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STAR*NET V6 - Circe

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6.5 Preanalysis<br />

Chapter 6 Running Adjustments<br />

When you choose Run>Preanalysis, <strong>STAR*NET</strong> processes the network using a list of<br />

approximate coordinates for all stations supplied by you, and a list of observation codes<br />

to indicate which distances, angles, and other field data will be observed. No actual field<br />

observation data is required. <strong>STAR*NET</strong> will analyze the geometric strength of the<br />

network using your approximate layout and the instrument accuracies supplied as<br />

observation standard errors. The predicted accuracy of each station will be computed,<br />

and error ellipses generated.<br />

# Approximate coordinates for proposed survey<br />

#<br />

C 1 51002 101009 ! !<br />

C 2 51005 101343<br />

C 3 51328 101291<br />

C 4 51416 101073<br />

#<br />

# Proposed Observations<br />

#<br />

4<br />

D 1-2<br />

D 2-3<br />

ANGLE<br />

D 3-4<br />

D 4-1<br />

D 1-3<br />

A 2-1-3<br />

A 3-2-4<br />

A 4-3-1<br />

A 1-4-2<br />

A<br />

#<br />

1-4-3<br />

# Fixed Bearing<br />

#<br />

ANG<br />

B 1-2 ? !<br />

1<br />

D IS TA N C E<br />

Sample Preanalysis Data<br />

The example above shows a very small Preanalysis data file. It is important to note that<br />

approximate coordinates are required for all stations, to indicate roughly where survey<br />

points are planned. The distance and angle lines show which observations are planned.<br />

Observation standard errors default to the global values for each data type. If an explicit<br />

standard deviation is required, for example to fix a bearing as shown in the sample data<br />

above, use the “?” character as a place holder for the unknown data. An example in<br />

Appendix-A, the <strong>STAR*NET</strong> Tour, provides another, somewhat larger, sample<br />

Preanalysis data set.<br />

106<br />

ANGLE<br />

D IS TA N C E<br />

D IS T A N C E<br />

B E A R IN G<br />

D IS TA N C E<br />

ANGLE<br />

ANGLE<br />

3<br />

D ISTA N C E<br />

2

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