Hall effect thruster

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2 kW Hall thruster in operation as part of the Hall Thruster Experiment at the Princeton Plasma Physics Laboratory.
2 kW Hall thruster in operation as part of the Hall Thruster Experiment at the Princeton Plasma Physics Laboratory.

A Hall effect thruster (HET) or Hall thruster is a type of ion thruster in which the propellant is accelerated by an electric field in a plasma discharge with a radial magnetic field. Also known simply as plasma thrusters, HETs use the Hall effect to trap electrons and then use the electrons to ionize propellant, efficiently accelerate the ions to produce thrust, and neutralize the ions in the plume.

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[edit] Research

The Hall thruster was studied independently in the U.S. and the Soviet Union in the 1950s and 60s. The concept of a Hall thruster was only developed into an efficient propulsion device in the former Soviet Union. (In the U.S., scientists focused instead on developing gridded ion thrusters.) Two types of Hall thrusters were developed, the Stationary Plasma Thruster (SPT) at Design Bureau Fakel, and the Thruster with Anode Layer (TAL), at the Central Research Institute for Machine Building (TsNIIMASH). These thrusters were introduced to the West in 1992 after a team of electric propulsion specialists, under the support of the Ballistic Missile Defense Organization, visited Soviet laboratories and experimentally evaluated the SPT-100 (i.e., a 100 mm diameter SPT thruster). Over 200 Hall thrusters have been flown on Soviet/Russian satellites in the past thirty years. They were used mainly for stationkeeping and small orbital corrections.

This technology was used on the European lunar mission SMART-1 and is used on a number of commercial geostationary satellites [1].

Current research on Hall thrusters is ongoing and focuses mainly on:

  1. Scaling the typically 1-kW Hall thruster to higher powers (50 to 100 kW) and lower powers (50 to 100 W)
  2. Resolving spacecraft integration issues regarding the large plume divergence
  3. Enabling operation at higher specific impulse and variable specific impulse
  4. Flight validating thrusters for use on western spacecraft

A Hall thruster typically operates at around 50–60% thrust efficiency and provides specific impulse from 1,200 to 1,800 seconds (12 to 18 kN·s/kg), and thrust-to-power ratios of 50–70 mN/kW.

[edit] Operation

Schematic of a Hall Thruster
Schematic of a Hall Thruster

A schematic of a Hall thruster is shown in the image to the right. (Notice that this is a cross-section of an axis-symmetric device.) The Hall thruster discharge is a DC plasma discharge. An electric potential on the order of 300 volts is applied between the anode and cathode. Xenon gas, which is the propellant, is fed through the anode, which has numerous small holes in it to act as a gas distributor. Xenon propellant is used because of its high molecular weight and low ionization potential. As the neutral xenon atoms diffuse into the channel of the thruster, they are ionized by collisions with high energy electrons (10–20 eV or 100,000 to 250,000 °C). The xenon ions typically have a charge of +1 though a small fraction (~10%) are +2. The xenon ions are then accelerated by the electric field between the anode and the cathode. The electric field accelerates the ions to around 15,000 m/s (or a specific impulse of 1,500 seconds (15 kN·s/kg)).

The magnetic field in the thruster traps electrons, creating a ring-shaped electron cloud at the exit of the anode channel. The ions are accelerated toward this cloud and out of the thruster. Upon exiting, the ions pull an equal number of electrons with them, creating a plume with no net charge. In a hall thruster, a magnetic field is used to ensure that the discharge power goes into accelerating the xenon propellant and not the electrons, thus the thruster is efficient. The magnetic field is strong enough to substantially deflect the low-mass electrons, but not the high-mass ions. The majority of electrons are thus stuck orbiting in the region of high radial magnetic field near the thruster exit plane, while the ions are accelerated and produce thrust. The electrons are trapped in E×B (axial electric field and radial magnetic field) and rotate azimuthally. This azimuthal rotation of the electrons is a Hall current and it is from this that the Hall thruster gets its name. Collisions and instabilities allow some of the electrons to be freed from the magnetic field and they move towards the anode. About 30% of the discharge current is electron current and doesn't produce thrust, which limits the efficiency of the thruster; only 70% of current is ions. Because the majority of electrons are trapped in the Hall current, they have a long residence time inside the thruster and are able to ionize almost all (~90%) of the xenon propellant. The ionization efficiency of the thruster is thus around 90%, while the discharge current efficiency is around 70% for a combined thruster efficiency of around 60% (= 90% × 70%).

The amount of thrust is very small, on the order of 80 mN for a typical thruster. For comparison, the weight of a coin like the U.S. quarter or a 20-cent Euro coin is approximately 60 mN.

Hall thrusters are a type of ion thruster, and thus operate at a high specific impulse. One advantage of Hall thrusters is that the acceleration of the ions takes place in a quasi-neutral plasma and so there is no Child-Langmuir charge saturated current limitation on the thrust density. Another advantage of the Hall thruster is the high ionization efficiency. One problem with Hall thrusters is that there is a wide spread in the angle of the ions in the plume of the thruster. The ions can impinge on other spacecraft parts leading to thermal and contamination problems.

[edit] Applications

The solar electric propulsion system of the European Space Agency's SMART-1 spacecraft used a Hall thruster. Over the course of 13 months and 289 engine pulses it had consumed about 58.8 kg of xenon and produced a delta-v of 2737 m/s (46.5 m/s per kg xenon). A similar thruster is planned for the upcoming BepiColombo mission.

[edit] See also

[edit] External links

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