STAR*NET V6 - Circe
STAR*NET V6 - Circe
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 />
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