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Explore the magnetic field, plasmas, currents, and force balance in the Earth's magnetosphere. Learn about radiation belts, plasma parameters, particle energization, and guiding center drift velocity in the plasmasphere.
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The Magnetosphere Feifei Jiang, UCLA fjiang@igpp.ucla.edu
Outline • Magnetic field • Plasmas • Currents • Force Balance
The Earth’s Main Field Dipole in spherical coordinates L L0 Dipole field lines
The Stretched Tail Magnetic Reconnection Viscous Interaction
The Tail Plasma Sheet Plasma parameters in the central plasma sheet E B N = 0.1~0.5 cm-3 Ti = 2~10 keV Ti/Te = 6 EXB Mantle particles will ExB drift towards the center of the tail To move from the center of mantle to the center of plasma sheet
The Radiation Belts • One proton belt: • 0.1~ 100 MeV, peak near L~1.8 • Two electron belts with a slot region: • For E> 1 MeV peak near L=1.6 and 4.0 Re Source: ~keV particles in the plasma sheet How are these particles energized? 1. Acceleration by chorus waves 2. Radial diffusion 3. Substorm injection
The Plasmasphere Guiding center drift velocity • Cold, dense plasmas: • ~103 cm-3, ~1 eV • Plasmapause, 3~5 Re depending on geomagnetic activity • 2 sources: Polar wind and convection Stagnation Point
Magnetopause Current The current crossing y=y0 per unit length in z
Field-aligned current Region 1 current: Flow shear/parallel flow vorticity Region 2 current: surfaces of constant pressure are not aligned with magnetic shells
Ring Current Magnetic field of a current loop Dessler-Parker-Sckopke relationship
Force Balance At the magnetopause nose K=0.89, a ~ 2.4 At the magnetopause on the tail side At the tail plasma sheet