Modeling the Earth's Climate Using OneLayer Energy Balance Model
Activity
Note:
For this assignment, you will need to record your work on a word processing document. Your work must be submitted in Word (.doc or .docx) or PDF (.pdf) format so the instructor can open it.
For this activity, you will explore the workings of a onelayer EBM climate model, which you will run through an Excel spreadsheet that is provided.
Directions
 First, save the Problem Set #4 Worksheet to your computer. You will use this word processing document to electronically record your work in the remaining steps.
 Save the worksheet to your computer by rightclicking on the link above and selecting "Save link as..."
 The worksheet is in Microsoft Word format. You can use either Word or Google Docs (free) to work on this assignment. You will submit your worksheet at the end of the activity, so it must be in Word (.doc or .docx) or PDF (.pdf) format so the instructor can open it.
 Please show your work! When you are explicitly asked to create plots in a question, please cutandpaste graphics and the output from the screen to submit along with your discussion and conclusions.

This exercise will work with solar insolation and the onedimensional energybalance model.
a. Using the provided Excel spreadsheet, calculate values of global surface temperature and global tropospheric temperature for varying values of the solar constant, ranging from 0 to 2000 W m^{2}, incremented by 100 W m^{2}. Assume that the value of planetary albedo is 0.32, emissivity is 0.77, and StefanBoltzmann constant is 5.67 x 10^{8 }W m^{2} K^{4}. Construct a table to show your results.
b. Using the values you obtained in (a), plot both global surface temperature and global tropospheric temperature as a function of solar constant; use the same grid for both sets of temperature values. That is, the horizontal axis of the plot should give values of solar constant, and the vertical axis should give values of temperature. Use Excel or another plotting utility of your choice.
c. Describe the relationship between solar constant and global surface and tropospheric temperature. Comment on the approximate range of values of solar constant that could support human life on Earth.

This exercise will work with planetary reflectivity and the onedimensional energybalance model.
a. Using the provided Excel spreadsheet, calculate values of global surface temperature and global tropospheric temperature for varying values of planetary albedo, ranging from 0 to 1, incremented by 0.05. Assume that the value of the solar constant is 1360 W m^{2}, emissivity is 0.77, and StefanBoltzmann constant is 5.67 x 10^{8 }W m^{2} K^{4}. Construct a table to show your results.
b. Using the values you obtained in (a), plot both global surface temperature and global tropospheric temperature as a function of planetary albedo; use the same grid for both sets of temperature values. That is, the horizontal axis of the plot should give values of planetary albedo, and the vertical axis should give values of temperature.
c. Describe the relationship between planetary albedo and global surface and tropospheric temperature. Comment on the approximate range of values of planetary albedo that could support human life on Earth.

This exercise will work with planetary emissivity and the onedimensional energybalance model.
a. Using the provided Excel spreadsheet, calculate values of global surface temperature and global tropospheric temperature for varying values of planetary emissivity, ranging from 0 to 1, incremented by 0.05. Assume that the value of the solar constant is 1360 W m^{2}, planetary albedo is 0.32, and StefanBoltzmann constant is 5.67 x 10^{8 }W m^{2} K^{4}. Construct a table to show your results.
b. Using the values you obtained in (a), plot both global surface temperature and global tropospheric temperature as a function of planetary emissivity; use the same grid for both sets of temperature values. That is, the horizontal axis of the plot should give values of planetary albedo, and the vertical axis should give values of temperature.
c. Describe the relationship between planetary emissivity and global surface and tropospheric temperature. Comment on the approximate range of values of planetary emissivity that could support human life on Earth.
 Discuss the various energybalance models covered in Lessons 4 and 5, comparing and contrasting their assumptions. Limit your discussion to a paragraph.
Submitting your work
 Upload your file to the "Problem Set #4" assignment in Canvas by the due date indicated on our Canvas calendar.
Grading rubric
The instructor will use the general grading rubric for problem sets to grade this activity.