gistfile1.txt

//
//  
//	NTSolar.swift
//
//  Created by Neil Tiffin on 5/8/19.
//  Copyright © 2019 Performance Champions, Inc.
//  Copyright © 2019 Neil Tiffin.
//
//  Released to the public domain by Neil Tiffin, May 2019
//  Released to the public domain by Performance Champions, Inc., May 2019
//

import Foundation
import CoreLocation

/// Class to calculate sunrise sunset.
///
/// C code originally from: [http://stjarnhimlen.se/comp/sunriset.c](http://stjarnhimlen.se/comp/sunriset.c)
class NTSolar {

    // MARK: - Public Swift Interface

    /// Calculate the sun rise and set times.
    ///
    /// - Parameters:
    ///   - forDate: The date for the calculation. You should ensure that the date, which is stored as UTC, is the date
    ///         really wanted in the given time zone. It will be converted to the given time zone before being used.
    ///   - atLocation: The latitude and longitude for the calculation.
    ///   - inTimeZone: The time zone for the resulting date and times.
    /// - Returns: If the sun both rises and sets on the day requested and at the
    ///     latitude requested then return sun rise and set times rounded down to the minute, nil othewise.
    class func sunRiseAndSet(forDate: Date,
                             atLocation: CLLocationCoordinate2D,
                             inTimeZone: TimeZone) -> (sunrise: Date, sunset: Date)? {
        
        var calendar = Calendar(identifier: .gregorian)
        calendar.timeZone = inTimeZone
        var comp = calendar.dateComponents([.day, .year, .month], from: forDate)
        comp.calendar = calendar

        guard let year = comp.year,
            let month = comp.month,
            let day = comp.day else {
                gLog.error("Failed to find date components.")
                return nil
        }

        let (riseUTC, setUTC, code) = NTSolar.sun_rise_set(year: year,
                                                           month: month,
                                                           day: day,
                                                           lon: atLocation.longitude,
                                                           lat: atLocation.latitude)

        if code != .RiseAndSet {
            gLog.error("Failed to find rise and set.")
            return nil
        }

        // Calc sunrise
        var riseLocalHrs = riseUTC + (Double(inTimeZone.secondsFromGMT()) / 3600.0)
        if riseLocalHrs > 24.0 {
            riseLocalHrs -= 24.0
        }
        let riseHoursInt = Int(riseLocalHrs)
        comp.hour = riseHoursInt

        comp.minute = Int(  (( riseLocalHrs - Double(riseHoursInt) ) * 60.0).rounded() )
        comp.second = 0
        comp.nanosecond = 0
        guard let riseTime = comp.date else {
            gLog.error("\nFailed to calculate rise time hrs: \(riseLocalHrs).\n\(comp)\n")
            return nil
        }

        // Calc sunset
        var setLocalHrs = setUTC + (Double(inTimeZone.secondsFromGMT()) / 3600.0)
        if setLocalHrs > 24.0 {
            setLocalHrs -= 24.0
        }
        let setHoursInt = Int(setLocalHrs)
        comp.hour = setHoursInt
        comp.minute = Int( ((setLocalHrs - Double(setHoursInt) ) * 60.0).rounded() )
        comp.second = 0
        comp.nanosecond = 0
        guard let setTime = comp.date else {
            gLog.error("\nFailed to calculate set time hrs: \(setLocalHrs).\n\(comp)\n")
            return nil
        }

        return (riseTime, setTime)
    }

    // MARK: - SUNRISET.C

    // C code originally from: [http://stjarnhimlen.se/comp/sunriset.c](http://stjarnhimlen.se/comp/sunriset.c)
    //
    // The conversion process removed pointers in favor of return tuples, converted macros to function calls,
    // added return code enum, and converted
    // comments to work with Xcode.  Of course the C code had to be converted to Swift, but that was minimal.
    //
    // As much as possible the original code was left intact in order to not introduce bugs.
    // In other words, some code was left unfashionable by today's standards.

    enum ReturnCode: Int {
        /// Sun is below the specified "horizon" 24 hours
        /// "Day" length = 0 hours, trise and tset are
        /// both set to the time when the sun is at south.
        case SunAlwaysBelow = -1

        /// Sun rises/sets this day, times stored at rise and set.
        case RiseAndSet = 0

        /// Sun above the specified "horizon" 24 hours.
        /// trise set to time when the sun is at south,
        /// minus 12 hours while tset is set to the south
        /// time plus 12 hours. "Day" length = 24 hours
        case SunAlwaysAbove = 1
    }

    /* +++Date last modified: 05-Jul-1997 */
    /* Updated comments, 05-Aug-2013 */
    /*
     SUNRISET.C - computes Sun rise/set times, start/end of twilight, and
     the length of the day at any date and latitude

     Written as DAYLEN.C, 1989-08-16

     Modified to SUNRISET.C, 1992-12-01

     (c) Paul Schlyter, 1989, 1992

     Released to the public domain by Paul Schlyter, December 1992
     */

    /// A macro to compute the number of days elapsed since 2000 Jan 0.0
    /// (which is equal to 1999 Dec 31, 0h UT)
    private class func days_since_2000_Jan_0(y:Int, m:Int, d:Int) -> Int {
        return (367*(y)-((7*((y)+(((m)+9)/12)))/4)+((275*(m))/9)+(d)-730530)
    }

    /* Some conversion factors between radians and degrees */
    private static let PI  =      3.1415926535897932384
    private static let RADEG   =  ( 180.0 / PI )
    private static let DEGRAD  =  ( PI / 180.0 )

    /* The trigonometric functions in degrees */
    private class func sind(x: Double) -> Double  { return sin((x)*DEGRAD) }
    private class func cosd(x: Double) -> Double  { return  cos((x)*DEGRAD) }
    private class func tand(x: Double) -> Double  { return  tan((x)*DEGRAD) }
    private class func atand(x: Double)  -> Double  { return   (RADEG*atan(x)) }
    private class func asind(x: Double)  -> Double  { return   (RADEG*asin(x)) }
    private class func acosd(x: Double)  -> Double  { return   (RADEG*acos(x)) }
    private class func atan2d(y: Double,x: Double)-> Double  { return  (RADEG*atan2(y,x)) }

    /* Following are some macros around the "workhorse" function __daylen__ */
    /* They mainly fill in the desired values for the reference altitude    */
    /* below the horizon, and also selects whether this altitude should     */
    /* refer to the Sun's center or its upper limb.                         */


    /** This macro computes the length of the day, from sunrise to sunset. */
    /** Sunrise/set is considered to occur when the Sun's upper limb is    */
    /** 35 arc minutes below the horizon (this accounts for the refraction */
    /** of the Earth's atmosphere).                                        */
    class func day_length(year: Int, month: Int, day: Int, lon: Double, lat: Double) -> Double {
        return daylen( year: year, month: month, day: day, lon: lon, lat: lat, altit: -35.0/60.0, upper_limb: 1 )
    }

    /** This macro computes the length of the day, including civil twilight. */
    /** Civil twilight starts/ends when the Sun's center is 6 degrees below  */
    /** the horizon.                                                         */
    class func day_civil_twilight_length(year: Int, month: Int, day: Int, lon: Double, lat: Double) -> Double {
        return daylen( year: year, month: month, day: day, lon: lon, lat: lat, altit: -6.0, upper_limb: 0 )
    }

    /** This macro computes the length of the day, incl. nautical twilight.  */
    /** Nautical twilight starts/ends when the Sun's center is 12 degrees    */
    /** below the horizon.                                                   */
    class func day_nautical_twilight_length(year: Int, month: Int, day: Int, lon: Double, lat: Double) -> Double {
        return daylen( year: year, month: month, day: day, lon: lon, lat: lat, altit: -12.0, upper_limb: 0 )
    }

    /** This macro computes the length of the day, incl. astronomical twilight. */
    /** Astronomical twilight starts/ends when the Sun's center is 18 degrees   */
    /** below the horizon.                                                      */
    class func day_astronomical_twilight_length(year: Int, month: Int, day: Int, lon: Double, lat: Double) -> Double {
        return daylen( year: year, month: month, day: day, lon: lon, lat: lat, altit: -18.0, upper_limb: 0 )
    }

    /** This macro computes times for sunrise/sunset.                      */
    /** Sunrise/set is considered to occur when the Sun's upper limb is    */
    /** 35 arc minutes below the horizon (this accounts for the refraction */
    /** of the Earth's atmosphere).                                        */
    class func sun_rise_set(year: Int, month: Int, day: Int , lon: Double, lat: Double) -> (trise: Double, tset: Double, code: ReturnCode) {
        let (start, end, code) = sunriset( year: year, month: month, day: day, lon: lon, lat: lat, altit: -35.0/60.0, upper_limb: 1)
        return (start, end, code)
    }

    /** This macro computes the start and end times of civil twilight.       */
    /** Civil twilight starts/ends when the Sun's center is 6 degrees below  */
    /** the horizon.                                                         */
    class func civil_twilight(year: Int, month: Int, day: Int, lon: Double, lat: Double) -> (trise: Double, tset: Double, code: ReturnCode) {
        let (start, end, code) = sunriset( year: year, month: month, day: day, lon: lon, lat: lat, altit: -6.0, upper_limb: 0)
        return (start, end, code)
    }

    /** This macro computes the start and end times of nautical twilight.    */
    /** Nautical twilight starts/ends when the Sun's center is 12 degrees    */
    /** below the horizon.                                                   */
    class func nautical_twilight(year: Int, month: Int ,day: Int, lon: Double, lat: Double) -> (trise: Double, tset: Double, code: ReturnCode) {
        let (start, end, code) = sunriset( year: year, month: month, day: day, lon: lon, lat: lat, altit: -12.0, upper_limb: 0)
        return (start, end, code)
    }

    /** This macro computes the start and end times of astronomical twilight.   */
    /** Astronomical twilight starts/ends when the Sun's center is 18 degrees   */
    /** below the horizon.                                                      */
    class func astronomical_twilight(year: Int, month: Int, day: Int, lon: Double, lat: Double) -> (trise: Double, tset: Double, code: ReturnCode) {
        let (start, end, code) = sunriset( year: year, month: month, day: day, lon: lon, lat: lat, altit: -18.0, upper_limb: 0)
        return (start, end, code)
    }

    /// The "workhorse" function for sun rise/set times
    ///
    /// - Parameters:
    ///   - year: calendar date, 1801-2099 only.
    ///   - month: calendar date, 1801-2099 only.
    ///   - day: calendar date, 1801-2099 only.
    ///   - lon: Eastern longitude positive, Western longitude negative. The longitude value IS critical in this function!
    ///   - lat: Northern latitude positive, Southern latitude negative
    ///   - altit: the altitude which the Sun should cross. Set to -35/60 degrees for rise/set, -6 degrees
    ///       for civil, -12 degrees for nautical and -18 degrees for astronomical twilight.
    ///   - upper_limb: non-zero -> upper limb, zero -> center
    ///       Set to non-zero (e.g. 1) when computing rise/set
    ///       times, and to zero when computing start/end of twilight.
    /// - Returns: rise, set, code.
    ///
    ///     Both times in hours UT are relative to the specified altitude,
    ///     and thus this function can be used to compute
    ///     various twilight times, as well as rise/set times.
    ///
    ///     Code 0 = sun rises/sets this day, times stored at rise and set.
    ///
    ///     Code +1 = sun above the specified "horizon" 24 hours.
    ///     *trise set to time when the sun is at south,
    ///     minus 12 hours while *tset is set to the south
    ///     time plus 12 hours. "Day" length = 24 hours
    ///
    ///     Code -1 = sun is below the specified "horizon" 24 hours
    ///     "Day" length = 0 hours, *trise and *tset are
    ///     both set to the time when the sun is at south.
    private class func sunriset(year: Int,
                                month: Int,
                                day: Int,
                                lon: Double,
                                lat: Double,
                                altit: Double,
                                upper_limb: Int) -> (trise: Double, tset: Double, code: ReturnCode) {

        var altit = altit
        var  d: Double         /* Days since 2000 Jan 0.0 (negative before) */
        var sr: Double         /* Solar distance, astronomical units */
        var sRA: Double        /* Sun's Right Ascension */
        var sdec: Double       /* Sun's declination */
        var sradius: Double    /* Sun's apparent radius */
        var t: Double          /* Diurnal arc */
        var tsouth: Double     /* Time when Sun is at south */
        var sidtime: Double    /* Local sidereal time */

        var rc: ReturnCode = ReturnCode.RiseAndSet     /* Return cde from function - usually 0 */

        /* Compute d of 12h local mean solar time */
        d = Double(days_since_2000_Jan_0(y: year,m: month,d: day)) + 0.5 - lon/360.0;

        /* Compute the local sidereal time of this moment */
        sidtime = revolution( x: GMST0(d: d) + 180.0 + lon )

        /* Compute Sun's RA, Decl and distance at this moment */
        (sRA, sdec, sr) = sun_RA_dec(d: d)

        /* Compute time when Sun is at south - in hours UT */
        tsouth = 12.0 - rev180(x: sidtime - sRA)/15.0

        /* Compute the Sun's apparent radius in degrees */
        sradius = 0.2666 / sr

        /* Do correction to upper limb, if necessary */
        if upper_limb != 0 {
            altit -= sradius
        }

        /* Compute the diurnal arc that the Sun traverses to reach */
        /* the specified altitude altit: */
        do {
            let cost: Double = ( sind(x: altit) - sind(x: lat) * sind(x: sdec) ) / ( cosd(x: lat) * cosd(x: sdec) );
            if ( cost >= 1.0 ) {
                rc = ReturnCode.SunAlwaysBelow
                t = 0.0       /* Sun always below altit */
            }
            else if ( cost <= -1.0 ) {
                rc = ReturnCode.SunAlwaysAbove
                t = 12.0      /* Sun always above altit */
            }
            else {
                t = acosd(x: cost)/15.0   /* The diurnal arc, hours */
            }
        }

        /* Store rise and set times - in hours UT */
        let trise = tsouth - t;
        let tset  = tsouth + t;

        return (trise, tset, rc)
    }  /* __sunriset__ */

    /// The "workhorse" function
    ///
    /// - Parameters:
    ///   - year: year,month,date = calendar date, 1801-2099 only.
    ///   - month: year,month,date = calendar date, 1801-2099 only.
    ///   - day: year,month,date = calendar date, 1801-2099 only.
    ///   - lon: Eastern longitude positive, Western longitude negative
    ///   - lat: Northern latitude positive, Southern latitude negative
    ///   - altit: altit = the altitude which the Sun should cross
    ///               Set to -35/60 degrees for rise/set, -6 degrees
    ///               for civil, -12 degrees for nautical and -18
    ///               degrees for astronomical twilight.
    ///   - upper_limb: upper_limb: non-zero -> upper limb, zero -> center
    ///               Set to non-zero (e.g. 1) when computing day length
    ///               and to zero when computing day+twilight length.
    /// - Returns: Day number
    private class func daylen(year: Int, month: Int, day: Int, lon: Double, lat: Double,
                              altit: Double, upper_limb: Int ) -> Double {
        /**********************************************************************/
        /* Note: year,month,date = calendar date, 1801-2099 only.             */
        /*       Eastern longitude positive, Western longitude negative       */
        /*       Northern latitude positive, Southern latitude negative       */
        /*       The longitude value is not critical. Set it to the correct   */
        /*       longitude if you're picky, otherwise set to to, say, 0.0     */
        /*       The latitude however IS critical - be sure to get it correct */
        /*       altit = the altitude which the Sun should cross              */
        /*               Set to -35/60 degrees for rise/set, -6 degrees       */
        /*               for civil, -12 degrees for nautical and -18          */
        /*               degrees for astronomical twilight.                   */
        /*         upper_limb: non-zero -> upper limb, zero -> center         */
        /*               Set to non-zero (e.g. 1) when computing day length   */
        /*               and to zero when computing day+twilight length.      */
        /**********************************************************************/

        var altit = altit
        var d: Double          /* Days since 2000 Jan 0.0 (negative before) */
        var obl_ecl: Double    /* Obliquity (inclination) of Earth's axis */
        var sr: Double         /* Solar distance, astronomical units */
        var slon: Double       /* True solar longitude */
        var sin_sdecl: Double  /* Sine of Sun's declination */
        var cos_sdecl: Double  /* Cosine of Sun's declination */
        var sradius: Double    /* Sun's apparent radius */
        var t: Double          /* Diurnal arc */

        /* Compute d of 12h local mean solar time */
        d = Double(days_since_2000_Jan_0(y: year, m: month, d: day)) + 0.5 - lon/360.0;

        /* Compute obliquity of ecliptic (inclination of Earth's axis) */
        obl_ecl = 23.4393 - 3.563E-7 * d;

        /* Compute Sun's ecliptic longitude and distance */
        (slon, sr) = sunpos( d: d )

        /* Compute sine and cosine of Sun's declination */
        sin_sdecl = sind(x: obl_ecl) * sind(x: slon);
        cos_sdecl = sqrt( 1.0 - sin_sdecl * sin_sdecl );

        /* Compute the Sun's apparent radius, degrees */
        sradius = 0.2666 / sr;

        /* Do correction to upper limb, if necessary */
        if upper_limb != 0 {
            altit -= sradius
        }

        /* Compute the diurnal arc that the Sun traverses to reach */
        /* the specified altitude altit: */
        do {
            let cost: Double = ( sind(x: altit) - sind(x: lat) * sin_sdecl ) / ( cosd(x: lat) * cos_sdecl );
            if cost >= 1.0 {
                t = 0.0     /* Sun always below altit */
            }
            else if cost <= -1.0 {
                t = 24.0;                     /* Sun always above altit */
            }
            else  {
                t = (2.0/15.0) * acosd(x: cost); /* The diurnal arc, hours */
            }
        }

        return t;
    }  /* __daylen__ */


    /// This function computes the Sun's position at any instant.
    private class func sunpos(d: Double) -> (lon: Double, r: Double ) {
        /******************************************************/
        /* Computes the Sun's ecliptic longitude and distance */
        /* at an instant given in d, number of days since     */
        /* 2000 Jan 0.0.  The Sun's ecliptic latitude is not  */
        /* computed, since it's always very near 0.           */
        /******************************************************/

        var M: Double         /* Mean anomaly of the Sun */
        var w: Double         /* Mean longitude of perihelion */
                              /* Note: Sun's mean longitude = M + w */
        var e: Double         /* Eccentricity of Earth's orbit */
        var E: Double         /* Eccentric anomaly */
        var x: Double
        var y: Double         /* x, y coordinates in orbit */
        var v: Double         /* True anomaly */

        /* Compute mean elements */
        M = revolution( x: 356.0470 + 0.9856002585 * d );
        w = 282.9404 + 4.70935E-5 * d;
        e = 0.016709 - 1.151E-9 * d;

        /* Compute true longitude and radius vector */
        E = M + e * RADEG * sind(x: M) * ( 1.0 + e * cosd(x: M) );
        x = cosd(x: E) - e;
        y = sqrt( 1.0 - e*e ) * sind(x: E);
        let r = sqrt( x*x + y*y );              /* Solar distance */
        v = atan2d( y: y, x: x );               /* True anomaly */
        var lon = v + w                         /* True solar longitude */
        if lon >= 360.0 {
            lon -= 360.0                        /* Make it 0..360 degrees */
        }
        return (lon, r)
    }

    private class func sun_RA_dec( d: Double ) -> (RA: Double, dec: Double, r: Double ) {
        /******************************************************/
        /* Computes the Sun's equatorial coordinates RA, Decl */
        /* and also its distance, at an instant given in d,   */
        /* the number of days since 2000 Jan 0.0.             */
        /******************************************************/

        var obl_ecl: Double
        var x: Double
        var y: Double
        var z: Double

        /* Compute Sun's ecliptical coordinates */
        let (lon, r) = sunpos( d: d )

        /* Compute ecliptic rectangular coordinates (z=0) */
        x = r * cosd(x: lon)
        y = r * sind(x: lon)

        /* Compute obliquity of ecliptic (inclination of Earth's axis) */
        obl_ecl = 23.4393 - 3.563E-7 * d

        /* Convert to equatorial rectangular coordinates - x is unchanged */
        z = y * sind(x: obl_ecl)
        y = y * cosd(x: obl_ecl)

        /* Convert to spherical coordinates */
        let RA = atan2d( y: y, x: x )
        let dec = atan2d( y: z, x: sqrt(x*x + y*y) )
        return (RA, dec, r)
    }  /* sun_RA_dec */

    private static let INV360: Double = ( 1.0 / 360.0 )

    /*******************************************************************/
    /** This function reduces any angle to within the first revolution */
    /** by subtracting or adding even multiples of 360.0 until the     */
    /** result is >= 0.0 and < 360.0                                   */
    /*******************************************************************/
    private class func revolution( x: Double ) -> Double {
        /*****************************************/
        /* Reduce angle to within 0..360 degrees */
        /*****************************************/

        return( x - 360.0 * floor( x * INV360 ) );
    }  /* revolution */

    private class func rev180(x: Double ) -> Double {
        /*********************************************/
        /* Reduce angle to within +180..+180 degrees */
        /*********************************************/

        return( x - 360.0 * floor( x * INV360 + 0.5 ) );
    }  /* revolution */

    /********************************************************************/
    /** This function computes GMST0, the Greenwich Mean Sidereal Time  */
    /** at 0h UT (i.e. the sidereal time at the Greenwhich meridian at  */
    /** 0h UT).  GMST is then the sidereal time at Greenwich at any     */
    /** time of the day.  I've generalized GMST0 as well, and define it */
    /** as:  GMST0 = GMST - UT  --  this allows GMST0 to be computed at */
    /** other times than 0h UT as well.  While this sounds somewhat     */
    /** contradictory, it is very practical:  instead of computing      */
    /** GMST like:                                                      */
    /**                                                                 */
    /**  GMST = (GMST0) + UT * (366.2422/365.2422)                      */
    /**                                                                 */
    /** where (GMST0) is the GMST last time UT was 0 hours, one simply  */
    /** computes:                                                       */
    /**                                                                 */
    /**  GMST = GMST0 + UT                                              */
    /**                                                                 */
    /** where GMST0 is the GMST "at 0h UT" but at the current moment!   */
    /** Defined in this way, GMST0 will increase with about 4 min a     */
    /** day.  It also happens that GMST0 (in degrees, 1 hr = 15 degr)   */
    /** is equal to the Sun's mean longitude plus/minus 180 degrees!    */
    /** (if we neglect aberration, which amounts to 20 seconds of arc   */
    /** or 1.33 seconds of time)                                        */
    /**                                                                 */
    /********************************************************************/
    private class func GMST0( d: Double ) -> Double {
        var sidtim0: Double
        /* Sidtime at 0h UT = L (Sun's mean longitude) + 180.0 degr  */
        /* L = M + w, as defined in sunpos().  Since I'm too lazy to */
        /* add these numbers, I'll let the C compiler do it for me.  */
        /* Any decent C compiler will add the constants at compile   */
        /* time, imposing no runtime or code overhead.               */
        sidtim0 = revolution( x: ( 180.0 + 356.0470 + 282.9404 ) +
            ( 0.9856002585 + 4.70935E-5 ) * d )
        return sidtim0
    }  /* GMST0 */

}