oce (version 0.9-18)

sunAngle: Solar Angle as Function of Space and Time

Description

Solar angle as function of space and time.

Usage

sunAngle(t, longitude=0, latitude=0, useRefraction=FALSE)

Arguments

t

Time, a POSIXt object (must be in timezone UTC), or a numeric value that corresponds to such a time.

longitude

observer longitude in degrees east

latitude

observer latitude in degrees north

useRefraction

boolean, set to TRUE to apply a correction for atmospheric refraction

Value

• A list containing the following.
• time
  time
• azimuth
  azimuth, in degrees eastward of north, from 0 to 360. (See diagram below.)
• altitude
  altitude, in degrees above the horizon, ranging from -90 to 90. (See diagram below.)
• diameter
  solar diameter, in degrees
• distance
  distance to sun, in astronomical units
• html{

  starCoords.png

  {options: width=400px alt="Figure: starCoords.png"}}

Details

Based on NASA-provided Fortran program, in turn (according to comments in the code) based on "The Astronomical Almanac".

References

Based on Fortran code retrieved from ftp://climate1.gsfc.nasa.gov/wiscombe/Solar_Rad/SunAngles/sunae.f on 2009-11-1. Comments in that code list as references:

Michalsky, J., 1988: The Astronomical Almanac's algorithm for approximate solar position (1950-2050), Solar Energy 40, 227-235

The Astronomical Almanac, U.S. Gov't Printing Office, Washington, D.C. (published every year).

The code comments suggest that the appendix in Michalsky (1988) contains errors, and declares the use of the following formulae in the 1995 version the Almanac:

• p. A12: approximation to sunrise/set times;
• p. B61: solar altitude (AKA elevation) and azimuth;
• p. B62: refraction correction;
• p. C24: mean longitude, mean anomaly, ecliptic longitude, obliquity of ecliptic, right ascension, declination, Earth-Sun distance, angular diameter of Sun;
• p. L2: Greenwich mean sidereal time (ignoring T^2, T^3 terms).

The code lists authors as Dr. Joe Michalsky and Dr. Lee Harrison (State University of New York), with modifications by Dr. Warren Wiscombe (NASA Goddard Space Flight Center).

See Also

The equivalent function for the moon is moonAngle.

Examples

rise <- as.POSIXct("2011-03-03 06:49:00", tz="UTC") + 4*3600
set <- as.POSIXct("2011-03-03 18:04:00", tz="UTC") + 4*3600
mismatch <- function(lonlat) 
{
    sunAngle(rise, lonlat[1], lonlat[2])$altitude^2 + sunAngle(set, lonlat[1], lonlat[2])$altitude^2
}
result <- optim(c(1,1), mismatch)
lon.hfx <- (-63.55274)
lat.hfx <- 44.65
dist <- geodDist(result$par[1], result$par[2], lon.hfx, lat.hfx)
cat(sprintf("Infer Halifax latitude %.2f and longitude %.2f; distance mismatch %.0f km", 
            result$par[2], result$par[1], dist))