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Pre-Phase A Report - Lisa - Nasa

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94 Chapter 4 Measurement Sensitivity<br />

The charge build up will be the result of the random arrival of cosmic rays, with each<br />

‘hit’ depositing a variable amount of charge according to the stochastic nature of the<br />

interaction process. Following an argument similar to that already used for Lorentz force<br />

noise it turns out that the acceleration noise arising from this process can be approximated<br />

by<br />

<br />

˙ne f −1 (m s −2 / √ Hz ) . (4.17)<br />

ãn =10 −29.9 ne<br />

In order to keep this acceleration noise below its budget allocation the amount of accumulated<br />

charge must controlled such that<br />

ne ≤ 2×10 13 <br />

f<br />

f 1+<br />

3×10−3 <br />

2<br />

electrons/protons. (4.18)<br />

This limit is much less severe than that from the Lorentz force noise. It has been based<br />

on a 1 µm ‘asymmetry’ assumption. Whether this is a reasonable figure to use remains to<br />

be confirmed.<br />

Another source of acceleration noise which will occur if the proof mass becomes charged is<br />

through displacement noise modifying the electrostatic force. There are two components<br />

(arising from the second term in equation 4.15) due to changes in the total capacitance<br />

and in the asymmetry factor, which in turn affects the capacitance gradients. Adding<br />

these two in quadrature gives an acceleration noise (for the displacement type sensor<br />

geometry)<br />

ãn = Q2<br />

mC 2<br />

∂C<br />

∂k<br />

<br />

1 1<br />

+<br />

4δk2 C2 2 ∂C<br />

˜kn (m s<br />

∂k<br />

−2 / √ Hz ) , (4.19)<br />

where ˜ kn is the spatial displacement noise spectral density and all other symbols retain<br />

their earlier meanings. Putting in the numericalvalues for the LISA sensor design and<br />

using ˜ kn =10 −9 m/ √ Hz gives ãn =1.8×10 −33 n 2 e ms−2 / √ Hz .<br />

The final noise source which will be discussed in this section arises from the interaction<br />

between any free charges on the proof mass and the applied control voltages, Vi, andany<br />

associated voltage noise, Vni. Using the third term in equation 4.15 this noise component<br />

is given by<br />

a 2 n = Q2<br />

m2C 2<br />

<br />

n<br />

∂Ci<br />

Vni<br />

∂k<br />

i=1<br />

2<br />

+ Q2<br />

m2C 4<br />

<br />

n<br />

Vi<br />

i=1<br />

<br />

2<br />

2<br />

∂Ci<br />

k<br />

∂k<br />

2 n (m 2 s −4 / √ Hz ) . (4.20)<br />

The electrostatic forces which come about through the proof mass becoming charged<br />

bring with them associated effective spring constants. There are three effects, two of<br />

which involve the applied potentials and one which does not, which have been considered.<br />

The two involving the applied potentials are given by terms of the form |K| ≈ QVcm<br />

and |K| ≈ 2QVcm<br />

C<br />

4ɛA<br />

C g3 ∂2Ci ∂k2 ,whereVcm and Vdm are the voltages applied in common mode and<br />

differential mode to electrodes on opposite sides of the proof mass. The second of these<br />

two spring constant terms is the most significant for the current sensor design. The spring<br />

constant term arising out of pure electrostatic interaction with the surrounding conducting<br />

surfaces is of the form (for displacement type sensor geometries) |K| ≈ Q2<br />

2C<br />

4ɛA<br />

g 3 .Thisterm<br />

3-3-1999 9:33 Corrected version 2.08

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