ECR Plasma Thruster development at Onera
Transcription
ECR Plasma Thruster development at Onera
ECR Plasma Thruster development at Onera Denis Packan ONERA, Physics and Instrumentation Department, Palaiseau EPIC Workshop, 25-28 November 20114, Brussel Two Neutralizer-free gridded ion thrusters developed at the LPP, Ecole Polytechnique, France (Dr A. Aanesland) 1. PEGASES Plasma Propulsion with Electronegative Gases Accelerates positive and negative ions to generate thrust T. Lafleur, D. Rafalskyi and A. Aanesland, PSST 24 015005 (2014) State-of-the-art: Principle: A+ A2 A+ e- RF power Advantages: • • • • A+ A- High density ion-ion plasma Alternate ± ion beams A- A- Electronegative plasma A proof-of-concept combining experiments, simulations and analytical models Magnetic Ion-ion Alternate Recombination barrier plasma acceleration v External e-neutralizer redundant Interesting plume properties (no electrons and low density of charged particles) Control of the emitted net charge Solid propellant (Iodine) v Generalized CL law for alternate acceleration Full space charge compensation in the beam Two Neutralizer-free gridded ion thrusters developed at the LPP, Ecole Polytechnique, France Technology transfer from the semiconductor industry Accelerates continuously positive ions with burst of electrons D. Rafalskyi and A. Aanesland, J.Phys.D: 47 495203 (2014) 2. Neptune State-of-the-art: Principle: Laboratory proof-of-concept RF rectification to a DC bias RF to DC bias linear dependency RF source (ICP) RF biased grid A+ e RF Blocking capacitor Advantages: • • • • • • mean ion energy v No Cathode Capacitive system ensure extracted Idc=0 Anisotropic EEDF = low plume divergence No DC amplification needed Any gas can be used also solid iodine Technology heritage from ion engines v electron extraction Efficient RF extraction High ion energies Low anisotrop electron energies ECR Thruster Principle • • Electron heating in an electron cyclotron resonance (ECR) source + Plasma acceleration in a magnetic nozzle ECR effect: application of an EM field at electron cyclotron frequency eB ce at 2.45 GHz, B=875 Gauss me Efficient ionization of the propellant gas (Ar, Xe) • Magnetic nozzle: divergent magnetic field electron acceleration: conversion of electron gyrokinetic energy to longitudinal energy formation of a space charge at the thruster exit acceleration of ions by ambipolar electric field ECRA Thruster : Advantages and challenges Intrinsic advantages of ECRA thruster over existing electric propulsion technologies: • Plasma and plume electrically neutral no need for a neutralizer high thrust density (no space charge limit) • No DC electric field needed no grid or electrodes, no erosion (natural magnetic shiedling) no need for an additional power supply (only microwave) →Simplicity: reduced cost, increased reliability Potentially (observed): variable Isp (mission flexibility), magnetic beam steering Challenges for studies (with respect to other thrusters): - Plasma physics more complex than other thrusters (wave/ionisation/acceleration coupling): difficult to model. No direct experimental knowledge of the total current and of the ion energy: need for very refined experimental characterization Previous studies • ECR thruster studied in the 60s, and at Caltech in the 80s. • Experimental limitations: • • • • • high power studies: cost of design iterations limited pumping rates mircowave technology not mature no rare earth magnets limited numerical simulations → new study with lower power, new approach, more mature technologies. Results obtained already better. ECRA Thruster ONERA : Principle ωce 7 eB me at 2.45 GHz B=875 Gauss Microwave chain • • Measurement of forward power and reflected power power absorbed by the ECR source Only coaxial cables are used (no waveguides) compact thruster Circulator 2.45 GHz Bidirectional coupler MW generator 50 Ω Forward Reflected power power DC block ECR source ECR Source • • • • • Coaxial geometry: antenna-to-cylinder Small dimensions (Diameter=13mm, source length=15 mm) MW power provides a radial electric field Antenna and cylinder are floating Radial injection of the propellant gas (argon) ECR Source Magnetic field produced by permanent magnets: purely divergent in the source and the magnetic nozzle ECR source 1400 250 cylinder 1000 B dBz/dz 150 800 resonance at 2,45 GHz 100 600 50 400 0 200 -50 -100 0 0 magnet 10 20 30 40 Axial position z [mm] 50 60 dBz/dz [Gauss/m] 200 1200 |B| [Gauss] • View of ECR Thruster in Operation ECRA design configuration ECRA magnets version 13 mm diameter ECRA Coil version 27 mm diameter Influence of the Mass Flow on IEDF •Ion energy peaks shifted to lower energy when increasing gas density •Ion mean energy and thruster potential follow similar trends (Hiden mass-energy spectrometer) 200 350 Qm(Xe): 150 250 200 100 150 100 50 50 0 0,0 0 100 200 Ion energy [eV] 300 400 0,1 0,2 Qm(Xe) (mg/s) 0,3 Thruster potential (V) 300 Ei (eV) 0.06 mg/s 0.1 mg/s 0.15 mg/s 0.2 mg/s 0.3 mg/s Ion Mass Analysis • • Mainly Xe+ ions Small amounts of Xe2+, traces of Xe3+ Qm=0.1 mg/s, P=30 W Xe+ Xe2+ 0 20 40 60 80 m/z 100 120 140 Ion energy versus azimuthal angle. Angular profile of energy spectrum Qm(Ar)=0.2 mg/s Magnetic nozzle: LIF and emissive probe measurements 240 0.1 mg/s 0.06 mg/s 220 200 Calculated from: Doppler shift (LIF) Emissive probe 110 100 180 Plasma potential [V] Plasma potential [V] 0.1 mg/s 120 160 140 120 100 80 60 90 80 70 60 50 40 30 40 20 20 10 0 0 0 20 40 Axial position [mm] 60 80 0 20 40 60 80 100 120 140 160 180 200 220 240 Axial position [mm] Good agreement between velocity measurements (LIF) and plasma potential measurements (emissive probe) Results and perspectives Mass utilization Power Divergence Thruster Thrust to Power Mass flow rate Power ion energy Ion current Isp [s] Thrust [mN] efficiency [%] efficiency [%] efficiency [%] efficiency [%] ratio [mN/kW] [mg/s] absorbed [W] [eV] [mA] Gas Xenon 0,1 30,0 248,5 45,5 0,98 33 1001 0,62 0,38 0,83 16,1% Efficiency at the level of the state-of-the-art • Magnetic topology: • • • • • • • • • larger ECR zone (parallel B region) magnetic mirror at the exit: control of energy, better ionization magnetic mirror at the bottom: reduce losses to back wall …… Microwave coupling: slit, waveguide, …. n e2 2 Frequency: try 5 GHz (potentially 4 times the density) p m 0 Scale-up : 10 mN, then 100 mN Advanced diagnostic: thrust balance (activity proposed under Neosat, with support of Astrium and TAS), 3D LIF Modeling of the thruster Roadmap: Currently TRL 3. Promising performance, no show stopper at this time. Could be an emerging technology for space propulsion. Objective TRL 4: mastering all parameters and scale-up, get good averall efficiency (objective 50% @ 1 kW): scientific study ~3 years for TRL 4 → Go / No Go in 2017. TRL 6/8 in 2022 Compatible with H2020.