PPT-A multi-spacecraft analysis of energy transfer associated with near-Earth magnetic reconnection

S Fadanelli B Lavraud F Califano We present an analysis of energy transfers in a reconnecting nearEarth plasma obtained by interpreting MMS data within the framework of multifluid plasma theory In our analysis energy transfers are calculated and examined locally This way correlations between different mechanisms of energy exchange can be retrieved in all spatial and temporal detail provided by the highfrequency multipoint sampling capacity of the four MMS satellites . 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. 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 . 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. 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 . Dr Mark Price . (. mcp2@star.kent.ac.uk. ) , . Prof Mark Burchell (convener), Prof Richard Holdaway (CCLRC), Dr Vicky Fitzgerald.. Spring 2011.. Dr. Mark Price. Room 103C . E-mail: . mcp2@star.kent.ac.uk. Magnetic reconnection occurs throughout the Universe Magnetopause Reconnection: The Interplanetary Magnetic Field (IMF) reconnects with the Earth䇲s magnetic field, at the magnetopause (the oute 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?. Technology Report. Nicole Iwaki. ITMG 100 05. What is the Cassini Spacecraft?. O. ngoing project by the National Aeronautics and Space Administration. Launch date on October 15th, 1997. It’s mission is to conduct detailed studies of Saturn, its rings, icy satellites, magnetosphere and Titan.. 2. What controls the degree of plasma heating in reconnection?. => Plasma . b. and . Alfvén. speed. Tai Phan (UC Berkeley). Contributors: J. Drake, J. Gosling, M. Shay, M. . 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. Rendevous. using CNN. Ryan McKennon-Kelly. Sharma, . Sumant. , Connor . Beierle. , and Simone D’Amico. “Pose Estimation for Non-Cooperative Spacecraft Rendezvous Using Convolutional Neural Networks,” September 19, 2018. . Magnetic . Energy. . once an ancient mystery, is now recognized as the strongest natural force in the universe. . . Our Earth. . is a giant magnet and all life developed under the influence of the earth’s magnetic field. . the Earth's magnetic field at a given location. Objetive. The . objective of the activity is to measure the magnetic field of the Earth . an . a given . area. The relation . between . maximum . and minimum .