first example. The second example gives worse
results, since there are less points and the
turbolence is higher.
Table 4.1- Spatial analysis of turbolent flow fields (unit: mm)
1st example (n - 811) 2nd example (n = 452)
X y zZ X y z
- a priori standard deviation: 2315 . 206 .286 «248 . 348 .348
- 2nd order polynomial interpolation:
a posteriori sigma naught .205 . 145 4259 -205 .208 . 344
- covariance functions: (NS) (ES) (ES) (NS) (NS) (ES)
(insignificant crosscovariances)
a priori variance of the signal .144 .106 „142 4156 .148 . 149
a priori variance of the noise „120 . 084 „174 . 104 „120 . 246
best correlation coefficient 58% 54% 28% 68% 58% 24%
optimal radius 10 10 10 5 5 5
correlation length 30 20 10 20 15 10
"Zero point" 100 100 100 50 50 50
number of blunders (« = 1%) 26 26 20 12 15 15
- collocation filtering:
a posteriori variance of the signal . 145 :091 . 087 . 164 . 154 . 124
a posteriori variance of the noise „114 .076 . 183 .094 115 . 266
estimation error . 066 . 060 „112 :079 . 086 - 125
number of outliers (œ = 5%) 38 36 33 25 34 41
trimmed variance of the noise . 094 . 064 „148 . 073 . 092 . 185
- finite element method by using tricubic splines:
interpolation step 50 25 50 25 15
number of knots 44 192 24 60 132
a posteriori sigma naught x „152 . 123 «177 „153 . 128
y 2193 „109 -189 .160 „133
„253 . 224 „336 . 326 „316
APPENDIX Note that it is necessary to perform preceding
separate adjustments.Indeed the covariance matrix
Least squares collocation with stochastic - and of the signal Cats obtained from estimates for
non-stochastic parameters the unknown parameters or residuals; moreover the
variance of the noise o is assumed equal to the
(This appendix presents a development of basic sigma naught square obtained in the last preceding
ideas of Barzaghi et al., 1988; and is quoted with separate adjustment.
minor changes from Crippa/de Haan/Mussio, 1989). The use of both stochastic and non-stochastic
parameters causes the need to introduce a hybrid
In the above mentioned procedure different systems norm:
are solved successively. In the integrated geodesy
approach all systems are solved simultaneously.
Thus after the linearization of the observation c 0 S
and pseudo-observation equations, the observables 1176 7t ss t AS a A o 3
> - n + A (Ax t Bs — - =
and the other data « are collected in a unique zs (Ax S n g min
m
system containing uncorrelated unknowns x as well 0 P/o?
as correlated unknowns that can be interpreted as n
stochastic signal s to filter from the random
noise n: o = A
where « indicates the observations, x, s and n the
estimated values of x, s and n respectively, P the
œ = Ax * Bs weight matrix of the observations and A a vector
of Lagrange multipliers.
386