Solar zenith angle
The solar zenith angle is the zenith angle of the sun, i.e., the angle between the sun’s rays and the vertical direction.
It is the complement to the solar altitude or solar elevation, which is the altitude angle or elevation angle between the sun’s rays and a horizontal plane.
[1][2] At solar noon, the zenith angle is at a minimum and is equal to latitude minus solar declination angle.
This is the basis by which ancient mariners navigated the oceans.
[3] Solar zenith angle is normally used in combination with the solar azimuth angle to determine the position of the Sun as observed from a given location on the surface of the Earth.
sin δ + cos
where While the formula can be derived by applying the cosine law to the zenith-pole-Sun spherical triangle, the spherical trigonometry is a relatively esoteric subject.
By introducing the coordinates of the subsolar point and using vector analysis, the formula can be obtained straightforward without incurring the use of spherical trigonometry.
[4] In the Earth-Centered Earth-Fixed (ECEF) geocentric Cartesian coordinate system, let
be the latitudes and longitudes, or coordinates, of the subsolar point and the observer's point, then the upward-pointing unit vectors at the two points,
are the basis vectors in the ECEF coordinate system.
Now the cosine of the solar zenith angle,
, is simply the dot product of the above two vectors
is the hour angle defined earlier.
So the above format is mathematically identical to the one given earlier.
Additionally, Ref.
[4] also derived the formula for solar azimuth angle in a similar fashion without using spherical trigonometry.
At any given location on any given day, the solar zenith angle,
, at local solar noon when the hour angle
, it is polar night.
And at any given location on any given day, the solar zenith angle,
, at local midnight when the hour angle
The calculated values are approximations due to the distinction between common/geodetic latitude and geocentric latitude.
However, the two values differ by less than 12 minutes of arc, which is less than the apparent angular radius of the sun.
The formula also neglects the effect of atmospheric refraction.
[5] Sunset and sunrise occur (approximately) when the zenith angle is 90°, where the hour angle h0 satisfies[2]
Precise times of sunset and sunrise occur when the upper limb of the Sun appears, as refracted by the atmosphere, to be on the horizon.
A weighted daily average zenith angle, used in computing the local albedo of the Earth, is given by
where Q is the instantaneous irradiance.
[2] For example, the solar elevation angle is: An exact calculation is given in position of the Sun.
