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PhD thesis - Institute for Space Research - University of Calgary

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3.2.5: Geometric factor 43<br />

∆h<br />

∆α<br />

R s<br />

R o<br />

θ i<br />

x<br />

Figure 3.9: Symbols and layout <strong>for</strong> calculation <strong>of</strong> ∆α aperture.<br />

where f pixel can be determined by Monte Carlo analysis. For the present<br />

calculation I assume f pixel ≃ 1. The aperture area is approximated by<br />

the projection <strong>of</strong> the surface area <strong>of</strong> a cylinder with radius R s and height<br />

∆h onto a plane. This gives<br />

A aperture ≈ 2R s ∆h. (3.25)<br />

Equation 3.14 can be used to put r in term <strong>of</strong> E i :<br />

r =<br />

( ) 1<br />

Ei b<br />

. (3.26)<br />

a 1<br />

Substituting these into the expression <strong>for</strong> the geometric factor gives<br />

G pixel ≈ 2(∆r) 2 (∆h) 2<br />

a 2 b<br />

1 + Ro 1 bE b−2<br />

b<br />

i . (3.27)<br />

R s<br />

cos θ i<br />

Recalling that a 1 = −q∆V a, <strong>for</strong> simplicity I let a 1 = a 2 ∆V , where<br />

a 2 = −qa. The geometric factor takes the final <strong>for</strong>m<br />

G pixel ≈ 2b<br />

(∆r∆h)2 (a 2 ∆V ) 2 b−2<br />

b E<br />

b<br />

1 + Ro<br />

i . (3.28)<br />

R s<br />

cos θ i<br />

It has the properties that it is proportional to the square <strong>of</strong> the pixel<br />

size, (∆r) 2 , and the square <strong>of</strong> the aperture width, (∆h) 2 , which make<br />

sense. These properties are shared with the top-hat analyzer.

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