Object
of
the
Experiment
At the top of the earth's atmosphere, about 2 calories of
sunlight energy will pass through a 1 cm x 1 cm area every
minute. This is called the solar constant. In this
experiment you will attempt to measure the solar
irradiance or the amount of sunlight energy that arrives at the
ground. Basically you
will point a flat piece of aluminum straight at the sun and measure how
quickly it warms up. The aluminum plate has been painted black to
make it a good absorber of sunlight. In addition to measuring the
time rate
of change of temperature you will need to know the mass, specific heat,
and the crossectional area of the aluminum block.
Conducting the Experiment
Become familiar with the apparatus before you take it outside and place
it in the sunlight. The aluminum block will start to warm up
quickly once it's placed in the sunlight and you will need to be able
to align it and begin taking time and temperature measurements quickly.
The picture below shows how the apparatus should be assembled. Be
careful when pushing the thermometer through the styrofoam and
into the edge of the aluminum block. Don't force the thermometer,
but be sure it slides into the block. Be sure the
thermometer is turned so that you can easily read the scale without
getting in front of the apparatus and casting a shadow on the aluminum
block. The elevation can be adjusted by removing the wire support
and placing the two ends in a different set of holes. Practice
removing and inserting the wire support and adjusting the elevation of
the wooden stand. Your measurements should be taken on a clear
sunny day with calm or light winds. Measurements should be made
between late morning and early afternoon when the sun is relatively
high in the sky.
When you are ready to begin the experiment move the apparatus to a shady location outdoors and
let it sit there for a few minutes to allow the aluminum block to come
to the same temperature as the outside air. You can remove the
thermometer and use it to make a measurement of the outside air
temperature. You might even take the aluminum block out of the
styrofoam and place it on the ground so that it equilibrates more
quickly. In addition to the outside air temperature you should
measure and record the crossectional area of the block (the area of the
surface pointed at the sun). Make a note of the weather
conditions.
Move the apparatus out into the sun. Quickly turn the wooden
stand and adjust the elevation angle until the wooden dowel casts very
little shadow (remove the wire while adjusting the elevation, reinsert
it in appropriate holes when you are close to the necessary elevation
angle). The elevation angle adjustment is somewhat coarse and you
will probably not be able to obtain perfect alignment. Do the
best you can.
Try to align the apparatus in less than 1 minute so that you can make
your first temperature measurement 1 minute after beginning the
experiment. Continue making temperature measurements every minute
for a few minutes so that you can get an idea how quickly the block is
warming up. You might be able to decrease the interval to 2 or 3
minutes if the block is warming slowly. You should continue
making measurements until you see a clear indication in your data that
the rate of warming is beginning to decrease. You will probably
need to make measurements for a total of 20 to 30 minutes.
Periodically check the alignment of the apparatus during this time and
make any adjustments as they are needed.
Data Analysis
Solar irradiance, S, has units of energy per unit area per unit
time. In our experiment
If we assume that all of the sunlight striking the black plate is
absorbed, then a plate with area A that is left in the sunlight for a
time delta t will collect
An aluminum plate with large area will collect more energy than a
plate
with small area. The longer you leave the plate in the sun the
more energy it will collect.
Earlier in the course we came across the following relationship between
energy absorbed and the resulting temperature change
If we substitute in the earlier equation for delta E we obtain
Now we will just solve this equation for S
There is the equation we will use. If you know
the mass of the
aluminum plate, its crossectional area, the specific heat of aluminum,
and measure how quickly the block warms with time, you can calculate
the solar irradiance.
Example
Below are some actual data collected when the experiment was being
tested Your data, particularly the area and mass of
the aluminum block, may differ significantly from the values
below. You should try to collect your data somewhat later than
was done here.
These data are plotted below
The most rapid rise of temperature occurs during the first 10
minutes of the experiment. This is the part of the graph we will
use to determine the rate of rise of temperature. This is shown
on the next graph.
Early in the experiment (the green shaded portion of the curve)
the change in temperature is being caused by absorbed sunlight.
Later (the red portion of the curve) the block is absorbing sunlight
but also losing energy to the cooler surrounding air. Eventually
the block would warm enough that the loss of energy would balance the
absorption of sunlight energy and the temperature plot would level off.
We will first use the two data points at opposite ends of the green
line to calculate the rate of change of temperature with time. We
are just determining the slope of the line.
Now we just insert this value
(together with the mass, specific heat, and area) into the earlier
equation for solar irradiance
This is a very
reasonable result because, on average, about 50% of the sunlight energy
arriving at the top of the earth's atmosphere (2 cal/cm2 min) makes it
to the ground.