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DTSTART:19960101T000000 END:STANDARD BEGIN:STANDARD TZNAME:GMT TZOFFSETFROM:+0100 TZOFFSETTO:+0000 DTSTART:19961027T020000 RRULE:FREQ=YEARLY;BYMONTH=10;BYDAY=-1SU END:STANDARD END:VTIMEZONE BEGIN:VEVENT DTSTAMP:20260428T003054Z DTSTART;VALUE=DATE-TIME:20100125T150000 DTEND;VALUE=DATE-TIME:20100125T170000 SUMMARY:Dr Mark Dieckmann\, Linkoping University TZID:Europe/London UID:20100125-094d43f62568a3c7012568c2c6aa05ea@warwick.ac.uk CREATED:20091207T105013Z DESCRIPTION:Title: Asymmetric collision of plasma clouds in the presence of a quasi-parallel guiding magnetic field: Electron acceleration to ult rarelativistic speeds and magnetic field amplification to energy equipar tition with the ions. Abstract: Plasma processes close to SNR shocks res ult in the amplification of magnetic fields and in the acceleration of e lectrons\, injecting them into the diffusive acceleration mechanism. The acceleration of electrons and the B field amplification by the collisio n of two plasma clouds\, each consisting of electrons and ions\, at a sp eed of 0.5c is investigated. A quasi-parallel guiding magnetic field\, a cloud density ratio of 10 and a plasma temperature of 25 keV are consid ered. A quasi-planar shock forms at the front of the dense plasma cloud. It is mediated by a circularly left-hand polarized electromagnetic wave with an electric field component along the guiding magnetic field. Its propagation direction is close to that of the guiding field and orthogon al to the collision boundary. It has a low frequency and a wavelength th at equals several times the ion inertial length\, which would be indicat ive of a dispersive Alfven wave close to the ion cyclotron resonance fre quency of the left-handed mode (ion whistler)\, provided that the freque ncy is appropriate. However\, it moves with the super-alfvenic plasma co llision speed\, suggesting that it is an Alfven precursor or a nonlinear MHD wave such as a Short Large-Amplitude Magnetic Structure (SLAMS). Th e growth of the magnetic amplitude of this wave to values well in excess of those of the quasi-parallel guiding field and of the filamentation m ode results in a quasi-perpendicular shock. The waves developing upstrea m of the dense cloud give rise to electron acceleration ahead of the col lision boundary. Energy equipartition between the ions and the electrons is established at the shock and the electrons are accelerated to relati vistic speeds. LOCATION:PS1.28 CATEGORIES:CFSA Seminar LAST-MODIFIED:20091207T105013Z ORGANIZER;CN=Erwin Verwichte: END:VEVENT END:VCALENDAR