma pressure

10:00-10:30Break 

10:30-11:15Comic Ray Acceleration by Plasma TurbulenceKen Fowler 

11:15-11:45Flow driven reconnectionBarrett Rogers
2D Reconnection of multipolar magnetic fields in spherical source, with fields that drop off outward. Rotating plasma wind tunnel impinging on a dipole.

11:45-12:15A review of Terrella experiments investigating the Solar Wind/Magnetosphere interactionMark Koepke

12:30-12:45  DiscussionTroy Carter

12:45-1:45Lunch (provided) 

1:45-2:30Pulsar Winds and ShocksJonathan Arons
Concept: rotating dipole built into source in center in center of sphere, spewing off magnetic fields of alternating polarity; as density drops off, Alfvén velocity approaches speed of light. Heliospheric, sectored structure of heliosphere solar wind. Anomalous Cosmic Rays from Fermi accelleration from reconnection(Drake).

2:30-3:15Partially Ionized MHDEllen Zweibel
In what parameter regime should we be concerned with neutral particles in MHD? How does this differ from Hall MHD?

3:15-3:45Break

3:45-4:15SkunkworksCary Forest

4:15-6:00DiscussionEllen Zweibel
 


DAY III: MPDX Design Review - Thurs. Dec 17 
 Panel: Troy Carter, Fred Skiff, Mike Brown, Dave Anderson, Peter Titus
9:00-9:30OverviewCary Forest
Facility, Infrastructure, time line

9:30-10:15Vessel, Magnets, and CoolingJohn Wallace
Primary issues related to assembly of high field magnets, internal water cooling, insulating plasma facing components

10:15-10:45Break 

10:45-11:15LaB6 Plasma SourceTroy Carter
Large Area, spherical, plasma source (review of similar sources elsewhere, and design of spherical source)

11:15-11:30Data Acquisition and ControlAlex Squitieri
GA PCS, DTAQ, RealTime MDSPlus, Power supplies (review similar systems in use on MST, and give overview of how this will be implemented on experiment).

11:30-12:00Programmable Power SuppliesDon Holly

12:00-1:00Diagnostic OverviewWeiging Ding
Port layout, access. Probes, Faraday Rotation/Interferometry, Gas Puff imaging using fast camera, CXRS for flow, external magnetics, LIF, Brainstorming

1:00-1:30Working Lunch (provided) 

1:30-3:00Discussion 

3:30Adjourn 



A National Science Foundation Physics Frontier Center,
established in coordination with the Department of Energy.

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