space physics mhd research
DESCRIPTION
Space Physics MHD Research. Personnel: Jay R. Johnson Eun-Hwa Kim. Key Issues: Entry and Transport. Plasma Sheet Dynamics. How does mass, momentum and energy enter the magentosphere? Reconnection Kelvin-Helmholtz Instability Kinetic Alfven Waves/Mode Conversion. Plasma Sheet Dynamics. - PowerPoint PPT PresentationTRANSCRIPT
Personnel:
Jay R. Johnson
Eun-Hwa Kim
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Space Physics MHD Research
Key Issues: Entry and Transport
Plasma Sheet Dynamics
• How does mass, momentum and energy enter the magentosphere?– Reconnection
– Kelvin-Helmholtz Instability
– Kinetic Alfven Waves/Mode Conversion
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Plasma Sheet Dynamics
• Entropy Definition global/total: S=p1/dv; specific/local: s = p/
• Entropy Crisis– Steady Convection– Substorm Transition
• How are ions heated?• What convects cold plasma to the center of
the plasma sheet?
Mapping Technique
Role of Heavy Ions
• At Magnetopause– Reconnection (Threshold/Growth)– KH inertial effects (Inertial Scale Effects)– Mode Conversion (Strong Absorption)
• At Planets– Mercury– Jupiter
IIR AR