PPT-1. What controls the occurrence of reconnection?

Author : lindy-dunigan | Published Date : 2017-06-06

2 What controls the degree of plasma heating in reconnection gt Plasma b and Alfvén speed Tai Phan UC Berkeley Contributors J Drake J Gosling M Shay M

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1. What controls the occurrence of reconnection?: Transcript

2 What controls the degree of plasma heating in reconnection gt Plasma b and Alfvén speed Tai Phan UC Berkeley Contributors J Drake J Gosling M Shay M . Alex Flanagan (University of Wisconsin). J. F. Drake (UMD), M. Swisdak (UMD). Magnetic Reconnection?. Magnetic energy converted to kinetic . and thermal energy. Occurs in solar corona, magnetosphere, laboratory plasma experiments, and even at edge of solar system. A.C. Foster. 1. , C.J. Owen. 1. , A.N. Fazakerley. 1. , I. J. Rae. 1. , C. Forsyth. 1. , E. Lucek. 2. , H. Rème. 3. UCL, . Mullard. Space Science Laboratory, Surrey, UK. Imperial College, London, UK. 13th May 2005 Solar Flare. William M.R. Simpson, Angela Des . Jardins. University of St. Andrews, Montana State University. Contact. :. Email:. www. : . William M. R. Simpson. wmrs2@st-and.ac.uk. http://solar.physics.montana.edu/home/www/REU/2009/wsimpson . . . ReConnect. by. . . ensures accurate payments with the same ‘accept and reject’ safeguards . as our existing payment options. by Brian Welsch,. JSPS Fellow (Short-Term. ),. Space Sciences Lab, UC-Berkeley,. Non-Expert on Reconnection. Image by . Pevtsov. & Groening 2010. What can helicity redistribution in solar eruptions tell us about reconnection in these events?. in solar eruptions tell . us about . reconnection in these events?. by Brian Welsch,. JSPS Fellow (Short-Term. ),. Space Sciences Lab,. UC. -. Berkeley,. Non-. Expert on Reconnection. Image by . Pevtsov. A.C. Foster. 1. , C.J. Owen. 1. , A.N. Fazakerley. 1. , . C. Forsyth. 1. E. Lucek. 2. , H. Rème. 3. UCL, . Mullard. Space Science Laboratory, Surrey, UK. Imperial College, London, UK. CNRS, IRAP, Toulouse, France. Understanding . 3D . Magnetic Reconnection . in . Observations . and S. imulations. Session organizers:. Peter Wyper (NASA Goddard Space Flight Center/Oak Ridge Associated Universities). Silvina. . Guidoni. Daniel Gordon. Supervisor: Dana . Longcope. Simulating Shocks in Solar Flares:. Presentation Outline . Introduction. Background. The model. Previous results (single reconnection event). The multiple reconnection case . Daniel Gordon. Adviser: Dana . Longcope. Introduction. Magnetic reconnection is a significant mechanism for phenomenon involving high energy release such as solar flares.. Post-reconnection field lines act like elastic bands under tension.. Mass Transport (Acceleration?). J. Arons. UC Berkeley. Question: How Does Return Current in PSR Magnetosphere Form?. . What is density of current carriers?. Consequences (many): How do beamed gamma rays get emitted?. reconnection. and . jets . in the lower atmosphere. Hiroaki . Isobe. (Kyoto . Univ. ). collaborators: . K.A.P. Singh, K. Shibata (Kyoto U). V. . Krishan. (Indian Inst. . Astrophys. . Bangalore). Reconnection + plasma jets at various heights. Substorms. 2. 5-29 September 2017. Portsmouth, New Hampshire, USA. . Double Magnetic Reconnection Driven by Kelvin-Helmholtz . Vortices. W. . Horton. 1. , M. Faganello. 2. , F. . Pegoraro. 2. F.Califano. Alex Flanagan (University of Wisconsin). J. F. Drake (UMD), M. Swisdak (UMD). Magnetic Reconnection?. Magnetic energy converted to kinetic . and thermal energy. Occurs in solar corona, magnetosphere, laboratory plasma experiments, and even at edge of solar system.

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