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STAR*NET V6 - Circe

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Chapter 4 OPTIONS<br />

4.1 Overview<br />

<strong>STAR*NET</strong> maintains a list of settings for each job called “Project Options.” Most of<br />

these options are settings and values that control how <strong>STAR*NET</strong> processes an<br />

adjustment, and they are set by the user in dialogs discussed on the following pages.<br />

Other stored settings relate to the contents of plotting diagrams and DXF exports.<br />

<strong>STAR*NET</strong> stores the options for a project by creating a file named “PROJECT.PRJ,”<br />

where “PROJECT” is the name of the project, for example, SouthPark.prj. All project<br />

specific options are saved in this file. If you open an existing project at a later date, those<br />

options automatically load and will remain in effect until you change them.<br />

A special “default options” file is located in the directory you installed <strong>STAR*NET</strong>. It is<br />

referred to as the Company options file; its real name is STAR6.DEF. It is automatically<br />

created when run <strong>STAR*NET</strong> for the first time after installing the program. It initially<br />

contains a set of generic defaults you should change to settings more typical of your<br />

projects. These typical option settings will be applied automatically to any new project.<br />

Setting the Company options will be discussed later in this chapter.<br />

When you have a single project that requires several different weighting schemes<br />

(different instruments used, or combining an old survey with a new survey), you can<br />

store several sets of instrument standard error values in a special “Instrument Library”.<br />

This information may be saved in the Company options file for use in any project, or in<br />

the project’s own “PRJ” file for use only by that project. Using special “inline” codes,<br />

these settings can be referenced anywhere in the data files to change the weighting<br />

scheme of subsequent observations. Using the Instrument Library is discussed in detail<br />

later in this chapter.<br />

13

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