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National Undergraduate Fellowship Program in Plasma Physics and Fusion Engineering Plasma Astrophysics Michael Brown Swarthmore College June 2007 Outline.

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Presentation on theme: "National Undergraduate Fellowship Program in Plasma Physics and Fusion Engineering Plasma Astrophysics Michael Brown Swarthmore College June 2007 Outline."— Presentation transcript:

1 National Undergraduate Fellowship Program in Plasma Physics and Fusion Engineering Plasma Astrophysics Michael Brown Swarthmore College June 2007 Outline Brief plasma review (B-fields and MHD) Two important paradigms Astrophysical objects (solar flares to galactic jets) Astrophysical processes (dynamos, reconnection and pulsars)

2 Astrophysical Plasma Review Magnetic fields… related to electric fields by Lorentz transformation Q: why are there large scale B-fields but no large scale E-fields in the universe? A:...there are lots of electric monopoles around to short out electric fields B-fields are associated with currents but do currents cause B- fields are vice-versa? exert forces on currents Force=JxB contain energy

3 Astrophysical Plasma Review Newton II: Maxwell’s eqs: equations of MHD Ohm’s Law: induction eq. (curl of Ohm):

4 Astrophysical Plasma Review ramifications of MHD

5 Astrophysical Plasma Review Frozen-in Flux high conductivity: Coulomb collisionality drops with T (so  ~ T -3/2 ) universe is an excellent conductor of electricity almost everywhere frozen-in flux: assume perfectly conducting magnetofluid no electric field in a perfect conductor if field lines move with respect to fluid then an electric field is induced therefore fields move with the fluid!

6 Poynting Vector

7 Simple 2D Reconnection Theory (Sweet/Parker)

8 Reconnection Rate where R m is based on the Alfven velocity in the bulk magnetofluid and on the largest scale of the system L. M alf is a dimensionless measure of the reconnection rate or the rate at which magnetic field lines are annihilated or the direct electric field. More sophisticated models [Petschek, 1964 and Vasyliunas, 1975] predict a faster reconnection rateand a smaller ration of u out /u in. It appears, however that a bound exists:


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