# Mars obliquity of rotation axis [deg].
delta_0 = 24.936
#' Declination angle: the angular position of the Sun at solar noon with respect to the plane of the equator.
#'
#' For Mars: -24.936° <= delta <= 24.936°.
#' 0 deg at vernal (Ls 0°) and autumnal equinoxes (Ls 180°)
#' +24.936 deg at summer solstice (Ls 90) and -24.936 at at winter solstice (Ls 270°).
#'
#' Source: Equation 7 (1990)
#'
#' @param Ls Areocentric longitude [deg].
#' @param unit
#'
#' @return Declination angle in radians or degrees.
#' @export
declination = function(Ls, unit=1){
if(!unit %in% c(1, 2)){
stop("Declination angle unit option must either be 1 for radians or 2 for degrees.")
}
# For Ls = 180, we get delta = 2.95828423403174e-15 instead of delta = 0.
# This is a hardcoded fix:
if(Ls == 180){
return(0)
}
# Calculate declination angle in radians and degrees.
delta_rad = asin(sin(delta_0*pi/180) * sin(Ls*pi/180))
delta_deg = delta_rad * 180/pi
# # Alternative equation for delta.
# # Source: https://www.giss.nasa.gov/tools/mars24/help/algorithm.html
# delta_rad = asin(0.42565 * sin(Ls*pi/180)) + 0.25 * sin(Ls*pi/180)
# Return result.
if(unit == 1){
return(delta_rad)
}else if(unit == 2){
return(delta_deg)
}else{
# This should not happen.
stop("An unknown error has occurred.")
}
}
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