NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
From: Andrés Ruiz
Date: 2009 Oct 8, 08:16 +0200
Antoine is right in saying: “Only the presence
of higher order terms (in t**4 and maybe t**6) prevented Andres to do the
perfect pick of the exact Culmination time.”
I have simulated two theoretical
cases with very high speed, and the curve obtained for the altitude near
meridian transit is like this:
R=180º
V=3000 kt
R=135º
V=3000 kt
In this case the least squares
fit gives for Hmax:
yLS =
a0+a1*x+a2*x2+a3*x3+...+anxn
a0 = -51168.479530
a1 = 4885.116188
a2 = 118.025783
a3 = -20.281600
a4 = 0.107351
a5 = 0.025145
a6 = -0.000455
x |
y |
yLS |
y - yLS |
ErrorRel_y |
ErrorRel_yLS |
17.508889 |
53.34053 |
53.178178 |
0.162352 |
0.30437 |
0.305299 |
And the solution is:
R |
V |
|
UT1 |
B |
L |
GHA |
Dec |
LHA |
H |
Z |
|
UT1 |
tTransit-tMax |
135 |
3000 |
Transit: |
17.0775 |
21.4216279 |
-76.4695651 |
76.471408 |
-23.434998 |
0.00184292 |
45.1433741 |
180.002397 |
|
17:04:39 |
|
135 |
3000 |
Hmax: |
17.5088889 |
6.16972746 |
-60.8005176 |
82.9400037 |
-23.4348594 |
22.1394861 |
53.3405304 |
215.389641 |
|
17:30:32 |
0:25:53 |
Andrés Ruiz
Navigational Algorithms
http://sites.google.com/site/navigationalalgorithms/
Asunto: [NavList 10061] Re: Time of meridian passage
accuracy
...
I am quite surprised by these results because for
culminations close to zenit (say above 85d) the effect of a high N/S speed
component and/or change in declination significantly skews the heights vs times
curve. Given the almost perfect symmetry of this Altitude curve, the algorithm
used by Andres - apparently a second degree best fit as seems to be indicated
on his site - was very powerful to pick up almost the exact the Culmination
time. Only the presence of higher order terms (in t**4 and maybe t**6)
prevented Andres to do the perfect pick of the exact Culmination time.
...
Antoine M. "Kermit" Couette
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