# Atmospheric Dynamic II - Quiz 1 ##### Author: @1chooo > 有拿到這連結的人不需要註冊或登入便可以新增答案、題目或觀念上去,讓我們一起把這份考古變更完整。 > (註:若不知道怎麼打公式或排版可以去查 LaTex 跟 MarkDown 語法,向以前雲端硬碟形式考古挑戰,將資訊真正統整流傳) ### (1102-1) Must!!! For the two laver model. its instability regime is given by the right diagram and the phase speed is given by $c = U_m - \frac{\beta(k^2 + \lambda^2)}{k^2(k^2 + 2\lambda^2)} \pm \delta^{1/2}$ where $\delta \equiv \frac{\beta^2\lambda^4}{k^4{(k^2 + 2\lambda^2)}^2} - \frac{{U_T}^2 (2\lambda^2 - k^2)}{(k^2 + 2\lambda^2)}; \lambda^2 \equiv \frac{{f_0}^2}{[\sigma(\delta\rho)]}$ Discuss: * [ ] the setup of the two-layer model, * [x] stability of short waves. ![](https://i.imgur.com/Y1ya40p.jpg) * [x] the magnitude of minimum $U_T$ for instahility to occur. ![](https://i.imgur.com/YNFeKov.jpg) * [x] the role of $\beta - effect$ ![](https://i.imgur.com/lLJ7RLS.jpg) * [x] the most unstable (optmal) for instability(from the diagram) and![](https://i.imgur.com/Q1Ok8q5.jpg) * [x] the growth rate for the condition of $\beta = 0$![](https://i.imgur.com/o2G7z5t.jpg) ![](https://i.imgur.com/c2zZquY.jpg) ![](https://i.imgur.com/g4zpLAC.jpg) ### (1102-2) * [x] Diagram the structure of most amplifying baroclinic wave at upper and lower levels in the two-layer model, and discuss the roles of perturbation vertical circulation $(\bar{w^\prime T^\prime})$ and meridional circulation $(\bar{v^\prime T^\prime})$ in energy conversion for mean flow and eddy.![](https://i.imgur.com/7P0hR3G.jpg) ### (1102-3) Available Potential Energy (APE) * [x] Show that for a hvdrostatic system $E_p=\int_{0}^{\infty}\rho gz dz = (R/C_v)E_1$![](https://i.imgur.com/w6ywoRM.jpg) * [x] Discuss available potential energy (APE) and give one simple example to cxplain APE.![](https://i.imgur.com/Cp19zRI.jpg) ### (1102-4) Rayleigh The Rayleigh Theorem indicates that the quasi-geostrophic (O-G) system satisfies the constraint ![](https://i.imgur.com/1vLqiKQ.png)where $z^*$ is the log-pressure height with the flow top H. * [x] Please explain how both barotropic instability and baroclinic instability exist in the system.![](https://i.imgur.com/07cLcyo.jpg) * [ ] Explain how barotropic instability is related to the meridional gradient of absolute vorticity. ### (1102-5) Brietly answer the following problems * [x] Derive the mean incompressible continuity equation using Reynolds average and decomposition.![](https://i.imgur.com/DgZIoGO.jpg) * [x] What is TKE? Describe how the TKE can be produced or lost in the TKE equation.![](https://i.imgur.com/CQmsxpH.jpg) * [x] Show that vertical turbulent momentum fluxes are always downward near the lowest surface.![](https://i.imgur.com/4adn1Bw.jpg) ![](https://i.imgur.com/5uJtQ6K.jpg) * [ ] Express turbulent momentum and heat fluxes based on K-theory. * [x] Explain why the Navior-Stokes equations without Reynolds average are not applicable in practice.![](https://i.imgur.com/T5Ezpnu.jpg) ![](https://i.imgur.com/PjuYFlq.jpg) ### (1102-6) * [ ] Express the Reynolds-average large-scale momentum equations with K-theory and discuss how the steady-state mean flow in balance will be crossing isobars toward the lower pressure in PBL. * [ ] Depict the Ekman spiral of the wind solution for constant $K_m$ and estimate the depth of the Ekman layer with $K_m = 5 m^2s^{-2}$. ### (1102-7) The surface layer * [ ] Explain why the surface laver is usually called as a constant-flux layer and use this assumption to derive the wind profile in the neutral surface layer based on K-theory. ### (1102-8) Secondary Circulations & Spin Down * [ ] Qualitatively discuss how Ekman pumping can occur due to the presence of turbulent friction in the planetary boundary layer, and how such a pumping may cause the primary baroclinic cyclone to spin down effectively through the induced secondary circulation. --- TODOs: * [ ] Re-organize the question with their own topic below. ## Rayleigh