Declination angle \(\delta\)
- Def: The declination \(\delta\) is the angular distance of the sun’s rays north (orsouth) of the equator.
- it is the angle between a line extending from the centre ofthe sun to the centre of the earth and the projection of this line upon the earth’s equitorial plane.
- This is the direct consequence of the tilt and it would vary between 23.50 on June 22nd to 23.50 on December 22nd.
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- The declination in degrees for any given day may be calculated from the approximate equation of Cooper(1969) \(\delta(in degrees)=23.45sin(\frac{360}{365})(284+n)\)
where n is the day of the year (i.e., n=1 means January 1st and n=365 means December 31st)
#Assigning day number to dates
days<-seq( as.Date("2017-03-22"), as.Date("2018-03-21"), by="+1 day")
ndays<-length(seq( as.Date("2017-03-22"), as.Date("2018-03-21"), by="+1 day"))
ndays
## [1] 365
delta<-0
for (i in 1:ndays){
delta[i]<-23.45*sin((360/365)*(pi/180)*(280+i))
}
plot(days,delta,type="l",main="Variation of Sun's Declination",xlab="Time of the year",ylab = "Declination(delta) in degrees")

max(delta)
## [1] 23.44978