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| Miller compensates for the interferometer drift or slope over each page, ie 20 turns. | Miller compensates for the interferometer drift or slope over each page, ie 20 turns. | ||
| - | Advantage calculation are on single page. | + | Advantage calculation are on single page. see p214 |
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| + | The purpose of this test is to find the | ||
| + | effect of slope on the sin[ ] component in an interval of 2 Pi. | ||
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| + | === FindFit Approach === | ||
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| + | See ApexMeansTest.nb | ||
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| + | Fourier analysis assumes that a signal repeats on some fixed cycle. If a signal does not do this, then FA cannot be used. At least without closing the cycle or the like. | ||
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| + | This program shows that when the " | ||
| + | This means that the linear term "c x" completely prevents the linear slope from affecting the true Sin[ ] component. | ||
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| + | also to find out how to structure data for FindFit | ||
| + | " | ||
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| + | <code mathematica> | ||
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| + | Clear[x, | ||
| + | imax=20; | ||
| + | x2=Table[i/ | ||
| + | Print[" | ||
| + | |||
| + | a1=1.01; b1=25; c1=10; | ||
| + | xy= Table[{x1/ | ||
| + | Print[" | ||
| + | |||
| + | ff=FindFit[xy, | ||
| + | Print[" | ||
| + | Print[" | ||
| + | |||
| + | x {0.5, | ||
| + | xy {{0.5, | ||
| + | angles {0.314159, | ||
| + | ff {a-> | ||
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| + | |||
| + | </ | ||
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| + | === First approach. === | ||
| I could do the same over whole day: 24h * 60t/h = 1440 turns. | I could do the same over whole day: 24h * 60t/h = 1440 turns. | ||
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| This would cause a daily cycle in the interferometric sin component, albeit 1/1440 as large each day. | This would cause a daily cycle in the interferometric sin component, albeit 1/1440 as large each day. | ||
| - | Or even entire set of days in name-list. | + | Or even an entire set of days in name-list. |
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| + | Effect of slope on sin[ ] in interval 2 Pi. | ||
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