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Mini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher, P. Craven, NASA, MSFC W. Tomlinson, J. Cravens, J. Burch, SwRI Create a magnetic bubble around and attached to a spacecraft that will be pushed by the solar wind to produce a substantial enhancement in the thrust on the spacecraft for a given power
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Page 1: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Mini-Magnetospheric Plasma Propulsion (M2P2)

R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington

D. Gallagher, P. Craven, NASA, MSFCW. Tomlinson, J. Cravens, J. Burch, SwRI

Create a magnetic bubble around and attached to a spacecraft that will be pushed by the solar wind to produce a substantial enhancement in the thrust on the spacecraft for a given power

Page 2: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

The Solar System : A Large Unexplored Region

Voyager 1: Launched 1977

Page 3: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

AdvancedElectrical

(MPD)

Ion Engines(Deep Space 1)

M2P2

Specific Impulse (sec)

Thru

st (N

)

Che

mi c

al P

rope

ll ant

s

10

1

.1

.01

100 1,000 10,000 100,000

The Need for Advanced Propulsion Systems

Page 4: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

The Dynamic Sun:

soft X-RaysUVVisible

Electrical Storms raising the solar corona (solar atmosphere to 2 million degrees)

Page 5: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Expanding Magnetic Flare Loops seen by Yohkoh

Page 6: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

The Solar Wind

•Charged Particles: Ions and electrons

•300-800 km/s

•Tenuous being only about 6 particles per cubic cm at Earth

Page 7: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Magnetosphere: Magnetic field, usually attached to a planet or moon, that is able to deflect the charged particles of the solar wind

Page 8: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 9: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 10: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 11: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 12: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 13: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 14: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example of Solar Wind Ions interacting with a magnetosphere

Page 15: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

M2P2• Seeks to create a magnetosphere around the spacecraft

• Enhanced the size of the magnetosphere by the injection of low energy plasma

• Size needs to be about 20-30 km radius

•Advantage is that the inflation is done fully electromagnetically, and deployment of large scale structures in space

Page 16: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,
Page 17: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Initial Magnetic Field

Terrestrial

Field Lines

Magnetic

Field

Lines

Page 18: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Expanding Magnetic Field

Terrestrial

Field Lines

Magnetic

Field

Lines

Page 19: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Expanding Magnetic Field

Terrestrial

Field Lines

Magnetic

Field

Lines

Page 20: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Terrestrial

Field Lines

Magnetic

Field

Lines

Expanding Magnetic Field

Page 21: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

M2P2 Milestones:�Prove Feasibility through Computer Simulations

�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

�Demonstrate Deflection of an external Plasma Wind

�Test Performance of Different Propellants

� Measure Thrust and verify Efficiency

Page 22: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

M2P2 Capabilities� Mini-Magnetosphere (Single Unit) : 20-30 km Radius

Inflation is Purely ElectromagneticNo Large Mechanical Struts have to be deployed

� Intercept ~ 1-3 N of Solar Wind Force~ 0.6 MW of Solar Wind Energy using only ~ 1kW

� Scientific Payload of 100 to 200 kg would attain50- 80 km/s in 3 month acceleration period

�Economies of Scale for Multiple Units

Page 23: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

400 Liter Vacuum Chamber

Propellant Bottle

RF Amplifier

Power Supply

Experimental Arrangement

Page 24: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

• Prototype Specifications– 11 cm radius magnet, 300-1000 G– Antenna, small (1.5 cm radius) and large

( 2.5 cm radius), ~ 1kW

• Prototype Performance– Sustained densities of 1013 cm-3

– Temperatures of 4 – 12 eV– Small Antenna: 0.4 kg/day (5.4 mg/s) @

25% gas efficiency, for 3.3 amps of plasma and 4 mN

– Large Antenna: 0.8 kg/day (11 mg/s) @>50% gas efficiency, for 12 amps and 16 mN

•Variety of Propellants Possible–Argon or Helium (for lab use)–Nitrogen/Hydrogen–Water – refueling in space–Other light weigh fuels : CH4, NH3

CO2,

Mini-Magnetospheric Plasma Propulsion:Prototype Development and Performance

RF Antenna

Magnetic Field Coil

Gas Feed Support StrutElectronics Box

Page 25: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Examples of

Plasma

Inflation

Page 26: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,
Page 27: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

NASA/MSFC

Test Area 300

Vacuum Chamber

32 ft high by 18 ft

Objectives:

• Demonstrate Magnetospheric Inflation

•Demonstrate Magnetospheric Plasma Deflection

Page 28: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Demonstration of Plasma Expansion of a Mini-Magnetosphere:

•Large Chamber Tests at MSFCHelium plasma @ 350 G–Vacuum field solution shows no

closed field lines within ~ 3ft–Plasma emissions initially seen to

closely match the vacuumfield solution

–Expansion seen as plasma βapproaches unity.

–Expansion out to at least 30 timesthe magnet radius demonstrated.

–Main limitation due to recombination with chamber neutrals

Page 29: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

M2P2: MSFC Operation

Page 30: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Demonstration of Plasma Deflection by a Mini-Magnetosphere: M2P2 vs SEPAC

•SEPAC (right hand side)– 4 Amp Xenon ion source– 800 W @ 1 eV

•M2P2 (left hand side)– ~ 4 Amps of Argon @ 400 W– the two sources separated by about

14 ft (only 6ft field of view around M2P2 shown in figures)

•Deflection–Permanent barrier (magnetopause)

seen better the two plasmas–Barrier moves to the right as the

magnetosphere is inflated–Barrier moves to right with increase

magnetic field

(a) 400 G (Shot P)

(b) 800 G (Shot Q)

Page 31: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

M2P2 vs SEPAC

Page 32: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Mission Designs:• Mars Return (1.8 yrs)

• Jupiter Orbital (1.3yrs)

• Saturn/Titan (5.6 yrs)

• Pluto (6.2 yrs)

• Heliopause (10 yrs)

Page 33: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Example M2P2 Mission

250 Days to Mars Earth Orbit

Mars Orbit

M2P2 On

Coast

Page 34: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

250 Days to Mars

130 Days on Surface

Earth Orbit

Mars Orbit

M2P2 On

Coast

Example M2P2 Mission

Page 35: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

250 Days to Mars

130 Days on Surface

290 Day Return

Earth Orbit

Mars Orbit

M2P2 On

Coast

Example M2P2 Mission

Page 36: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

250 Days to Mars

130 Days on Surface

290 Day Return

Total: 1.8 Years

Earth Orbit

Mars Orbit

M2P2 On

Coast

Example M2P2 Mission

Page 37: Mini-Magnetospheric Plasma Propulsion (M2P2) - · PDF fileMini-Magnetospheric Plasma Propulsion (M2P2) R. M. Winglee, T. Ziemba, J. Slough, P. Euripides, Univ. of Washington D. Gallagher,

Concept

Mar.,991st Prototype

Dec.,99

Phase II

Large ChamberTesting

Aug.,00

Verificationof concept

Feb.,01 Efficiency,Thrust

PresentPhase I

NIAC Timeline


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