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- The Time Variable
-
-
- The program aims at providing the position of
- celestial bodies for a certain point in time and as seen
- from a certain location; therefore, information relative to
- this particular instant and this location has to be provided
- by the user.
-
- Year, month and day are entered according to
- normal practice. The calendar used is the Julian calendar
- for dates until October 5, 1582, and the Gregorian calendar
- afterwards.
-
- The time of the day is entered as "hour min"
- counted from midnight (hence 14h = 2 p. m.). The time scale
- is either Ephemeris Time, Universal Time, Mean Local Time,
- Standard Time (for wich you have to provide the Time Zone)
- or Sundial Time.
-
- Geographical longitude and latitude are entered as
- decimal angles (DDD.dd). "M" can also be used; this was an
- ancient way to determine latitude, by the ratio of the hours
- of daylight to twelve hours at the summer solstice. If "M"
- is not available, just enter two dashes "--". If "M" is
- available and entered, it will override the geographical
- latituded entered earlier.
-
- Finally, you might want to enter a note of some
- sort for future reference if a printout of the screen is
- needed.
-
- The program will display on a single screen the
- information already entered, plus a number of time
- conversions and other related information.
-
- All input data provided by the user are kept into
- memory for further runs of the program. If one wishes, one
- can go over again the input data routine and change only
- selected variables.
-