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//SOLAR.CPP--Example from Chapter 3, "An Introduction to C++" #include #include #include struct planet { char name[10]; float distance; float radius;

//SOLAR.CPP--Example from Chapter 3, "An Introduction to C++" #include #include #include struct planet { char name[10]; float distance; float radius;

/* * Solar.h * * Author: Samuel R. Buss * * Software accompanying the book * 3D Computer Graphics: A Mathematical Introduction with OpenGL, * by S. Buss, Cambridge University Press,

/* * Solar.c * * Program to demonstrate how to use a local * coordinate method to position parts of a * model in relation to other model parts. * * Draws a simple solar system, with a s

Microsoft Developer Studio Workspace File, Format Version 6.00 # WARNING: DO NOT EDIT OR DELETE THIS WORKSPACE FILE! ###############################################################################

function [z,sorad]=soradna1(yd,yr,long,lat) % SORADNA1: computes no-sky solar radiation and solar altitude. % [z,sorad]=SORADNA1(yd,yr,long,lat) computes instantaneous values of % solar radiati

%IRRADWINDOW Calculates the irradiation through window % % SYNTAX: E=irrad(Dh,En,iday,LST,gamma,beta) % % OUTPUT: vector E % E(1)= diffuse solar irradiation on an inclined surface % E(2)= dir

//SOLAR.CPP--Example from Chapter 3, "An Introduction to C++" #include #include #include struct planet { char name[10]; float distance; float radius;

;Simplest Solar Window ;Compile and run with F5 format binary use32 xor eax,eax ret

;Simplest Solar Window ;Compile and run with F5 format binary use32 xor eax,eax ret