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\chapter[CAMAL: Celestial Mechanics]{CAMAL: Calculations in Celestial Mechanics} \label{CAMAL} \typeout{{CAMAL: Calculations in Celestial Mechanics}} {\footnotesize \begin{center} J. P. Fitch \\ School of Mathematical Sciences, University of Bath\\ BATH BA2 7AY, England \\[0.05in] e--mail: jpff@cs.bath.ac.uk \end{center} } \ttindex{CAMAL} The CAMAL package provides facilities for calculations in Fourier series similar to those in the specialist Celestial Mechanics system of the 1970s, and the Cambridge Algebra system in particular.\index{Fourier Series}\index{CAMAL}\index{Celestial Mechanics} \section{Operators for Fourier Series} \subsection*{\f{HARMONIC}}\ttindex{HARMONIC} The celestial mechanics system distinguish between polynomial variables and angular variables. All angles must be declared before use with the \f{HARMONIC} function. \begin{verbatim} harmonic theta, phi; \end{verbatim} \subsection*{\f{FOURIER}}\ttindex{FOURIER} The \f{FOURIER} function coerces its argument into the domain of a Fourier Series. The expression may contain {\em sine} and {\em cosine} terms of linear sums of harmonic variables. \begin{verbatim} fourier sin(theta) \end{verbatim} Fourier series expressions may be added, subtracted multiplies and differentiated in the usual \REDUCE\ fashion. Multiplications involve the automatic linearisation of products of angular functions. There are three other functions which correspond to the usual restrictive harmonic differentiation and integration, and harmonic substitution. \subsection*{\f{HDIFF} and \f{HINT}}\ttindex{HDIFF}\ttindex{HINT{}} Differentiate or integrate a Fourier expression with respect to an angular variable. Any secular terms in the integration are disregarded without comment. \begin{verbatim} load_package camal; harmonic u; bige := fourier (sin(u) + cos(2*u)); aa := fourier 1+hdiff(bige,u); ff := hint(aa*aa*fourier cc,u); \end{verbatim} \subsection*{\f{HSUB}}\ttindex{HSUB} The operation of substituting an angle plus a Fourier expression for an angles and expanding to some degree is called harmonic substitution. The function takes 5 arguments; the basic expression, the angle being replaced, the angular part of the replacement, the fourier part of the replacement and a degree to which to expand. \begin{verbatim} harmonic u,v,w,x,y,z; xx:=hsub(fourier((1-d*d)*cos(u)),u,u-v+w-x-y+z,yy,n); \end{verbatim} \section{A Short Example} The following program solves Kepler's Equation as a Fourier series to the degree $n$. \begin{verbatim} bige := fourier 0; for k:=1:n do << wtlevel k; bige:=fourier e * hsub(fourier(sin u), u, u, bige, k); >>; write "Kepler Eqn solution:", bige$ \end{verbatim}