Save
Busy. Please wait.
Log in with Clever
or

show password
Forgot Password?

Don't have an account?  Sign up 
Sign up using Clever
or

Username is available taken
show password


Make sure to remember your password. If you forget it there is no way for StudyStack to send you a reset link. You would need to create a new account.
Your email address is only used to allow you to reset your password. See our Privacy Policy and Terms of Service.


Already a StudyStack user? Log In

Reset Password
Enter the associated with your account, and we'll email you a link to reset your password.
focusNode
Didn't know it?
click below
 
Knew it?
click below
Don't Know
Remaining cards (0)
Know
0:00
Embed Code - If you would like this activity on your web page, copy the script below and paste it into your web page.

  Normal Size     Small Size show me how

Global Circulation

Stull Chapter 11

QuestionAnswer
Radiative Differential Heating Net radiative heating in tropics and net radiative cooling at poles creates and imbalance in the atmosphere/ocean system.
Thermal Wind Relationship The relationship between horizontal and vertical temperature gradient of geostrophic wind. dUg/dz=(-g/Tvfc)(dTv/dy) dVg/dz=(g/Tvfc)(dTv/dx) The north-south temperature gradient alters the east-weest geostrophic winds with height, and vice versa.
Thermal Wind Components UTH=Ug2-Ug1=-(g/fc)(dTH/dy) VTH=Vg2-Vg1=(g/fc)(dTH/dx) *Implies that the thermal wind is parallel to the thickness contours (cold temps to left in N hemisphere).
What is the Thermal Wind? The vector difference between geostrophic winds at two different heights or pressures.
Troposphere Trends The tropopause is lower near poles than near equator. Causing the air over the equator to be colder and warmer over the poles in the stratosphere.
Thickness vs. Isobars Greater TH btwn P sfcs in warmer equatorial air than colder polar air causes isobars to become more tilted at mid-latitudes as tropopause is approached. Regions with greatest tilt have greatest S-N P gradient -- drives fastest geostrophic wind.
Jet Stream Fast geostrophic wind occurs in region greatest S-N P gradient; @ tropopause in mid-lat; move N in summer, S in winter. Velocity +, E-W, in N/S hemis. Mark boundary btwn cold air & warm air b/c T dif generates jet stream winds (thermal wind relationship).
Jet Stream Speeds Actual average speeds of 40 m/s are observed over a three-month average in the winter hemisphere. Velocities up to 100 m/s can be observed on individual days.
Angular Momentum- Theoretical Eastward angular momentum conserved as it moves northward from a source latitude [phi]s to a destination [phi]d.
Angular Momentum and the Earth Radius - Earth's axis to [phi]: R[phi]=ReCos([phi]) Tangential velocity - Earth at [phi]: U[phi]=[omega]R[phi]=[omega]ReCos([phi]) Air parcel - source to dest., velocity relative to Earth: U'=[omega]Re((Cos([phi]s)^2/Cos([phi]d))-cos([phi]d)).
Angular Momentum - Actual Angular momentum is not conserved b/c P gradient, Coriolis, and turbulent drag forces act on the air. The actual vertical circulation pattern extends only to about 30 deg N and S (Hadley Cell).
Relative Vorticity A measure of the rotation of fluids about a vertical axis relative to Earth's sfc. Positive in counterclockwise direction. [Zeta]r=dV/dx-dU/dy [Zeta]r=-dM/dn+M/R If the fluid is rotating as a solid body, [Zeta]r=2M/R
Absolute Vorticity Measure with respect to "fixed" stars. Earth's rotation in addition to the relative vorticity. [Zeta]a=[Zeta]r+fc The Coriolis parameter is a measure of the vorticity of the planet.
Potential Vorticity Absolute vorticity divided by depth of rotating column of air. [Zeta]p=([Zetar]r+fc)/dz=constant Conserved in the absence of turbulent drag and heating.
Vorticities Combined If rotating column of air is stretched vertically, then relative vorticity must increase or move further N where planetary vorticity is greater. Relative={Shear={-dM/dn} Curvature={M/R}} Planetary={fc} Stretching={[Zeta]p(dz)} -dM/dn+M/R+fc=[Zeta]p(dz
Planetary Waves The jet stream meanders N and S in a wavy pattern due to instabilities in the atmosphere as they circle the globe. average wavelength of 3000 km to 4000 km.
Created by: lawli
Popular Science sets

 

 



Voices

Use these flashcards to help memorize information. Look at the large card and try to recall what is on the other side. Then click the card to flip it. If you knew the answer, click the green Know box. Otherwise, click the red Don't know box.

When you've placed seven or more cards in the Don't know box, click "retry" to try those cards again.

If you've accidentally put the card in the wrong box, just click on the card to take it out of the box.

You can also use your keyboard to move the cards as follows:

If you are logged in to your account, this website will remember which cards you know and don't know so that they are in the same box the next time you log in.

When you need a break, try one of the other activities listed below the flashcards like Matching, Snowman, or Hungry Bug. Although it may feel like you're playing a game, your brain is still making more connections with the information to help you out.

To see how well you know the information, try the Quiz or Test activity.

Pass complete!
"Know" box contains:
Time elapsed:
Retries:
restart all cards