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@igponce
Created April 26, 2016 10:32
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R - civil Sunrise and sunset time
# Copyright (c) 2016, Iñigo Gonzalez Ponce <igponce (at) gmail>
# All rights reserved.
# Redistribution and use in source and binary forms, with or without
# modification, are permitted provided that the following conditions are met:
# 1. Redistributions of source code must retain the above copyright notice,
# this list of conditions and the following disclaimer.
# 2. Redistributions in binary form must reproduce the above copyright notice,
# this list of conditions and the following disclaimer in the documentation
# and/or other materials provided with the distribution.
# THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
# AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
# IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
# ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT HOLDER OR CONTRIBUTORS BE
# LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR
# CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF
# SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS
# INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN
# CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)
# ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
# POSSIBILITY OF SUCH DAMAGE.
# civilSunriseSunset.R
# Method from: http://williams.best.vwh.net/sunrise_sunset_algorithm.htm
civilSunriseSunset <- function (year, month, day, latitude, longitude, utcOffset = 0) {
# Sunrise/Sunset Algorithm
# Source:
# Almanac for Computers, 1990
# published by Nautical Almanac Office
# United States Naval Observatory
# Washington, DC 20392
# Inputs:
# day, month, year: date of sunrise/sunset
# latitude, longitude: location for sunrise/sunset
# zenith: Sun's zenith for sunrise/sunset
# offical = 90 degrees 50'
# civil = 96 degrees
# nautical = 102 degrees
# astronomical = 108 degrees
zenith = (96 / 90) * pi
# NOTE: longitude is positive for East and negative for West
# NOTE: the algorithm assumes the use of a calculator with the
# trig functions in "degree" (rather than "radian") mode. Most
# programming languages assume radian arguments, requiring back
# and forth convertions. The factor is 180/pi. So, for instance,
# the equation RA = atan(0.91764 * tan(L)) would be coded as RA
# = (180/pi)*atan(0.91764 * tan((pi/180)*L)) to give a degree
# answer with a degree input for L.
# 1. first calculate the day of the year
N1 <- floor(275 * month / 9)
N2 <- floor((month + 9) / 12)
N3 <- (1 + floor((year - 4 * floor(year / 4) + 2) / 3))
N <- N1 - (N2 * N3) + day - 30
# 2. convert the longitude to hour value and calculate an approximate time
lngHour <- longitude / 15
#if rising time is desired:
# t = N + ((6 - lngHour) / 24)
# t.Rise <- N + ((6 - lngHour) / 24)
#if setting time is desired:
# t = N + ((6 - lngHour) / 24)
t <- c( N + ((6 - lngHour) / 24), #rising time
N + ((18 - lngHour) / 24) #settint time
)
# 3. calculate the Sun's mean anomaly
M <-(0.9856 * t) - 3.289
# 4. calculate the Sun's true longitude
L <- M + (1.916 * sin((pi/180)*M)) + (0.020 * sin((pi/180) * 2 * M)) + 282.634
# NOTE: L potentially needs to be adjusted into the range [0,360) by adding/subtracting 360
L <- ifelse(L > 360, L-360, L)
L <- ifelse(L < 0, L+360, L)
# 5a. calculate the Sun's right ascension
RA <- atan(0.91764 * tan((pi/180)* L))
# NOTE: RA potentially needs to be adjusted into the range [0,360) by adding/subtracting 360
RA <- ifelse (RA <0, RA+360, RA )
RA <- ifelse (RA>360, RA-360, RA)
# 5b. right ascension value needs to be in the same quadrant as L
Lquadrant <- (floor( L/90)) * 90
RAquadrant <- (floor(RA/90)) * 90
RA <- RA + (Lquadrant - RAquadrant)
# 5c. right ascension value needs to be converted into hours
RA <- RA / 15
# 6. calculate the Sun's declination
sinDec <- 0.39782 * sin((pi/180) * L)
cosDec <- cos((pi/180) * asin(sinDec))
# 7a. calculate the Sun's local hour angle
cosH <- (cos((pi/180) * zenith) - (sinDec * sin((pi/180) * latitude))) / (cosDec * cos((pi/180) * latitude))
# if (cosH < -1)
# # the sun never sets on this location (on the specified date)
# if (cosH > 1 )
# # the sun never rises on this location (on the specified date)
# 7b. finish calculating H and convert into hours
#
# if if rising time is desired:
# H = 360 - acos(cosH)
# if setting time is desired:
# H = acos(cosH)
#
# H = H / 15
H <- c( 360 - (180/pi)* acos((pi/180)*cosH[1]), (180/pi)*acos((pi/180)*cosH[2]) ) / 15
# 8. calculate local mean time of rising/setting
T <- H + RA - (0.06571 * t) - 6.622
# 9. adjust back to UTC
UT <- T - lngHour
# NOTE: UT potentially needs to be adjusted into the range [0,24) by adding/subtracting 24
UT <- ifelse(UT < 0, UT+24, UT)
UT <- ifelse(UT > 24, UT-24, UT)
# 10. convert UT value to local time zone of latitude/longitude
localT <- UT + utcOffset
return( localT )
}
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