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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-4903
DTSTART:20180924T170500Z
DURATION:PT1H0M0S
DTSTAMP:20260305T173058Z
LAST-MODIFIED:20180913T213449Z
LOCATION:2241 Chamberlin hall
SUMMARY:Reconnection in Realistic Astrophysical Settings: Turbulent  F
 luids and Partially Ionized Gas\, Plasma Physics (Physics/ECE/NE 922) 
 Seminar\, Alex Lazarian
DESCRIPTION:I shall explain why turbulent reconnection is the most nat
 ural setting for the astrophysical reconnection. The turbulence can be
  pre-existing<br>
\nor induced by the reconnection itself. I shall pro
 vide a comparison of the domains of the applicability of the turbulent
  and tearing reconnection.<br>
\nFinally\, I shall discuss how partial
  ionization modifies the turbulent reconnection and consider the conse
 quences of the reconnection in partially<br>
\nionized astrophysical e
 nvironments.
URL:https://www.physics.wisc.edu/events/?id=4903
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