|Palm Globe, version 1.10||13 Nov 1998|
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When distance calculations are carried out, the pen position can only be determined to the nearest pixel (picture element) on the screen. The longitude and latitude is then reported as being at the center of that pixel. However, more accurate positions can be entered by using the Tap button in the Viewpoint dialog, which simulates a pen tap at the exact point specified.
Distances are then calculated between the two coordinates selected and should be accurate to the nearest unit (km or mile), or 0.2%, whichever is greater. The 0.2% limit is a consequence of the assumption used in the calculation that the earth is spherical (which it is not).
Time and sun position calculations are only important when the Sunlight option is selected. In this case, Palm Globe needs to know the current date and time-of-day (taken from your computer's clock -- make sure it is set correctly). It also needs to know which time zone that clock is set to: you will have been asked for this when Palm Globe was first started (you may also need to change it if your computer clock changes for daylight saving, summer, or winter time).
From the current time and time zone information, Palm Globe can determine the apparent solar time (which is as much as 16 minutes different from the Civil time used for clocks) and hence the sun's position. This is then used to display the globe as though lit by the sun: the light/dark dividing line thus shows where the sun is rising or setting.
The various calculations done should give an accuracy of sun position that leads to a sunset or sunrise indication that is correct to within twenty seconds of time. Actual sunset or sunrise times will be a little different because of atmospheric effects, which vary with the time of year, the weather, and latitude. However, Palm Globe does give a useful indication of sunrise and sunset, and of course lets you see at a glance which parts of the globe are in night or daylight.
Celestial events such as equinoxes, and solstices especially, are very dependent on the earth's movements; equinoxes should be correct within some tens of minutes, solstices should be correct within about ten hours.
Please note that results will be incorrect if you set your computer's date to be earlier than 1 January 1990. Also, the formulae used to calculate the sun's position may prove to be inaccurate at some distant time in the future, because the earth's movement is not entirely predictable.