-- usage -- SunTime:setPosition() -- SunTime:setSimple() or SunTime:setAdvanced() -- SunTime:setDate() -- SunTime:calculate(height, hour) height==Rad(0°)-> Midday; hour=6 or 18 for rise or set -- SunTime:calculateTimes() -- use values -- math abbrevations local toRad = math.pi/180 local toDeg = 1/toRad local floor = math.floor local sin = math.sin local cos = math.cos local tan = math.tan local asin = math.asin local acos = math.acos local atan = math.atan local function Rad(x) return x*toRad end -------------------------------------------- local SunTime = {} SunTime.astronomic = Rad(-18) SunTime.nautic = Rad(-12) SunTime.civil = Rad(-6) -- SunTime.eod = Rad(-49/60) -- approx. end of day ---------------------------------------------------------------- -- simple 'Equation of time' good for dates between 2008-2027 -- errors for latitude 20° are within 1min -- 47° are within 1min 30sec -- 65° are within 5min -- https://www.astronomie.info/zeitgleichung/#Auf-_und_Untergang (German) function SunTime:getZglSimple() local T = self.date.yday return -0.171 * sin(0.0337 * T + 0.465) - 0.1299 * sin(0.01787 * T - 0.168) end -- more advanced 'Equation of time' goot for dates between 1800-2200 -- errors are better than with the simple method -- https://de.wikipedia.org/wiki/Zeitgleichung (German) and -- more infos on http://www.hlmths.de/Scilab/Zeitgleichung.pdf (German) function SunTime:getZglAdvanced() local e = self.num_ex local e2 = e*e local e3 = e2*e local e4 = e3*e local e5 = e4*e local M = self.M -- https://de.wikibooks.org/wiki/Astronomische_Berechnungen_f%C3%BCr_Amateure/_Himmelsmechanik/_Sonne local C = (2*e - e3/4 + 5/96*e5) * sin(M) + (5/4*e2 + 11/24*e4) * sin(2*M) + (13/12*e3 - 43/64*e5) * sin(3*M) + 103/96*e4 * sin(4*M) + 1097/960*e5 * sin(5*M) -- rad local lamb = self.L + C local tanL = tan(self.L) local tanLamb = tan(lamb) local cosEps = cos(self.epsilon) local zgl = atan( (tanL - tanLamb*cosEps) / (1 + tanL*tanLamb*cosEps) ) --rad return zgl*toDeg/15 -- to hours *4'/60 end -- set current date or year/month/day daylightsaving hh/mm/ss -- if dst == nil use curent daylight saving of the system function SunTime:setDate(year, month, day, dst, hour, min, sec) self.oldDate = self.date self.date = os.date("*t") if year and month and day and hour and min and sec then self.date.year = year self.date.month = month self.date.day = day local feb = 28 if year % 4 == 0 and (year % 100 ~= 0 or year % 400 == 0) then feb = 29 end local days_in_month = {31, feb, 31, 30, 31, 30, 31, 31, 30, 31, 30, 31} self.date.yday = day for i = 1, month-1 do self.date.yday = self.date.yday + days_in_month[i] end self.date.hour = hour or 12 self.date.min = min or 0 self.date.sec = sec or 0 if dst ~= nil then self.date.isdst = dst end end -- use cached results if self.olddate and self.oldDate.day == self.date.day and self.oldDate.month == self.date.month and self.oldDate.year == self.date.year and self.oldDate.isdst == self.date.isdst then return end self:initVars() if not self.getZgl then self.getZgl = self.getZglAdvanced end self.zgl = self:getZgl() end function SunTime:setPosition(name, latitude, longitude, time_zone, altitude) altitude = altitude or 200 self.oldDate = nil --invalidate cache self.pos = {name, latitude = latitude, longitude = longitude, altitude = altitude} self.time_zone = time_zone self.refract = Rad(33/60 * .5 ^ (altitude / 5500)) end function SunTime:setSimple() self.getZgl = self.getZglSimple end function SunTime:setAdvanced() self.getZgl = self.getZglAdvanced end function SunTime:daysSince2000() local delta = self.date.year - 2000 local leap = floor(delta/4) local days_since_2000 = delta * 365 + leap + self.date.yday -- WMO No.8 return days_since_2000 end -- more accurate parameters of earth orbit from -- Title: Numerical expressions for precession formulae and mean elements for the Moon and the planets -- Authors: Simon, J. L., Bretagnon, P., Chapront, J., Chapront-Touze, M., Francou, G., & Laskar, J., , -- Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 2, p. 663-683 -- Bibliographic Code: 1994A&A...282..663S function SunTime:initVars() self.days_since_2000 = self:daysSince2000() local T = self.days_since_2000/36525 -- self.num_ex = 0.016709 - 0.000042 * T -- self.num_ex = 0.0167086342 - 0.000042 * T -- see wikipedia: https://de.wikipedia.org/wiki/Erdbahn-> Meeus self.num_ex = 0.0167086342 + T*(-0.0004203654e-1 + T*(-0.0000126734e-2 + T*( 0.0000001444e-3 + T*(-0.0000000002e-4 + T* 0.0000000003e-5)))) -- self.epsilon = (23 + 26/60 + 21/3600 - 46.82/3600 * T) * toRad -- see wikipedia: https://de.wikipedia.org/wiki/Erdbahn-> Meeus local epsilon = 23 + 26/60 + (21.412 + T*(-46.80927 + T*(-0.000152 + T*(0.00019989 + T*(-0.00000051 - T*0.00000025)))))/3600 --° self.epsilon = epsilon * toRad -- local L = (280.4656 + 36000.7690 * T ) --° -- see Numerical expressions for precession formulae ... -- shift from time to Equinox as data is given for JD2000.0, but date is in days from 20000101 local nT = T * 1.0000388062 --mean longitude local L = 100.46645683 + (nT*(1295977422.83429E-1 + nT*(-2.04411E-2 - nT* 0.00523E-3)))/3600--° self.L = (L - floor(L/360)*360) * toRad -- wikipedia: https://de.wikipedia.org/wiki/Erdbahn-> Meeus local omega = 102.93734808 + nT*(17.194598028e-1 + nT*( 0.045688325e-2 + nT*(-0.000017680e-3 + nT*(-0.000033583e-4 + nT*( 0.000000828e-5 + nT* 0.000000056e-6))))) --° -- Mittlere Länage local M = L - omega self.M = (M - floor(M/360)*360) * toRad -- Deklination nach astronomie.info -- local decl = 0.4095 * sin(0.016906 * (self.date.yday - 80.086)) --Deklination nach Brodbeck (2001) -- local decl = 0.40954 * sin(0.0172 * (self.date.yday - 79.349740)) --Deklination nach John Kalisch (derived from WMO-No.8) --local x = (36000/36525 * (self.date.yday+hour/24) - 2.72)*toRad --local decl = asin(0.397748 * sin(x + (1.915*sin(x) - 77.51)*toRad)) -- Deklination WMO-No.8 page I-7-37 --local T = self.days_since_2000 + hour/24 --local L = 280.460 + 0.9856474 * T -- self.M --L = (L - floor(L/360)*360) * toRad --local g = 357.528 + 0.9856003 * T --g = (g - floor(g/360)*360) * toRad --local l = L + (1.915 * sin (g) + 0.020 * sin (2*g))*toRad --local ep = self.epsilon -- -- sin(decl) = sin(ep)*sin(l) --self.decl = asin(sin(ep)*sin(l)) -- Deklination WMO-No.8 page I-7-37 local l = self.L + math.pi + (1.915 * sin (self.M) + 0.020 * sin (2*self.M))*toRad self.decl = asin(sin(self.epsilon)*sin(l)) -- Nutation see https://de.wikipedia.org/wiki/Nutation_(Astronomie) local A = { 2.18243920 - 33.7570460 * T, -2.77624462 + 1256.66393 * T, 7.62068856 + 16799.4182 * T, 4.36487839 - 67.140919 * T} local B = {92025e-4 + 8.9e-4 * T, 5736e-4 - 3.1e-4 * T, 977e-4 - 0.5e-4 * T, -895e-4 + 0.5e-4 * T} local delta_epsilon = 0 for i = 1, #A do delta_epsilon = delta_epsilon + B[i]*cos(A[i]) end -- add nutation to declination self.decl = self.decl + delta_epsilon/3600 -- https://de.wikipedia.org/wiki/Kepler-Gleichung#Wahre_Anomalie self.E = self.M + self.num_ex * sin(self.M) + self.num_ex^2 / 2 * sin(2*self.M) self.a = 149598022.96E3 -- große Halbaches in m self.r = self.a * (1 - self.num_ex * cos(self.E)) -- self.eod = -atan(6.96342e8/self.r) - Rad(33.3/60) -- without nutation self.eod = -atan(6.96342e8/self.r) - self.refract -- with nutation -- ^--sun radius ^- astronomical refraction (500m altitude) end -------------------------- function SunTime:getTimeDiff(height) local val = (sin(height) - sin(self.pos.latitude)*sin(self.decl)) / (cos(self.pos.latitude)*cos(self.decl)) if math.abs(val) > 1 then return end return 12/math.pi * acos(val) end -- get time for a certain height -- set hour to 6 for rise or 18 for set -- result rise or set time -- nil sun does not reach the height function SunTime:calculateTime(height, hour) hour = hour or 12 local dst = self.date.isdst and 1 or 0 local timeDiff = self:getTimeDiff(height, hour) if not timeDiff then return end local local_correction = self.time_zone - self.pos.longitude*12/math.pi + dst - self.zgl if hour < 12 then return 12 - timeDiff + local_correction else return 12 + timeDiff + local_correction end end function SunTime:calculateTimeIter(height, hour) return self:calculateTime(height, hour) end function SunTime:calculateTimes() self.rise = self:calculateTimeIter(self.eod, 6) self.set = self:calculateTimeIter(self.eod, 18) self.rise_civil = self:calculateTimeIter(self.civil, 6) self.set_civil = self:calculateTimeIter(self.civil, 18) self.rise_nautic = self:calculateTimeIter(self.nautic, 6) self.set_nautic = self:calculateTimeIter(self.nautic, 18) self.rise_astronomic = self:calculateTimeIter(self.astronomic, 6) self.set_astronomic = self:calculateTimeIter(self.astronomic, 18) self.noon = (self.rise + self.set) / 2 self.midnight = self.noon + 12 self.times = {} self.times[1] = self.noon - 12 self.times[2] = self.rise_astronomic self.times[3] = self.rise_nautic self.times[4] = self.rise_civil self.times[5] = self.rise self.times[6] = self.noon self.times[7] = self.set self.times[8] = self.set_civil self.times[9] = self.set_nautic self.times[10] = self.set_astronomic self.times[11] = self.noon + 12 end -- get time in seconds (either actual time in hours or date struct) function SunTime:getTimeInSec(val) if not val then val = os.date("*t") end if type(val) == "table" then return val.hour*3600 + val.min*60 + val.sec end return val*3600 end return SunTime