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Mini-Magnetospheric Plasma 
Propulsion (M2P2): 
for 
High Speed Interplanetary and 
Heliospheric Missions 
R. M. Winglee 
Geophysics Program, Univ. of Washington 
J. Slough, T. Ziemba, P. Euripides 
Aeronautics and Astronautics, Univ. Of Washington
Mini-Magnetospheric Plasma Propulsion (M2P2) 
• Facilitate High Speed Spacecraft 
For the Exploration of the Solar System and Beyond 
• Use the Solar Wind as a Free Energy Source 
Greatly reduce the Energy and Fuel Requirements -> 
Cheaper, Faster and More Diverse Missions 
• Enabling Technology Exists Today 
to attain 50-80 km/s in 3 month accel. period 
• Immediate Return to NASA Missions 
- Interstellar Probe Precusor 
race Voyager 1 out of the Solar System 
- Planetary Missions: Mars, Jupiter
Interstellar 
Wind 
Heliopause : End of the Plasma 
Solar System 
Termination 
Shock: 
Subsonic 
Solar Wind 
Solar Wind 
Voyager 1: 
Launched 1977
Proposed NASA Missions : Sample Return 
Needed: Fast Propulsion 
Radiation Shielding 
The Moon 
(<100 day) 
Mars 
(<1000 day) 
Jupiter 
(<5000 day)
Formation of a Magnetic Wall 
Supersonic Solar Wind 
(400 - 1000 km/s) 
Streamlines 
& 
Contours of 
density 
Magnetic Wall 
•15 - 30 km radius 
•Electromagnetic- 
Plasma Interaction 
•Not Mechanical 
•Constant Force Surface
10 
0 
y (RE) 
-10 
Earth 
and its 
Magnetosphere 
-16 0 x (RE) 24 
1 RE = 6371 km
Mars 
and its 
Magnetosphere 
6 
3 
0 
1 RM = 3393 km 
-2 0 x (RM) 6 
y (RM)
150 
0 
Jupiter 
and its 
Magnetosphere 
-1-51050 0 x (RJ) 300 
1 RE = 71,600 km 
y (RJ)
Solar Activity : 
Corona Mass Ejections 
Example of Magnetic 
Inflation in Nature
Creating A Mini-Magnetosphere 
Magnetic Field + Plasma Injection = Strong Solar Wind 
Spacecraft 
Magnetic 
Field 
Solar Wind 
IMF Bow Shock 
Coupling 
Plasma 
Injection 
Dipole : B ~ R 
-3 
Current Sheet : B ~ R -1
Magnetic Wall for Large Scale Radiation 
Shielding 
Isosurface of Magnetic Field Intensity
M2P2 Milestones: 
Prove Feasibility through Computer Simulations (Phase 1) 
Generation of High Density, Strongly Magnetized Plasma 
1011 cm-3 plasma density 
 300 G magnetic field 
 1 kW of Power 
~ 0.25 to 1 kg/day fuel consumption 
Demonstrate Inflation of Magnetic Field 
Test Performance of Different Propellants 
• Demonstrate Deflection and Thrust from a Plasma Wind
M2P2 Capabilities 
 Mini-Magnetosphere (Single Unit) : 20-30 km Radius 
Inflation is Purely Electromagnetic 
No Large Mechanical Struts have to be deployed 
 Intercept 
~ 1-3 N of Solar Wind Force 
~ 0.6 MW of Solar Wind Energy 
 Scientific Payload of 100 to 20 kg would attain 
50- 80 km/s in 3 month acceleration period 
Economies of Scale for Multiple Units
Propellant 
Plasma 
Limiter 
Quartz 
Tube 
Helicon 
Antenna ionizes 
gas 
Magnetic 
Field Coils 
Ionized gas 
inflates magnetic 
field 
Magnetic Field Lines 
Inside the M2P2: 
~ 1011 cm-3, few eV 
~ 400 G
Experimental Arrangement 
400 Liter Vacuum 
Chamber 
Propellant Bottle 
RF Amplifier 
Power Supply
Experimental Arrangement 
RF plasma source 
Dipole magnets 
Gas feed tube 
400 liter vacuum 
chamber 
Top View
Helical single turn coil 
5cm OD (Copper braid) 
Quartz encasement 
Center gas feed 
Helium: 40 mTorr, No 
magnetic Field
Laboratory Helicon Antenna Design 
Argon: 15 mTorr, 600 ms, 350 G
Argon: 350 G, 250 msec exposure, 200 W input 
(a) 0.25 mTorr (b) 1.0 mTorr 
Plasma Production: ~ 1012 cm-3
Argon: 500 G 2 mTorr, 280 W, 250 msec 
duration – frames from an mpeg movie 
Motion of Field Lines
Nitrogen: 0.5 mTorr, 350 G, 
1200 ms, 500 W 
Helium: 4.0 mTorr, 350 G, 
1200 ms, 500 W 
 M2P2 has flexibility in propellant to be used
Mini-Magnetospheric Plasma Propulsion 
New Approach for Rapid Exploration of the Solar System 
• Description 
– Create a magnetic bubble around and 
attached to a spacecraft that will then be 
carried by the solar wind. 
– Low energy plasma is used to inflate the 
magnetic field to produce a large cross-section 
(15-30 km) requiring about 
3-9 mN of force, 1 kilowatt of power 
and 0.25 – 1.0 kg/day 
• M2P2 - Low-Cost Advanced Propulsion 
– Intercept 1-3 N of force 
– 0.6 MW of solar wind power 
– Accelerate a spacecraft of 100-200 kg to 50- 
80 km/s with an acceleration period of about 3 
months using only about 15 to 30 kg of 
propellant. 
• Economies of Scale with Multiple Units 
– Reduction of Surface to Volume Ratio 
– Lead to smaller losses of plasma from the 
mini-magnetosphere 
• M2P2 - Magnetic Radiation Shield 
– At a radius of few 100 km reflect MeV and 
possibly GeV cosmic rays 
– Ideally suited for Human Exploration
Mini-Magnetospheric Plasma Propulsion 
Technology Readiness Level and Potential Applications 
• Working Lab. Prototype 
– Small Facility at Univ. of Washington 
– Preparing for a Large Tank Test at NASA-Marshall 
• Potential Applications: 
Interstellar Precusor Mission 
– LEO De-orbiting 
– Geosynchronous Station Keeping 
– Geosynchronous to Escape Velocity 
– High Speed Planetary Orbit Transfers 
– Magnetospheric/Solar Wind Braking 
•Variety of Propellants Possible 
–Argon or Helium (for lab use) 
–Liquid Hydrogen 
–Water – refueling in space 
–Waste Products : CO2, NH3

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Plasma propulsionm2p2

  • 1. Mini-Magnetospheric Plasma Propulsion (M2P2): for High Speed Interplanetary and Heliospheric Missions R. M. Winglee Geophysics Program, Univ. of Washington J. Slough, T. Ziemba, P. Euripides Aeronautics and Astronautics, Univ. Of Washington
  • 2. Mini-Magnetospheric Plasma Propulsion (M2P2) • Facilitate High Speed Spacecraft For the Exploration of the Solar System and Beyond • Use the Solar Wind as a Free Energy Source Greatly reduce the Energy and Fuel Requirements -> Cheaper, Faster and More Diverse Missions • Enabling Technology Exists Today to attain 50-80 km/s in 3 month accel. period • Immediate Return to NASA Missions - Interstellar Probe Precusor race Voyager 1 out of the Solar System - Planetary Missions: Mars, Jupiter
  • 3. Interstellar Wind Heliopause : End of the Plasma Solar System Termination Shock: Subsonic Solar Wind Solar Wind Voyager 1: Launched 1977
  • 4. Proposed NASA Missions : Sample Return Needed: Fast Propulsion Radiation Shielding The Moon (<100 day) Mars (<1000 day) Jupiter (<5000 day)
  • 5. Formation of a Magnetic Wall Supersonic Solar Wind (400 - 1000 km/s) Streamlines & Contours of density Magnetic Wall •15 - 30 km radius •Electromagnetic- Plasma Interaction •Not Mechanical •Constant Force Surface
  • 6. 10 0 y (RE) -10 Earth and its Magnetosphere -16 0 x (RE) 24 1 RE = 6371 km
  • 7. Mars and its Magnetosphere 6 3 0 1 RM = 3393 km -2 0 x (RM) 6 y (RM)
  • 8. 150 0 Jupiter and its Magnetosphere -1-51050 0 x (RJ) 300 1 RE = 71,600 km y (RJ)
  • 9. Solar Activity : Corona Mass Ejections Example of Magnetic Inflation in Nature
  • 10. Creating A Mini-Magnetosphere Magnetic Field + Plasma Injection = Strong Solar Wind Spacecraft Magnetic Field Solar Wind IMF Bow Shock Coupling Plasma Injection Dipole : B ~ R -3 Current Sheet : B ~ R -1
  • 11.
  • 12. Magnetic Wall for Large Scale Radiation Shielding Isosurface of Magnetic Field Intensity
  • 13. M2P2 Milestones: Prove Feasibility through Computer Simulations (Phase 1) Generation of High Density, Strongly Magnetized Plasma 1011 cm-3 plasma density 300 G magnetic field 1 kW of Power ~ 0.25 to 1 kg/day fuel consumption Demonstrate Inflation of Magnetic Field Test Performance of Different Propellants • Demonstrate Deflection and Thrust from a Plasma Wind
  • 14. M2P2 Capabilities Mini-Magnetosphere (Single Unit) : 20-30 km Radius Inflation is Purely Electromagnetic No Large Mechanical Struts have to be deployed Intercept ~ 1-3 N of Solar Wind Force ~ 0.6 MW of Solar Wind Energy Scientific Payload of 100 to 20 kg would attain 50- 80 km/s in 3 month acceleration period Economies of Scale for Multiple Units
  • 15. Propellant Plasma Limiter Quartz Tube Helicon Antenna ionizes gas Magnetic Field Coils Ionized gas inflates magnetic field Magnetic Field Lines Inside the M2P2: ~ 1011 cm-3, few eV ~ 400 G
  • 16. Experimental Arrangement 400 Liter Vacuum Chamber Propellant Bottle RF Amplifier Power Supply
  • 17. Experimental Arrangement RF plasma source Dipole magnets Gas feed tube 400 liter vacuum chamber Top View
  • 18. Helical single turn coil 5cm OD (Copper braid) Quartz encasement Center gas feed Helium: 40 mTorr, No magnetic Field
  • 19. Laboratory Helicon Antenna Design Argon: 15 mTorr, 600 ms, 350 G
  • 20. Argon: 350 G, 250 msec exposure, 200 W input (a) 0.25 mTorr (b) 1.0 mTorr Plasma Production: ~ 1012 cm-3
  • 21. Argon: 500 G 2 mTorr, 280 W, 250 msec duration – frames from an mpeg movie Motion of Field Lines
  • 22. Nitrogen: 0.5 mTorr, 350 G, 1200 ms, 500 W Helium: 4.0 mTorr, 350 G, 1200 ms, 500 W M2P2 has flexibility in propellant to be used
  • 23. Mini-Magnetospheric Plasma Propulsion New Approach for Rapid Exploration of the Solar System • Description – Create a magnetic bubble around and attached to a spacecraft that will then be carried by the solar wind. – Low energy plasma is used to inflate the magnetic field to produce a large cross-section (15-30 km) requiring about 3-9 mN of force, 1 kilowatt of power and 0.25 – 1.0 kg/day • M2P2 - Low-Cost Advanced Propulsion – Intercept 1-3 N of force – 0.6 MW of solar wind power – Accelerate a spacecraft of 100-200 kg to 50- 80 km/s with an acceleration period of about 3 months using only about 15 to 30 kg of propellant. • Economies of Scale with Multiple Units – Reduction of Surface to Volume Ratio – Lead to smaller losses of plasma from the mini-magnetosphere • M2P2 - Magnetic Radiation Shield – At a radius of few 100 km reflect MeV and possibly GeV cosmic rays – Ideally suited for Human Exploration
  • 24. Mini-Magnetospheric Plasma Propulsion Technology Readiness Level and Potential Applications • Working Lab. Prototype – Small Facility at Univ. of Washington – Preparing for a Large Tank Test at NASA-Marshall • Potential Applications: Interstellar Precusor Mission – LEO De-orbiting – Geosynchronous Station Keeping – Geosynchronous to Escape Velocity – High Speed Planetary Orbit Transfers – Magnetospheric/Solar Wind Braking •Variety of Propellants Possible –Argon or Helium (for lab use) –Liquid Hydrogen –Water – refueling in space –Waste Products : CO2, NH3