EME 812
Utility Solar Power and Concentration

3.2. Apparent daily path of the sun

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3.2. Apparent daily path of the sun

For most solar tracking applications, we need a reasonably accurate knowledge of where the sun will be at a specific hour during each day in a year. Theory is well developed to calculate the sun position with respect to the observation point on the earth surface, and it sets the background for design and modeling of both photovoltaic and concentrating solar power systems of various scale.

In order to discuss tracking or any other adjustments of solar receivers, it would be useful first to understand the sun's path across the sky dome. We are going to turn to the following reading, which describes the key parameters of the solar motion.

Reading Assignment

Book chapter: Kalogirou, A, Solar Energy Engineering, Chapter 2: "Environmental Characteristics." pp. 51-63. (See E-Reserves via the Library Resources tab.)

This reading explains a lot about the geometry of sun movement, provides the key equations and example calculations alongside with them. The objective here would be to learn how to estimate the sun position and draw its track for a particular location and time of the year.

The above materials provide the main tools for predicting the position of the sun at a location of choice at any specific time. Let us summarize a few key takeaways from this reading.

The main parameters to determine are solar altitude (α) and solar azimuth (z). Here are the equations that are used to calculate these coordinates:

sin(α)=sin(L)sin(δ)+cos(L)cos(δ)cos(h) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVCI8FfYJH8YrFfeuY=Hhbbf9v8qqaqFr0xc9pk0xbb a9q8WqFfeaY=biLkVcLq=JHqpepeea0=as0Fb9pgeaYRXxe9vr0=vr 0=vqpWqaaeaabiGaciaacaqabeaadaqaaqaaaOqaaiGacohacaGGPb GaaiOBaiaacIcacqaHXoqycaGGPaGaeyypa0Jaci4CaiaacMgacaGG UbGaaiikaiaadYeacaGGPaGaci4CaiaacMgacaGGUbGaaiikaiabes 7aKjaacMcacqGHRaWkciGGJbGaai4BaiaacohacaGGOaGaamitaiaa cMcaciGGJbGaai4BaiaacohacaGGOaGaeqiTdqMaaiykaiGacogaca GGVbGaai4CaiaacIcacaWGObGaaiykaaaa@5862@

(3.1)

where L is local latitude (GIS parameter defined as the angle between the line from the center of the earth to the site of interest and the equatorial plane), δ is the declination, and h is the hour angle for that location.

sin(z)=cos(δ)sin(h)/cos(α)

(3.2)

Let us consider an example showing how to use these equations.

Example

Calculate the solar position for Abu-Dhabi (UAE) on January 15 at 2 pm local time.

For this calculation, we will use equations (3.1) and (3.2) to find the solar altitude and solar azimuth, respectively. We will need to find the following parameters:

L - local latitude - Abu-Dhabi coordinates are: latitude 24.492o N, and longitude 54.358o E

You can use this website to get GIS data.

δ - declination - It is a function of the day of the year (N). For Jan 15, δ = -21.27o

as found by Eq. (2.5), Kalogirou's text.

δ=23.45sin[ 360 365 ( 284+N ) ]
 

h - hour angle - It is a function of the time of the day. For 2 pm, h = 22.04o as found by Eq. (2.9), Kalogirou's text. For calculating hour angle, you need to determine the apparent solar time (AST) - refer to Eq. (2.3) of Kalogirou's text. Applying it to the current location, we find that AST = 13.47 hr decimal time or 1:28 pm clock time. And the hour angle will be:

h = (AST-12) x 15 = (13.47 - 12) x 15 = 22.04

Now we can plug these L, δ, and h numbers into Eq. (3.1):

sin(α) = sin (24.493o)sin(-21.27o) + cos(24.492o)cos(-21.27o)cos(22.04o) = 0.6356

α = 39.47o

For solar azimuth, we use Eq. (3.2):

sin(z) = cos(d)sin(h)/cos(α) = cos(-21.27o)sin(22.04o) / cos(39.47o) = 0.453

z = 26.93o

This calculation can be essentially used for any location and any time in a year. The algorithms available help to produce detailed solar resource data for different settings. These data are available for reference and use, so you do not have to calculate all things from scratch, although it is useful to understand the theoretical background of it.

We can use the Sun Path Chart Program calculator at the University of Oregon's Solar Radiation Monitoring Laboratory website to obtain a complete picture of sun movement throughout the year. The calculator allows data to be plotted in either orthogonal or polar coordinates. For example, the diagram below (Figure 3.2) was obtained for the same location (Abu Dhabi).

graph of sun path adequately described in surrounding text
Figure 3.2. The orthogonal projection of the solar path for the location.
Credit: (Abu Dhabi, 24.5o N, 54.4o W) obtained by the SunChart calculator [UO SRML, 2007].

In this diagram, the solar altitude (elevation) is plotted versus solar azimuth as shown by the blue curves for each date. There are a few representative dates shown, and January 21 is the closest to the calculation example previously given. Note that the solar azimuth is given on the 360o scale, with 180o corresponding to the south. The hourly position of the sun is marked by the red curves. In this particular case, the local standard times are plotted, while a similar diagram can be made in terms of solar time.

Check Your Understanding - Questions 1-3 (Multiple Choice)

Check Your Understanding - Question 4 (Short Answer)

Is it possible for the sun to reach 90° altitude at any time in a year in the following states? Type "yes" or "no" for each location. Can you explain why?

Arizona

Pennsylvania

California

Hawaii

Problem 3-1: Solar path calculation

(This calculation will be submitted as part of Lesson 3 problem set).

  1. Go to the Sun Path Chart Program calculator and calculate the sun path for a location of your choice. Use the orthogonal projection. Save your diagram.

    You may need to find geographical coordinates and time zone for your location as input. Here is one of the websites that can be conveniently used for that purpose: TimeandDate.com. Just type in your location and get the data.

  2. Using equations (3.1) and (3.2) in this lesson, perform a manual calculation of the sun position (solar altitude and solar azimuth) for the same location on April 20th, at 11 am and 3 pm local time.
  3. Mark your manual points on the diagram. Are you able to match your calculations with the plot?

The above materials and activity make sure that you can employ proper tools for defining solar position on the sky dome. Further on positioning of the receiver and respective tracking directions will use this information as the operational basis. Different types of tracking systems are discussed in the next section of the lesson.