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Solar-powered space flight

7c. Achieving the desired level of optical precision: Examples

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7.5          For mirror layouts as per Figures 9 and 10 then  are as per Table 6 for a range of well spread out values of . We note that in the situation where  and  is constant for all  (for a given ), i.e.  and  can be ignored, the following apply:

 

(a)    For small , the terms in  and  predominate, and as we might expect have the desired signs, i.e. they involve the wires pulling the mirror along in the direction of the negative x-axis and radially inwards.

 

(b)   For any given , the terms in  and  still predominate for sufficiently large . This means that sufficient tension to achieve a smooth reflective surface can always in principle be achieved as long as  is large enough.

 

Table 6: Values of  arising from ,  and  for various

 

0.999

-1.43

-1.05

-1.51

1.05

-1.05

0.31

-0.95

0.99

0.04

-1.05

-1.05

1.06

-1.04

0.31

-0.95

0.95

0.48

-1.05

-0.95

1.11

-1.00

0.31

-0.95

0.90

0.57

-1.05

-0.99

1.17

-0.94

0.30

-0.95

0.81

0.62

-1.04

-1.11

1.29

-0.84

0.28

-0.96

0.70

0.66

-1.03

-1.31

1.47

-0.72

0.24

-0.97

0.62

0.68

-1.02

-1.51

1.66

-0.63

0.22

-0.98

0.52

0.69

-1.02

-1.81

1.94

-0.53

0.19

-0.98

0.4

0.70

-1.01

-2.31

2.42

-0.42

0.15

-0.99

0.30

0.72

-1.01

-3.26

3.34

-0.30

0.11

-0.99

 

 

If, say,  =  kg m-3,  = 1 MPa  (so  is roughly 8 – 14 MPa during flight),  = 0.01 and  = 200 m then ,  and  (and if there is a single stanchion per mirror area element, ) are as per Table 7 for various values of . The above values of ,  etc. have been chosen to be akin to those that might arise when lifting a reasonably modest payload into orbit. We note that  and  have the desired signs as per (i) for all relevant . As long as the stanchions are sufficiently close together the tension will vary only a little in the regions between stanchions, making it possible in principle to achieve the desired level of optical accuracy. Some cross buttressing might also be desirable, to limit vibration of the mirror during flight, unless a particularly smooth acceleration is delivered by the engine.

 

Table 7: ,  and hence  as multiples of  (and hence angle, , that a single cross-stanchion should make to the x-axis) needed in order to achieve uniform tension in larger mirror for a hypothetical mirror example

 

 ()

 ()

 ()

 ()

0.999

-17.6

-23.3

29.2

52.9

0.99

-10.3

-20.8

23.2

63.6

0.95

-8.1

-19.2

20.8

67.1

0.90

-7.6

-17.9

19.4

66.9

0.81

-7.3

-15.9

17.5

65.4

0.70

-7.0

-13.6

15.3

62.7

0.62

-6.9

-11.9

13.8

60.1

0.52

-6.7

-10.0

12.1

56.1

0.41

-6.6

-7.9

10.3

50.2

0.30

-6.5

-5.7

8.6

41.2

 


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