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STAR*NET V6 - Circe

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6.4 Blunder Detect<br />

Chapter 6 Running Adjustments<br />

This is a modified form of adjustment that can be used to find various types of blunders<br />

in your input data file. Choose Run>Blunder Detect to run this routine. Blunder Detect<br />

is never used in place of a normal adjustment, it is a data debugging tool only! When you<br />

run Blunder Detect, a modified version of the listing file is generated. Your listing file<br />

will contain a section entitled “Differences from Observations” for each data type. In the<br />

example shown below, the best fit angles are listed in the Angle column, followed by<br />

their differences from the input values. The largest difference is listed at the end of each<br />

data type. Or, if you have chosen in the listing options to have output observations sorted<br />

by residual size, your output will be sorted by observations having the largest differences<br />

shown first.<br />

Differences From Observations<br />

=============================<br />

Differences from Observed Angles<br />

At From To Angle Difference<br />

3 4 5 153-38-56.31 1-00-17.19<br />

9 1 7 159-51-49.11 0-00-00.76<br />

11 10 12 4-59-09.78 -53-00-35.34<br />

15 14 16 42-48-09.82 0-00-05.68<br />

Largest Difference from Observed Angle<br />

11 10 12 4-59-09.78 -53-00-35.34<br />

Blunder Detect<br />

Blunder Detect functions by performing several iterations, successively deweighting<br />

observations that do not fit into the network in an attempt to isolate those observations<br />

that contain blunders. The routine works best in a situation where you have a strong,<br />

over-determined network. This means that you should have as many redundant distances<br />

and angles as possible. The Blunder Detect routine will be of little or no help in<br />

determining blunders in simple traverses. To utilize Blunder Detect is a strong argument<br />

for collecting additional field data wherever possible. If you can tie across traverses to<br />

another stations, or observe angles to distant stations in the network, your chances of<br />

detecting gross errors are much improved. Of course, you will also improve the<br />

adjustment results.<br />

Using the Blunder Detect routine can be very effective under certain circumstances in<br />

locating multiple gross errors in your input data. However it is not useful in analyzing<br />

survey networks that contain the normal small random errors present in all field<br />

measurements. You should not run Blunder Detect “just to see if things are OK”,<br />

because it may give you misleading indications of problems when there are none. You<br />

should reserve its use for those cases where you have a number of large residuals in your<br />

input data you cannot account for.<br />

105

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