CASSINI In Space

 

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GALILEO

Investigation of the Magnetosphere of Ganymede with Galileo's Energetic Particle Detector


Ph.D. dissertation by Shawn M. Stone, University of Kansas, 1999.

 

Copyright 1999 by Shawn M. Stone.  Used with permission.

 

M1 07:22:14 Figures

 

Figure B34 (A) Simulated M1 and real (Re) rate profile for the feature G7-07:22:14 of channel E1 normalized to 90º of pitch. The simulated runs are done in extended bounce mode with scattering included. Stars show a scattering coefficient of 50x10-3 and diamonds show a scattering coefficient of 10x10-3. (B) The pitch and phase angles are computed from the look direction of the EPD detector and the appropriate magnetic field vector R for real and S for simulated.
Figure B35 (A) Simulated M1 and real (Re) rate profile for the feature G7-07:22:14 of channel E1 normalized to 90º of pitch. The simulated runs are done in extended bounce mode with scattering included. Stars show a scattering coefficient of 50x10-3 and diamonds show field trace results with no scattering. (B) The pitch and phase angles are computed from the look direction of the EPD detector and the appropriate magnetic field vector R for real and S for simulated.
Figure B36 (A) Simulated M1 and real (Re) rate profile for the feature G7-07:22:14 of channel E3 normalized to 90º of pitch. The simulated runs are done in extended bounce mode with scattering included. Stars show a scattering coefficient of 50x10-3 and diamonds show a scattering coefficient of 10x10-3. (B) The pitch and phase angles are computed from the look direction of the EPD detector and the appropriate magnetic field vector R for real and S for simulated.
Figure B37 (A) Simulated M1 and real (Re) rate profile for the feature G7-07:22:14 of channel E3 normalized to 90º of pitch. The simulated runs are done in extended bounce mode with scattering included. Stars show a scattering coefficient of 50x10-3 and diamonds show field trace results with no scattering. (B) The pitch and phase angles are computed from the look direction of the EPD detector and the appropriate magnetic field vector R for real and S for simulated.
Figure B38 (A) Simulated M1 and real (Re) rate profile for the feature G7-07:22:14 of channel F2 normalized to 90º of pitch. The simulated runs are done in extended bounce mode with scattering included. Stars show a scattering coefficient of 50x10-3 and diamonds show a scattering coefficient of 10x10-3. (B) The pitch and phase angles are computed from the look direction of the EPD detector and the appropriate magnetic field vector R for real and S for simulated.
Figure B39 (A) Simulated M1 and real (Re) rate profile for the feature G7-07:22:14 of channel F2 normalized to 90º of pitch. The simulated runs are done in extended bounce mode with scattering included. Stars show a scattering coefficient of 50x10-3 and diamonds show field trace results with no scattering. (B) The pitch and phase angles are computed from the look direction of the EPD detector and the appropriate magnetic field vector R for real and S for simulated.

 

 

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Updated 8/23/19, Cameron Crane

QUICK FACTS

Manufacturer: The Galileo Spacecraft was manufactured by the Jet Propulsion Laboratory, Messerschmitt-Bölkow-Blohm, General Electric, and the Hughes Aircraft Company.

Mission Duration: Galileo was planned to have a mission duration of around 8 years, but was kept in operation for 13 years, 11 months, and 3 days, until it was destroyed in a controlled impact with Jupiter on September 21, 2003.

Destination: Galileo's destination was Jupiter and its moons, which it orbitted for 7 years, 9 months, and 13 days.