Intercept method: Difference between revisions

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'''Bold text'''The "Intercept Method", or "Marcq St Hilaire method", as it is also rather inaccurately kn'''ownknown, is an astronomical [[navigation]] method of calculating an observer's position on earth. It was originally called the ''azimuth intercept'' method because the process involves drawing a line which intercepts the azimuth line. This name was shortened to ''intercept'' method and the ''intercept distance'' was shortened to "intercept".

The method yields a line of position (LOP) on which the observer is situated. The intersection of two or more such lines will define the observer's position, called a "fix". Sights may be taken at short intervals, usually during hours of twilight, or they may be taken at an interval of an hour or more (as in observing the Sun during the day). In either case, the lines of position, if taken at different times, must be advanced or retired to correct for the movement of the ship during the interval between observations. If observations are taken at short intervals, a few minutes at most, the corrected lines of position by convention yield a "fix". If the lines of position must be advanced or retired by an hour or more, convention dictates that the result is referred to as a "running fix".

'''[[File:Example.jpg]]

== Summary ==

The intercept method is based on the following principle.