\documentclass[twoside]{article} \usepackage{amssymb} % font used for R in Real numbers \usepackage{graphicx} % for including postscript figures \pagestyle{myheadings} \markboth{\hfil Calculations of the hurricane eye motion \hfil EJDE--2002/??} {EJDE--2002/??\hfil Vladimir Danilov, Georgii Omel'yanov, \& Daniil Rozenknop \hfil} \begin{document} \title{\vspace{-1in}\parbox{\linewidth}{\footnotesize\noindent {\sc Electronic Journal of Differential Equations}, Vol. {\bf 2002}(2002), No. 16, pp. 1--17. \newline ISSN: 1072-6691. URL: http://ejde.math.swt.edu or http://ejde.math.unt.edu \newline ftp ejde.math.swt.edu (login: ftp)} \vspace{\bigskipamount} \\ % Calculations of the hurricane eye motion based on singularity propagation theory % \thanks{ {\em Mathematics Subject Classifications:} 35D99, 86A10. \hfil\break\indent {\em Key words:} asymptotic behavior, forecast, hurricane. \hfil\break\indent \copyright 2002 Southwest Texas State University. \hfil\break\indent Submitted November 7, 2001. Published February 18, 2002.} } \date{} % \author{Vladimir Danilov, Georgii Omel'yanov, \& Daniil Rozenknop} \maketitle \begin{abstract} We discuss the possibility of using calculating singularities to forecast the dynamics of hurricanes. Our basic model is the shallow-water system. By treating the hurricane eye as a vortex type singularity and truncating the corresponding sequence of Hugoniot type conditions, we carry out many numerical experiments. The comparison of our results with the tracks of three actual hurricanes shows that our approach is rather fruitful. \end{abstract} \newcommand{\Hess}{\mathop{\rm Hess}\nolimits} \section{Introduction} In this paper we discuss a possibility of using an approach related to calculating singularities for numerical modeling the dynamics of hurricanes. It is well known that for a detailed mathematical description of large-scale and meso-scale processes in the atmosphere one needs to use very complicated systems of nonlinear partial differential equations based on equations of three-dimensional gas dynamics (e.g., see [1--5]). So far it is impossible to solve such systems numerically in real time, therefore, one must use different simplifying assumptions. The first simplification is to neglect viscosity and heat conduction effects. As a result, the order of equations decreases and the problem of posing boundary conditions disappears. Further possible simplifications (neglect of vertical displacements, heat exchange effects, etc.) lead to comparatively simple models, the simplest of which is the so-called shallow-water system \begin{eqnarray}%1 \frac{\partial U}{\partial t}+\langle U,\nabla\rangle U+\nabla z &=&f\Pi U,\\ \frac{\partial z}{\partial t}+\langle \nabla, zU\rangle&=&0.\nonumber \end{eqnarray} Here $U=(u,v)$ is the vector of horizontal velocity, $\Pi$ is the matrix of rotation through $\pi/2$ ($\Pi_{11}=\Pi_{22}=0$, $\Pi_{12}=-\Pi_{21}=1$), $f$ is the Coriolis parameter, and~$z$ is the geopotential. At the same time, if we neglect dissipative effects, then the solution loses its smoothness. The fact that the solution is singular, allows us to calculate its dynamics by using rather powerful tools developed within the framework of the theory of generalized functions. Roughly speaking, these tools allow us to avoid finding the solution in the entire range of variables and thus only to determine the dynamics of the singularity support. Besides of a natural simplification due a decrease in the dimension of the problem, this approach allows us to avoid a very difficult problem of choosing the initial data in the entire range of spatial variables. Namely, existing monitoring facilities do not allow one to determine the initial distributions of velocity, density, and temperature with sufficient accuracy for large-scale formations. Simultaneously, the hurricane trajectory (the singularity support) can be fixed well by satellite imaging. V.~P.~Maslov [6] proposed the hypothesis that a solution with a weak singularity whose singular support is of codimension~2 corresponds to the center of a hurricane. Such solution admits the representation \begin{equation}%2 U=U^0(x,t)+\sqrt{S(x,t)}U^1(x,t), \quad z=z^0(x,t)+\sqrt{S(x,t)}z^1(x,t), \end{equation} where $U^i$, $z^i$ and $S$ are smooth functions and \begin{equation} S\geq0,\quad \nabla S\Big|_{S=0}=0,\quad \Hess S\Big|_{S=0}>0. \end{equation} To find the trajectory $\Gamma=\{(x,t),S(x,t)=0\}$ of the singularity support, i.e., of a moving point, we substitute a solution of the form (2) into the equation (e.g., into (1)), which leads to the relation \begin{equation} D^0+S^{-1/2}D^1=0, \end{equation} where $D^i$ are smooth functions. In turn, (4) implies the relations \begin{equation} \frac{\partial^{|\alpha|}}{\partial x^\alpha}D^i\bigg|_{\Gamma}=0,\quad |\alpha|=0,1, \dots, \quad i=0,1, \end{equation} which lead to necessary conditions for the existence of a solution of the form~(2). Maslov called these conditions {\em Hugoniot type conditions\/} (by analogy with the Hugoniot condition for shock waves). The above scheme was realized by Maslov and Zhikharev [6, 7] for the shallow-water system without Coriolis effects and by group of authors [8] for the system~(1) with the Coriolis force. Hugoniot type conditions form an infinite non-triangular system. The first 14 equations of them have the form [8] \begin{eqnarray} \dot z^0_0&=&-2q z^0_0,\nonumber\\ \dot V_1&=&fV_2- z^0_{10},\nonumber\\ \dot V_2&=&-fV_1- z^0_{01},\nonumber\\ \dot z^0_{10}&=&-3qz^0_{10}+pz^0_{01}-z^0_0(v^0_{11}+2u^0_{20}),\nonumber\\ \dot z^0_{01}&=&-3qz^0_{01}-pz^0_{10}-z^0_0(u^0_{11}+2v^0_{02}),\nonumber\\ \dot q&=&-q^2+p^2-fp-2r,\nonumber\\ \dot p&=&-2pq+fq,\\ \dot r&=&-4qr-z^0_{10}(3u^0_{20}+v^0_{11})-z^0_{01}v^0_{20} -\{z^0_0(3u^0_{30}+v^0_{21})\},\nonumber\\ \dot u^0_{20}&=&-3qu^0_{20}+p(u^0_{11}-v^0_{20})+fv^0_{20}-\{3z^0_{30}\},\nonumber\\ \dot u^0_{11}&=&-3qu^0_{11}+p(2u^0_{02}-2u^0_{20}-v^0_{11})+fv^0_{11} -\{2z^0_{21}\},\nonumber\\ \dot u^0_{02}&=&-3qu^0_{02}-p(u^0_{11}+v^0_{02})+fv^0_{02}-\{z^0_{12}\},\nonumber\\ \dot v^0_{20}&=&-3qv^0_{20}+p(v^0_{11}+u^0_{20})-fu^0_{20}-\{z^0_{21}\},\nonumber\\ \dot v^0_{11}&=&-3qv^0_{11}+p(2v^0_{02}-2v^0_{20}+u^0_{11})-fu^0_{11} -\{2z^0_{12}\},\nonumber\\ \dot v^0_{02}&=&-3qv^0_{02}-p(v^0_{11}-u^0_{02})-fu^0_{02} -\{3z^0_{03}\}.\nonumber \end{eqnarray} Here $V=(V_1,V_2)$ is the velocity of the singularity support $x=a(t)$, $q=u^0_{10}=v^0_{01}$, $p=u^0_{01}=-v^0_{10}$, $r=z^0_{20}=z^0_{02}$, and $u^0_\alpha, v^0_\alpha, z^0_\alpha$ are coefficients of the expansion of the solution~(2) in a neighborhood of the singularity support, i.e., $U^i=(u^i, v^i)$, $i=0,1$, $$ u^i=\sum^\infty_{k=0}\sum_{|\alpha|=k}u^i_\alpha(t)\big(x-a(t)\big)^\alpha, \quad v^i=\sum^\infty_{k=0}\sum_{|\alpha|=k}v^i_\alpha(t)\big(x-a(t)\big)^\alpha, $$ $$ z^i=\sum^\infty_{k=0}\sum_{|\alpha|=k}z^i_\alpha(t)\big(x-a(t)\big)^\alpha. $$ The truncation of the sequence at the 14th term means that we neglect the terms in the braces in~(6). A comparison of numerical results with the actual track of the hurricane FORREST (21/09--31/09/1983, the Pacific Ocean) shows that there is a qualitative coincidence between these trajectories~[8]. It was also shown that, besides (2), Eqs. (1) do not have any other singular solutions with pointwise support of the singularity [9] and that the truncated system~(6) can be reduced to the Hill equation [10]. These results stimulated us to try to forecast the dynamics of hurricanes. It should be noted that we consider not simply a nonsmooth solution from a Banach space but a solution of some special structure and try to calculate the trajectory of motion its singularity. It is impossible to ``catch'' this solution by traditional methods for studying PDE. The authors developed a special method for estimating the error of the asymptotic with respect to smoothness solution. By using this method, the simplest version of the shallow water equations, i.e., the Hopf equation, has been studied [11]. Even in this special case, the estimation of the remainder turned out to be a very nontrivial problem. For the shallow water equations, this estimation must be more difficult. On the other hand, the obtained asymptotic solution could be compared with the results of the direct numerical computation for the shallow water equations. However, here we have a very complicated problem of setting the boundary conditions corresponding to the hurricane problem, which are necessary for numerical computations. Therefore, we decided to omit all stages that are traditional in the mathematical study and to test the constructed asymptotic solution by using the forecasted hurricane motion. We present the results of numerical calculations for three actually existing hurricanes (there we used the information about hurricane tracks delivered by the National Hurricane Center, USA). All results obtained can be judged as follows: the present approach is reasonable and competent and allows us to obtain a sufficiently good short-term forecast (not less than 24 hours). However, system~(6) cannot be used for a long-term forecast. The results obtained allow us to assume that, most likely, this fact is related to defects of model~(1) used here. Thus there is the problem of choosing an initial model that is more adequate than model~(1), for which we need to construct a sequence of Hugoniot type equations and to carry out the corresponding numerical experiments. This research was partially supported by the Russian Foundation for Basic Research, grants No.~99-01-01074 and No.~01-01-06057. \section{Numerical calculations of Hugoniot type equations. Long-term forecast} By truncating the system (6), we reduce the problem of calculating the dynamics of the hurricane center to the problem of solving a system consisting of 14 ordinary differential equations. There is the principal problem of choosing the Cauchy data. Our main idea is to choose the Cauchy data so that the trajectory calculated by the truncated system~(6) be maximally close to a given track of an actual hurricane during some time interval $[0,t_{K+1}]$. Obviously, by studying the corresponding solution of~(6) for $t>t_{K+1}$, we can forecast the further motion of the hurricane center. Let us describe the algorithm that realizes this idea. By $\xi(t)=(\lambda(t),\varphi(t))$, $t\in[0,t_I]$, we denote the trajectory of an actual hurricane. Let $\xi_i=\xi(t_i)$ be the coordinates of the hurricane center at time $t_i=(i-1)\Delta t$, where $i=1,\dots,I$ is the measurement number and $\Delta t$ is the time interval between successive measurements (usually, $\Delta t=6$\,hrs.). By $\mu^0=(z^0_0\big|_{t=0},\dots,v^0_{02}\big|_{t=0})$ we denote the set of initial data for system~(6) and by $\mu(t_i,\mu^0)$ the solution of the Cauchy problem for~(6) with the initial data~$\mu^0$ calculated at time~$t_i$. Here and in the following, system~(6) means that the system is truncated. We choose a number $Kt_{46}$ (see Fig.~12). Curiously enough, all these forecasts show that the hurricane makes a turn at a longitude of $27^\circ$--$33^\circ$, although the beach was not taken into account in model~(1). So, we see that our {\it a priori\/} assumption that model~(1) and system~(6) are sufficiently adequate for forecasting the hurricane GEORGES is true. \begin{figure}[t] \centering \includegraphics[width=0.7\textwidth]{fig19.eps} \caption{\small $\xi$ is the track of NICOLE starting at 09:00 a.m. 25/11 1998, $\zeta$ is the artificial trajectory. Initial data: 8.12 $10^{-5}$, ${}-2.64$, 1.33 $10^{-2}$, 0.10, 4.75, 2.22 $10^{-2}$, 0.165, 4.22 $10^{-9}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, K=3, M=1. Distances for approximation: 0, 0.35, 0.31, 0.28. Distances for forecast: 0.32, 1.08, 1.82, 2.77, 4.26, 6.02, 8.19, 10.8, 13.9. } \end{figure} 2. The behavior of the hurricane NICOLE was affected by powerful external factors. This hurricane, first observed on 24/11/1998 about 700 miles to the West of the Canary Isles, initially moved to the South--West and then turned to the West. About 96\,hrs. later, the hurricane sharply changed the direction of its motion and moved to the Northeast. Next, about 30\,hrs. after the turn, the trajectory of the hurricane started to bend in the direction opposite to the action of the Coriolis force. Because of such behavior of NICOLE, one can hardly expect that model~(1) can describe the actual trajectory. Nevertheless, the numerical experiments performed show that our algorithms provide a sufficiently good forecast for 24\,hrs. Figure~13 shows the artificial trajectory calculated for $K=3$ and $M=1$, which corresponds to the forecast for $t>t_4=18$\,hrs. We see that the artificial and actual trajectories agree sufficiently well until the turning point of the actual hurricane. \begin{figure}[t] \centering \includegraphics[width=0.7\textwidth]{fig20.eps} \caption{\small Initial data: 8.12 $10^{-5}$, ${}-4.21$, 9.50 $10^{-3}$, 0.195, 2.77, 3.54 $10^{-2}$, 0.321, 4.22 $10^{-9}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, ${}-9.8 10^{-16}$, K=3, M=9. Distances for approximation: 0, 0.03, 0.09, 0.22. Distances for forecast: 0.41, 0.45, 0.75, 0.23, 1.44, 3.26, 5.86, 10.0, 16.3. } \end{figure} \begin{figure}[t] \centering \includegraphics[width=0.7\textwidth]{fig21.eps} \caption{\small Initial data: 8.12 $10^{-5}$, ${}-2.15$, ${}-1.56$, 4.47, ${}-8.10$, 0.233, 0.299, 4.84 $10^{-11}$, ${}-8.22 10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, K=3, M=15. Distances for approximation: 0, 0.56, 0.79, 0.84. Distances for forecast: 2.37, 3.91, 6.30, 7.84, 10.9, 13.7. } \end{figure} The calculations of the next sloping part of the trajectory ($K=3$, $M=9$, see Fig.~14) yield extremely good qualitative forecast for 24\,hrs. ($\Delta_{16}\approx 23$\,km). Nevertheless, the artificial hurricane still does not forecast the turn of the trajectory, and therefore, the error of the forecast for the second 24\,hrs. increases to $\Delta_{19}\approx590$\,km, while $\Delta_{20}\approx 1000$\,km. One can hardly say that the forecast is successful in the region containing the turning point of NICOLE (see Fig.~15). The initial error is $\Delta_{18}\approx84$\,km for $t_{18}$, then it increases approximately by 200\,km every 6\,hrs., so that we obtain $\Delta_{22}\approx780$\,km after 24\,hrs. This failure can easily be explained, since the forecast shown in Fig.~15 is based on the hurricane trajectory till the turn at~$t_{17}$. \begin{figure}[t] \centering \includegraphics[width=0.7\textwidth]{fig22.eps} \caption{\small Initial data: 8.12 $10^{-5}$, ${}-6.63 10^{-3}$, ${}-0.891$, 0.126, ${}-12.6$, 0.363, 0.255, 4.84 $10^{-11}$, ${}-8.22 10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, ${}-10^{-16}$, K=3, M=18. Distances for approximation: 0, 0.09, 0.13, 0.83. Distances for forecast: 1.24, 2.19, 3.43, 4.57, 6.32, 7.28. } \end{figure} After the hurricane changes the direction of its motion, the forecast quality improves to some extent. Here a decisive factor is the fact that we forecast the motion of NICOLE on the basis of its trajectory after the turning point. The plot in Fig.~16 ($K=3$, $M=18$) shows that the trajectories are qualitatively close to one another until the latitude $\approx 37^\circ$ is achieved. Next, under the action of the Coriolis force, the artificial hurricane continues to move to the East, while the actual hurricane moves to the Northeast. An attempt to improve the situation by using a longer prehistory made the forecast quality even worse. Similar pictures are observed for the forecasts starting from~$t_{24}$ and from $t_{28}$: the actual and artificial hurricanes still behave in qualitatively different ways. \begin{figure}[t] \centering \includegraphics[width=0.7\textwidth]{fig28.eps} \caption{\small Probability that center of NICOLE will pass within 75 miles during the 72 hours starting at 10:00 a.m. 30/11 1998 (the National Hurricane Center, USA) Contour levels shown are 10\%, 20\% 50\%, and 100\%. $\xi$ is the track of NICOLE, curve 1 is the solution of (6) for K=3 and M=18, curve 2 is the solution of (6) for K=3 and M=25.} \end{figure} \section{Conclusions} The analysis of numerical results shows that, on all parts of the hurricane track corresponding to more or less stable external factors, the artificial trajectories calculated by the truncated system~(6) (with the initial data corresponding to this particular part) qualitatively and quantitatively coincide to a satisfactory extent with the actual trajectories. This coincidence is rather close in the low latitudes and becomes worse as the hurricane moves to the North. Both facts correspond to an {\it a priori\/} analysis of whether model~(1) is adequate. Therefore, we can draw the conclusion that the truncated system~(6) possesses sufficiently good approximating properties. This conclusion holds for a time interval of several days. However, to use the truncated system~(6) on larger time intervals is rather problematic. The plots in Figs.~4,~5 clearly demonstrate that there are restrictions on the long term applicability of this system. The trajectory ``breakdown'' (after the calculation time $\approx 150$\,hrs.) is closely related to an increase in the error arising due to the truncation of the infinite system of equations. Similar ``breakdowns'' can be seen in other figures, however, they occur at a considerable distance from the trajectory of the actual hurricane. Thus the error due to the truncation manifests itself after sufficiently large time and is unessential for short-term and medium-term forecast. Next, numerical results obtained do not allows us to hope that a good forecast can be obtained by using~(6) in the case of a sharp change in the trajectory. The hurricane NICOLE gives the most illustrative example of this fact. There is no doubt that this fact is closely related to the defects of the initial model~(1). In order to estimate the results of numerical experiments, let us compare the artificial trajectory of NICOLE with the probability forecast made by the National Hurricane Center at 10:00 a.m. 30/11/1998. This forecast was made almost at the same time as our forecast shown in Fig.~16, since the choice $K=3$, $M=18$ implies the absolute time $t_{21}=\mbox{09:00}$ a.m. 30/11/1998. The comparison of the probability forecast with the actual NICOLE trajectory for $t>t_{21}$ (see Fig.~17) shows that during 36\,hrs. the actual hurricane approaches the 20\% region and then, after 3\,days, enters the 10\% region. This means that the predicted probability $p=0.8$ (that the eye of NICOLE stays in the 20\% region during 72\,hrs.) is too excessive. Only the probability $p=0.9$ (that NICOLE stays in a considerably larger 10\% region) is adequate. The forecast obtained by using system~(6) (for $K=3$, $M=18$, curve~1 in Fig.~17) predicts that the trajectory leaves the 20\% region during 36\,hrs. In this sense our forecast is even better than the professional forecast. However, as shown above, the artificial trajectory qualitatively differs from the actual trajectory. We can partially improve this forecast by using the dynamical correction (curve~2 in Fig.~17). Thus, although the basic model~(1) is rough, the quality of our forecast is comparable (even if somewhat worse) with the quality of the professional forecast. All numerical experiments resulted in a sufficiently good forecast for 24--48\,hrs. Apparently, the forecast of extremely high quality in Fig.~4 (more than for 5\,days) is accidental. Nevertheless, several successful medium-term forecasts, including the 3-day forecasts (Figs.~3,~11) make us optimistic. Finally, the results obtained show that the following fundamental hypotheses hold: \begin{itemize} \item Methods of the theory of generalized functions can be used for calculating the dynamics of a hurricane; \item A hurricane can be treated as a weak pointwise singularity; \item The singularity dynamics can be calculated by using a truncated sequence of Hugoniot type conditions. \end{itemize} It is highly probable that we can improve the quality of short-term and medium-term forecasts by choosing a basic model that is more adequate than model~(1). \begin{thebibliography}{99} \frenchspacing \bibitem{1} E.~E.~Gossard and W.~H.~Hooke, {\em Waves in the Atmosphere}, Elsevier, Amsterdam, 1975. \bibitem{2} E.~Lorenz, {\em Nature and Theory of General Circulation in the Atmosphere\/} [Russian Translation], Gidrometeoizdat, Leningrad, 1971. \bibitem{3} A.~M.~Obukhov, {\em On the geostrophic wind problem}, Izv. Akad. Nauk SSSR, Ser. 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Notes in Math., vol.{\bf401}, Chapman and Hall, London, 1999, 63--74. \end{thebibliography} \noindent\textsc{Vladimir Danilov} (e-mail: pm@miem.edu.ru)\\ \textsc{Georgii Omel'yanov}\\ \textsc{Daniil Rozenknop}\\[3pt] Moscow State Institute of Electronics and Mathematics, \\ B. Trekhsvyatitel'skii per., 3/12, \\ Moscow 109028, Russia \end{document}