Pre-Phase A Report - Lisa - Nasa
Pre-Phase A Report - Lisa - Nasa
Pre-Phase A Report - Lisa - Nasa
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152 Chapter 7 Spacecraft Design<br />
There are mainly two designs being pursued by Centrospazio (Italy) and at the Austrian<br />
Research Centre Seibersdorf (ARC). The FEEPs originally developped by Centrospazio<br />
were designed for thrusts in the milli-Newton regime, as required for communication<br />
sattelites. For LISA, they had to be scaled-down by a factor of a thousand from the<br />
original design. The development at ARC, the Indium Liquid-Metal Ion Sources (In-LMIS)<br />
have originally been designed for spacecraft charge control and microanalysis instruments.<br />
They have already been flown on various missions and proven their reliability in space<br />
during more than 800 hours of operations.<br />
The description in the following subsections mainly refer to the Centrospazio design. We<br />
come back to the ARC design in subsection 7.3.5 .<br />
7.3.1 History of FEEP development<br />
Research on Field Emission Electric Propulsion (FEEP) using liquid metals has been<br />
carried out by ESA since 1972. The thruster has evolved from a single-pin emitter configuration<br />
in 1972, through linear arrays of stacked needles in 1975, to the high-efficiency<br />
solid-slit emitter in 1979. During the past phases of the development program, all the<br />
components of the system have been designed and tested, and the emitter manufacture<br />
problems have been solved. At that time, development had entered the industrialization<br />
phase, and research was devoted to the testing of the whole system in view of an application<br />
in the milli-Newton range, mainly for North-South station-keeping operations in<br />
geostationary telecommunication satellites. The high power-to-thrust ratio of FEEPs, in<br />
comparison with other electric propulsion systems now fully developed, made FEEPs lose<br />
competitiveness for this specific application. However, a rising interest of the international<br />
scientific community in missions requiring micro-Newton thrust levels for ultra-fine<br />
pointing operations (such as in LISA) sparked the present reorientation of FEEP activities<br />
to this new thrust range.<br />
7.3.2 The Field Emission Electric Propulsion System<br />
In the FEEP system, ions are created directly from the surface of a liquid metal exposed<br />
to vacuum, by means of a strong electric field resulting from suitable voltages applied to<br />
an emitting unit.<br />
When the surface of a liquid metal is subjected to a strong electric field, it distorts itself<br />
into a series of cusps that protrude more and more from the surface plane: the radius<br />
of curvature of the cusp tips becomes smaller and smaller, thus in turn increasing the<br />
strength of the local electric field. When the field reaches values of the order of 109 V/m,<br />
the atoms of the metal tip spontaneously ionize, and these ions are accelerated away by<br />
the electric field that has created them [123, 124].<br />
Cesium, whose melting point is about 29 ◦C, has been chosen as propellant because of its<br />
low work function, high atomic mass and good properties of wetting on steel surfaces.<br />
The basic FEEP system comprises: a single solid emitter/accelerator system or a cluster<br />
of them, a storage and feed system for the Cs propellant, a power conditioning and control<br />
unit, and a neutralizer (Figure 7.5).<br />
3-3-1999 9:33 Corrected version 2.08