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  1. RiseSet :: a -> a -> RiseSet a

    astro Data.Astro.CelestialObject.RiseSet

    Some Info of Rise and Set of the celestial object

  2. type RiseSetLCT = RiseSet RSInfo LocalCivilTime

    astro Data.Astro.CelestialObject.RiseSet

    Local Civil Time and Azimuth of Rise and Set

  3. type RiseSetLST = RiseSet RSInfo LocalSiderealTime

    astro Data.Astro.CelestialObject.RiseSet

    LST (Local Sidereal Time) and Azimuth of Rise and Set

  4. type RiseSetMB = RiseSet Maybe RSInfo LocalCivilTime

    astro Data.Astro.CelestialObject.RiseSet

    The optional Rise And optinal Set Information (LocalCivilTime and Azimuth)

  5. riseAndSet :: EquatorialCoordinates1 -> DecimalDegrees -> DecimalDegrees -> RiseSetLST

    astro Data.Astro.CelestialObject.RiseSet

    Calculate rise and set local sidereal time of a celestial object. It takes the equatorial coordinates of the celestial object, vertical shift and the latitude of the observation. To calculate vertical shift for stars use function refract from Data.Astro.Effects. In most cases you can assume that vertical shift equals 0.566569 (34 arcmins ~ 'refract (DD 0) 12 1012').

  6. riseAndSet2 :: DecimalHours -> (JulianDate -> EquatorialCoordinates1) -> GeographicCoordinates -> DecimalDegrees -> LocalCivilDate -> RiseSetMB

    astro Data.Astro.CelestialObject.RiseSet

    Calculate rise and set local sidereal time of a celestial object that changes its equatorial coordinates during the day (the Sun, the Moon, planets). It takes epsilon, the function that returns equatorial coordinates of the celestial object for a given julian date, vertical shift and the latitude of the observation. To calculate vertical shift for stars use function refract from Data.Astro.Effects. In most cases you can assume that vertical shift equals 0.566569 (34 arcmins ~ 'refract (DD 0) 12 1012').

  7. riseAndSetLCT :: GeographicCoordinates -> LocalCivilDate -> DecimalDegrees -> EquatorialCoordinates1 -> RiseSetLCT

    astro Data.Astro.CelestialObject.RiseSet

    Calculates set and rise of the celestial object It takes geographic coordinates of the observer, local civil date, vertical shift and equatorial coordinates of the celestial object.

  8. toRiseSetLCT :: DecimalDegrees -> LocalCivilDate -> RiseSetLST -> RiseSetLCT

    astro Data.Astro.CelestialObject.RiseSet

    Converts Rise and Set in Local Sidereal Time to Rise and Set in Local Civil Time. It takes longutude of the observer and local civil date. To calculate vertical shift for stars use function refract from Data.Astro.Effects. In most cases you can assume that vertical shift equals 0.566569 (34 arcmins ~ 'refract (DD 0) 12 1012').

  9. data RiseSet a

    astro Data.Astro.Sun

    Some Info of Rise and Set of a celestial object

  10. RiseSet :: a -> a -> RiseSet a

    astro Data.Astro.Sun

    Some Info of Rise and Set of the celestial object

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