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% a learning experience for me, and it shows. Much of the placement
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% was hacked in; if you make it better, let me know...
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% conditional page margins, depending on paper size. Thanks to Uwe Ziegenhagen
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% Made changes based on suggestions from Gene Cooperman. <gene at ccs.neu.edu>
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% -----------------------------------------------------------------------
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\begin{document}
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\raggedright
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\footnotesize
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\begin{multicols*}{3}
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\begin{center}
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\Large{Dynamics of Large-scale Atmospheric Flow} \\
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\small{\href{http://iacweb.ethz.ch/courses/id/701-1221-00L}{701-1221-00L}, HS 22} \\
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\small{Jannis Portmann} \\
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{\ccbysa}
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\rule{\linewidth}{0.25pt}
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\end{center}
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\section{Equations}
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\subsection{Fundamental equations}
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\subsubsection{Navier-Stokes}
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\begin{equation}
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\frac{D\vb{u}}{Dt} = \underbrace{-\frac{1}{\rho}\nabla p}_\mathrm{Pressure} - \underbrace{(2\Omega \times \vb{u})}_\mathrm{Coriolis} - \underbrace{g'K}_\mathrm{Gravity} + \underbrace{F^{**}}_\mathrm{Viscous}
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\end{equation}
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\subsubsection{Conservation of mass}
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\begin{equation}
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\frac{D \rho}{Dt} + \rho(\nabla \vb{u}) = 0
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\end{equation}
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\subsubsection{First law of thermodynamics}
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\begin{equation}
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\frac{D\theta}{Dt} = \bigg(\frac{\theta}{c_p T} \bigg) \mathcal{H}
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\end{equation}
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if $\mathcal{H} = 0$, the process is \textit{adiabatic}
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\subsubsection{Equation of state}
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\begin{equation}
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p = \rho RT
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\end{equation}
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\subsection{Circulation}
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\begin{equation}
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C = \oint_c \vec{v} \, dc = \oint (u \, dx + v \, dy + w \, dz) = \oint_0^{2\pi} \vec{v} \, r \, d\phi
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\end{equation}
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\subsection{Quasi geostrophic system of equations}
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\begin{equation}
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\zeta = \frac{\partial v}{\partial x} - \frac{\partial u}{\partial y}
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\end{equation}
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\subsubsection*{Vorticity equation}
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\begin{equation}
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\frac{D_h}{Dt} \zeta + \beta v = -f_0(\nabla_h \vec{v})
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\end{equation}
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\subsection{Geostrophic streamfunction}
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\begin{equation}
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\nabla_h \psi = \zeta_G
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\end{equation}
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\subsection{Wave theory}
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\subsubsection*{Pertubation tendency}
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\begin{equation}
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\psi = \underbrace{\bar{\psi}(y,z)}_\mathrm{Mean \, meridional \, flow} + \underbrace{\psi'(x,y,z,t)}_\mathrm{Pertubation}
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\end{equation}
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assuming $|\psi'| \ll |\bar{\psi}|$
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\begin{equation}
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\bigg(\frac{\partial}{\partial t} + \mathcal{U} \bigg) q' + v'(\frac{\partial}{\partial y} \bar{q} + \beta) = 0
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\end{equation}
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with $\mathcal{U} = - \frac{\partial \bar{\psi}}{\partial y}$
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\section{Concepts}
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\subsection{Thermal wind}
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\textit{Thermal wind} describes the vertical change of geostrophic (i.e. horizontal) wind
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\begin{equation}
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\frac{\partial}{\partial z} \vb{v_G} = \bigg(\frac{1}{f}\frac{g}{\theta_0}\bigg)(\vb{k} \times \nabla_h \theta^*)
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\end{equation}
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\subsection{$Q$-Vector}
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The $Q$-Vector indicates if there is cyclogenesis ($\mathcal{F} < 0$, $\mathcal{F} \sim \nabla_h Q$)
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\vspace{2mm} \\
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How to determine the $Q$-Vector on weather charts:
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\begin{enumerate}
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\item Locate regions with:
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\begin{itemize}
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\item Large temperature gradient
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\item Strong wind change
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\end{itemize}
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\item Determine wind-change vector along $\eta$ (warm to the right, see Figure~\ref{Q-eta})
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\item Rotate that vector by $-90^\circ$
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\end{enumerate}
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\begin{figure}[H]
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\centering
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\includegraphics[width=0.1\textwidth]{eta.png}
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\caption{Direction of $\eta$}
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\label{Q-eta}
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\end{figure}
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\begin{equation}
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\vb{Q} = -\frac{g}{\theta_0}|\nabla_h\theta^{*}|(\vb{k} \wedge \frac{\partial}{\partial \xi}\vb{v_G})
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\end{equation}
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\subsection{PV streamer}
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\begin{itemize}
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\item is an upper level positive PV anomaly
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\item induces cyclonal flow
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\end{itemize}
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\scriptsize
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\section*{Copyleft}
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\doclicenseImage \\
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This document is released under (CC BY-SA 3.0) \\
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\faGlobeEurope \kern 1em \url{https://n.ethz.ch/~jannisp/lsd-zf} \\
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\faGit \kern 0.88em \url{https://git.thisfro.ch/thisfro/lsd-zf} \\
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Jannis Portmann, HS22
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\printbibliography
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\section*{Image sources}
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\begin{itemize}
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\item Figure~\ref{Q-eta} (Skript, \cite{wernliLectureScript})
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\end{itemize}
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\end{multicols*}
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\end{document}
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