One objective of the U.S. Department of Energy's Atmospheric
Radiation Measurement (ARM) Project is to determine the various radiative
properties of different cloud types. For example, because cumulus clouds
form closer to the ground than do cirrus clouds, they emit more radiation
according to the Stefan-Boltzmann law. The effect of cloud type on Earth's
radiation budget is one of the great unanswered questions of climatology.
In this exercise, students will begin to understand the complex interactions
between clouds, the atmosphere and the surface energy budget.
Objectives
Objectives
- To begin to understand the effects of cloud type on radiative energy.
- To help understand how clouds affect the Earth's climate.
- Obtain ARM upwelling and downwelling shortwave radiation and ARM upwelling and downwelling longwave radiation data for two different days. One day should have overcast cirrus clouds during the 24-hour period; the second should have overcast cumulus congestus or cumulonimbus clouds during the 24-hour period.
- Divide the class into groups of 3 or 4 students. If possible, provide each group data at different sites.
- You may want to assign Procedures 3, 4 and 5 as homework.
| PROCEDURE Let Day 1 be the day with cirrus cloud cover and let Day 2 be the day with cumulus cloud cover. 1. Using WxScope, graph the 24-hour upwelling and downwelling shortwave radiation at 15-minute intervals for Day 1. Make a second graph with the upwelling and downwelling longwave radiation for Day 1. 2. Repeat Procedure 1 for Day 2. 3. Create a data table with columns for the hour of the day, average upwelling shortwave, average downwelling shortwave, average upwelling longwave, and average downwelling longwave radiation. 4. For each hour, use your graphs to estimate the hourly average radiation for each type of radiation. Write each of these values on the appropriate column of the table. 5. After your table is complete, compute the total (energy per unit area) for each type of radiation. Remember that the radiation is measured in Watts per square meter, and that Watts are Joules per second. To help you in your computations, note that the estimates you obtained in Procedure 3 are the power per square meter averaged over the hour. Hence, to obtain the energy per square meter, you will need to multiply the average power times the number of seconds in an hour. Then add the energy per square meter for every hour to get the total energy for the day. Shortcut: The following equation describes the same procedure as above, but you will not have to make as many computations: Total Energy per square meter of a given type of radiation = (1 hour) x (60 minutes per hour) x (60 seconds per minute) x [Power1 + Power2 + Power3 + ... + Power24]Be sure to put the appropriate units on your answers. QUESTIONS 1. How do your results compare? How were the individual components of radiation affected under the 2 different cloud covers? Why? 2. Does cloud type affect daily radiative energy balance? How will monthly or yearly radiative balance be affected? 3. What other things will affect the total energy incoming or outgoing at the Earth's surface? |
PREREQUISITES
Cirrus Cumulonimbus Cumulus congestus Energy Joules CORE CURRICULUM SKILLS APPLIED IN THIS LESSON
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