Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Primitive equations
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Forces that cause atmospheric motion== [[Force]]s that cause atmospheric motion include the [[pressure gradient]] force, [[gravity]], and [[viscous]] [[friction]]. Together, they create the forces that accelerate our atmosphere. The pressure gradient force causes an acceleration forcing air from regions of high pressure to regions of low pressure. Mathematically, this can be written as: :<math>\frac{f}{m} = \frac{1}{\rho} \frac{dp}{dx}.</math> The gravitational force accelerates objects at approximately 9.8 m/s<sup>2</sup> directly towards the center of the Earth. The force due to viscous friction can be approximated as: :<math>f_r = {f \over a} {1 \over \rho} \mu\left(\nabla\cdot(\mu \nabla v) + \nabla(\lambda\nabla\cdot v) \right). </math> Using Newton's second law, these forces (referenced in the equations above as the accelerations due to these forces) may be summed to produce an equation of motion that describes this system. This equation can be written in the form: :<math>\frac{dv}{dt} = - (\frac{1}{\rho}) \nabla p - g(\frac{r}{r}) + f_r</math> <!-- What is the r/r term here? --> :<math>g = g_e. \,</math> Therefore, to complete the system of equations and obtain 6 equations and 6 variables: *<math>\frac{dv}{dt} = - (\frac{1}{\rho})\nabla p - g(\frac{r}{r}) + (\frac{1}{\rho})\left[\nabla\cdot (\mu \nabla v) + \nabla(\lambda \nabla\cdot v)\right]</math> <!-- What is the r/r term here? --> *<math>c_{v} \frac{dT}{dt} + p \frac{d\alpha}{dt} = q + f</math> *<math>\frac{d\rho}{dt} + \rho\nabla\cdot v = 0</math> *<math>p = n T.</math> where n is the [[number density]] in mol, and T:=RT is the temperature equivalent value in Joule/mol.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)