Module 9
PlanningGuide

Lesson 3.5


.
Try This
.
Concepts
.
Equations
.
Examples
.
Exercises
.
Answers
.
Definitions

Lesson 3.5
Lesson 3.6
Lesson 3.7
Lesson 3.8
Lab 3.5
Lab 3.6
Lab 3.7
Lab 3.8
Project 9


Lesson 3.5 Radiation Flux & Absorption

Overview

This lesson deals with the variation in the amount of energy transported by electromagnetic waves as they spread out from their source. On completion of this lesson you should be able to explain the difference between intensity and flux. You should also be able to calculate the variation in flux with distance from a radiating source.

MINI LAB

CHOICE OF ACTIVITIES

  1. Connect a solar cell to a multi-meter and measure the current provided by the cell at various distances from a light source. Plot the meter reading versus distance and the square of the meter reading versus distance.
  2. Repeat the experiment with a different light source. e.g. Compare light from an incandescent bulb and light from a fluorescent tube.
  3. Using a solar cell connected to a meter, measure the solar power at regular intervals (say every hour) for a day and graph the measurements.
  4. Study the effects of clouds and smog on sunlight
  5. Fill three identical bottles with water and place them in the sun for 2 or 3 hours. Add dark dye to two of the bottles and place one of these inside a transparent enclosure that reduces cooling due to air currents. Measure the difference in temperature of the water in the three bottles at the end of the 2- or 3-hour period.

Solar Water Heaters

Many households save a significant amount in potential energy costs by using solar water heaters. Solar water heaters typically consist of a dark colored metal panel that heats up when exposed to the sun. This panel transfers heat to water that circulates through cavities or pipes connected to the panel. The panel is usually enclosed in a shallow box with a transparent cover to prevent cooling of the panel by wind and air currents. Water circulates through the heater to a holding tank either by convection or by means of a small pump. The amount of heat absorbed depends on the area of the panel, the efficiency of the absorber and where it is located.

Directly beneath the Sun, the top of the atmosphere receives roughly 1.39 kilowatts of radiant energy. The atmosphere absorbs some of this energy. The maximum amount of solar energy that reaches the earth’s surface at noon in the tropics is in the region of 1000 Watts per square meter. The maximum amount of energy that a panel can absorb depends on the direction and angle at which it is mounted and its distance from the equator.

Emission of Thermal Radiation

The relationship between temperature and radiant energy was developed and explained by Stephan and Boltzmann in 1884. According to the Stephan-Boltzmann model, the total energy emitted per unit area per second by a black body is given by the equation:

Total Energy = s T4

Where:

T is the absolute temperature (K)

And

s is the Stephan-Boltzmann constant (5.67x10-8 W.m-2 K-4)

Radiation Flux

Radiation flux is the quantity of radiant energy that is moving (or flowing) through an area of space at right angles to the direction of movement. It is defined in terms of this area. In the S.I system, flux is measured in Watts per square meter (W.m-1 ).

Since radiant energy generally spreads out with distance from the emitting source, the flux decreases with distance from the emitter. The area through which energy emitted from a small source can pass increases with the square of the distance from the source. This means that the flux decreases with the square of the distance from the source.

Radiation Intensity

Radiation intensity is the quantity of radiant energy per unit solid angle.

The intensity of radiation from an emitter is a measure of the emitter’s power and is not affected by the distance from the emitter. Radiation intensity is therefore defined in terms of the radiation emitted into a solid angle. A solid angle is a 3-dimensional angle.

Solar Radiation

The Sun’s surface is at 5777 K, it’s luminosity is in the region of 3.85 x 1026 Watts

Solar constant: The radiant flux density (W m-2) normal to the solar beam at the top of the atmosphere (TOA) at the mean sun-earth distance (1.0 Astronomical Unit, AU) equals ~1360 W m-2 varying about 7% between January (0.983 AU) & July (1.017 AU).

99% of solar energy reaching the earth falls between 0.15 - 4.0 µm
9% is ultraviolet (UV) (?< 0.4 µm)
49% is visible (VIS) (0.4 < ? < 0.8 µm)
42% is infrared (IR) ( ? > 0.8 µm)


Atmospheric scattering: Rayleigh scattering by molecules is wavelength dependent (produces blue sky); Mie scattering by dust & aerosols is largely wavelength independent (produces white/gray skies).

Absorption in the atmosphere depends on path-length and the concentration of selective absorbers, especially, H2O & CO2 (for IR), O3 (for UV). The atmosphere is relatively transparent in the visible region.

Transmission through the atmosphere is a function of optical air mass (optical depth) of which solar elevation and altitude are factors.


Diffuse radiation: This arises from atmospheric scattering, clouds, backscatter from the surface.

Photosynthetically Active Radiation: About 50% of solar energy (including scattered light) is Photosynthetically Active Radiation (PAR: 0.4 - 0.7 µm).

Absorptivity

The amount of radiation absorbed by an opaque object depends on the nature of its surface. In general, dark rough surfaces absorb more radiation than light colored, shiny surfaces. The ability of a surface to absorb radiation is measured in terms of its Absorptivity. The Absorptivity is the fraction of radiation that is absorbed. For example, a surface with an Absorptivity of 0.75 will absorb 75% of the radiation reaching that surface. In referring to Absorptivity, the wavelength or range of wavelengths needs to be specified. If a wavelength is not specified, the Absorptivity will be assumed to refer to thermal radiation which is roughly in the range: 0.15 to 4.0 µm

When radiation reaches the surface of an object, a fraction of the radiation will be absorbed and the remainder will be reflected. If the object is partially transparent, a fraction of the radiation will be absorbed, a fraction of the radiation will be reflected and the remainder will be transmitted through the object.

Reflectivity

Reflectivity is the fraction of incident radiation that is reflected by a body. Shiny surfaces and light colored surfaces tend to have relatively high reflectivities and correspondingly low absorptivities.

Transmissivity

The Transmissivity of an object is the fraction of incident radiation that is transmitted through the object. This depends on the thickness of the material since most transparent materials absorb radiation as it passes through the material.

Specific Heat Capacity

The specific heat capacity of water is used to estimate the increase in temperature that is produced by absorption of energy.

The specific heat capacity of water is roughly 4.18 kJ.kg–1 .K–1 . This means that if one kilogram of water absorbs 1000 Joules of energy, the temperature will be increased by one Kelvin.

The specific heat capacity of water at 10 oC is 4.1922 kiloJoules/kg/oC. This changes slightly with temperature. For example: The specific heat capacity of water at 25 oC is 4.1796 kiloJoules/kg/oC.

Solar Heating and Re-Radiation

The Absorptivity of the absorbing panel in a solar heater will affect the efficiency of the heater. In addition to this, the warm surface of the panel will also re-emit some of the absorbed energy. The net amount of energy that is absorbed by the water will depend on the difference between the amount absorbed and the amount that is re-emitted.

The transparent cover over the panel can also play an important part in the design of a solar heater. If it is made from glass, it will block UV and IR radiation from reaching the panel. or this reason, solar panels usually have plastic covers that allow more IR and UV to reach the panel. Plastic surfaces can also be made to have a lower reflectivity than glass and thus minimize the amount of energy lost due to reflection. The primary purpose of the cover is however to prevent cooling of the panel by conduction. Air is a poor conductor but its ability to absorb energy from hot surfaces is increased considerably by movement. By mounting the absorbing panel inside a shallow box with a transparent cover, the air trapped inside helps to insulate the absorber from heat losses due to conduction. Some convective cooling will occur bit this will be minimal due to the low speed of movement of the air.

Review Questions

  1. Intensity and flux both refer to the amount of energy carried by radiation. Explain the difference.
  2. A very small light source is mounted on the opaque surface of a table. If the source emits 3 Watts of radiation into the air above the table, what is the intensity of the source?
  3. A hemispherical plastic bowl with a diameter of 16 inches covers the small light source on the surface of a table referred to above. If the light source is at the center of a circle on the table created by the rim of the bowl, what is the radiation flux at the inner surface of the bowl?
  4. If a larger bowl with a diameter of 24 inches is placed over and centered on the source, what would be the flux at the inner surface of the large bowl?
  5. Radiation from the sun’s surface closely resembles the radiation from a black body at 5777 K. Calculate the amount of energy per square meter leaving the surface of the sun if its radius is estimated to be 6.96 x 108 meters.
  6. A solar water heater with collector area of 1.5 square meters is exposed to solar radiation with a flux of 500 W per square meter. If the net Absorptivity of the collector is 0.25, how much energy is absorbed by the water per hour?
  7. A photovoltaic cell on a handheld calculator has a surface area of 4 x 10-4 square meters is placed on a table directly under a light bulb. The photovoltaic cell intercepts .003 Watts of radiant energy when the distance from the cell to the bulb’s filament is 1 meter. How much energy will the cell intercept if the filament of the bulb is raised to a height of 1.5 meters directly above the cell?