space physics mhd research

5
Personnel: Jay R. Johnson Eun-Hwa Kim QuickTime™ and a TIFF (Uncompressed) decompressor are needed to see this picture. Space Physics MHD Research

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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 Presentation

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Page 1: Space Physics MHD Research

Personnel:

Jay R. Johnson

Eun-Hwa Kim

QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

Space Physics MHD Research

Page 2: Space Physics MHD Research

Key Issues: Entry and Transport

Page 3: Space Physics MHD Research

Plasma Sheet Dynamics

• How does mass, momentum and energy enter the magentosphere?– Reconnection

– Kelvin-Helmholtz Instability

– Kinetic Alfven Waves/Mode Conversion

QuickTime™ and aH.264 decompressor

are needed to see this picture.

Page 4: Space Physics MHD Research

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

Page 5: Space Physics MHD Research

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