Function sun_angles() returns the solar angles and Sun to Earth
relative distance for given times and locations using a very precise
algorithm. Convenience functions sun_azimuth(),
sun_elevation(), sun_zenith_angle() and
distance_to_sun() are wrappers on sun_angles() that return
individual vectors.
sun_angles(
time = lubridate::now(tzone = "UTC"),
tz = lubridate::tz(time),
geocode = tibble::tibble(lon = 0, lat = 51.5, address = "Greenwich"),
use.refraction = FALSE
)sun_angles_fast(time, tz, geocode, use.refraction)
sun_elevation(
time = lubridate::now(),
tz = lubridate::tz(time),
geocode = tibble::tibble(lon = 0, lat = 51.5, address = "Greenwich"),
use.refraction = FALSE
)
sun_zenith_angle(
time = lubridate::now(),
tz = lubridate::tz(time),
geocode = tibble::tibble(lon = 0, lat = 51.5, address = "Greenwich"),
use.refraction = FALSE
)
sun_azimuth(
time = lubridate::now(),
tz = lubridate::tz(time),
geocode = tibble::tibble(lon = 0, lat = 51.5, address = "Greenwich"),
use.refraction = FALSE
)
distance_to_sun(
time = lubridate::now(),
tz = lubridate::tz(time),
geocode = tibble::tibble(lon = 0, lat = 51.5, address = "Greenwich"),
use.refraction = FALSE
)
A data.frame with variables time (in same TZ as input),
TZ, solartime, longitude, latitude,
address, azimuth, elevation, declination,
eq.of.time, hour.angle, and distance. If a data frame
with multiple rows is passed to geocode and a vector of times longer
than one is passed to time, sun position for all combinations of
locations and times are returned by sun_angles. Angles are expressed
in degrees, solartime is a vector of class "solar.time",
distance is expressed in relative sun units.
A "vector" of POSIXct Time, with any valid time zone (TZ) is allowed, default is current time.
character string indicating time zone to be used in output.
data frame with variables lon and lat as numeric values (degrees), nrow > 1, allowed.
logical Flag indicating whether to correct for fraction in the atmosphere.
Given an instant in time and a time zone, the date is
computed from these, and may differ by one day to that at the location
pointed by geocode at the same instant in time, unless the argument
passed to tz matches the time zone at this location.
This function is an implementation of Meeus equations as used in NOAAs on-line web calculator, which are precise and valid for a very broad range of dates (years -1000 to 3000 at least). The apparent solar elevations near sunrise and sunset are affected by refraction in the atmosphere, which does in turn depend on weather conditions. The effect of refraction on the apparent position of the sun is only an estimate based on "typical" conditions for the atmosphere. The computation is not defined for latitudes 90 and -90 degrees, i.e. exactly at the poles. The function is vectorized and in particular passing a vector of times for a single geocode enhances performance very much as the equation of time, the most time consuming step, is computed only once.
For improved performance, if more than one angle is needed it
is preferable to directly call sun_angles instead of the wrapper
functions as this avoids the unnecesary recalculation.
The primary source for the algorithm used is the book: Meeus, J. (1998) Astronomical Algorithms, 2 ed., Willmann-Bell, Richmond, VA, USA. ISBN 978-0943396613.
A different implementation is available at https://github.com/NEFSC/READ-PDB-AstroCalc4R/.
An interactive web page using the same algorithms is available at https://gml.noaa.gov/grad/solcalc/. There are small differences in the returned times compared to our function that seem to be related to the estimation of atmospheric refraction (about 0.1 degrees).
Other astronomy related functions:
day_night(),
format.solar_time()
library(lubridate)
sun_angles()
sun_azimuth()
sun_elevation()
sun_zenith_angle()
sun_angles(ymd_hms("2014-09-23 12:00:00"))
sun_angles(ymd_hms("2014-09-23 12:00:00"),
geocode = data.frame(lat=60, lon=0))
sun_angles(ymd_hms("2014-09-23 12:00:00") + minutes((0:6) * 10))
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