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koreader/plugins/autowarmth.koplugin/suntime.lua

311 lines
10 KiB
Lua

-- 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