Pre-Phase A Report - Lisa - Nasa
Pre-Phase A Report - Lisa - Nasa
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