我有一个问题,经过多次挠头,我认为这与长双打中非常小的数字有关。
我正在尝试实现普朗克定律方程,以在给定波长范围和给定温度之间以 1nm 的间隔生成归一化黑体曲线。最终这将是一个接受输入的函数,现在它是 main(),变量固定并由 printf() 输出。
我在matlab和python中看到了示例,它们在类似的循环中实现了与我相同的方程,完全没有问题。
这是等式:
我已经独立测试了代码的关键部分。在尝试通过在 excel 中将方程分解成块来测试方程后,我注意到它确实会产生非常小的数字,我想知道我对大数字的实现是否会导致问题?有没有人对使用 C 来实现方程有任何见解?这对我来说是一个新领域,我发现数学比普通代码更难实现和调试。
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
//global variables
const double H = 6.626070040e-34; //Planck's constant (Joule-seconds)
const double C = 299800000; //Speed of light in vacume (meters per second)
const double K = 1.3806488e-23; //Boltzmann's constant (Joules per Kelvin)
const double nm_to_m = 1e-6; //conversion between nm and m
const int interval = 1; //wavelength interval to caculate at (nm)
//typedef structure to hold results
typedef struct {
int *wavelength;
long double *radiance;
long double *normalised;
} results;
int main() {
int min = 100 , max = 3000; //wavelength bounds to caculate between, later to be swaped to function inputs
double temprature = 200; //temprature in kelvin, later to be swaped to function input
double new_valu, old_valu = 0;
static results SPD_data, *SPD; //setup a static results structure and a pointer to point to it
SPD = &SPD_data;
SPD->wavelength = malloc(sizeof(int) * (max - min)); //allocate memory based on wavelength bounds
SPD->radiance = malloc(sizeof(long double) * (max - min));
SPD->normalised = malloc(sizeof(long double) * (max - min));
for (int i = 0; i <= (max - min); i++) {
//Fill wavelength vector
SPD->wavelength[i] = min + (interval * i);
//Computes radiance for every wavelength of blackbody of given temprature
SPD->radiance[i] = ((2 * H * pow(C, 2)) / (pow((SPD->wavelength[i] / nm_to_m), 5))) * (1 / (exp((H * C) / ((SPD->wavelength[i] / nm_to_m) * K * temprature))-1));
//Copy SPD->radiance to SPD->normalised
SPD->normalised[i] = SPD->radiance[i];
//Find largest value
if (i <= 0) {
old_valu = SPD->normalised[0];
} else if (i > 0){
new_valu = SPD->normalised[i];
if (new_valu > old_valu) {
old_valu = new_valu;
}
}
}
//for debug perposes
printf("wavelength(nm) radiance(Watts per steradian per meter squared) normalised radiance\n");
for (int i = 0; i <= (max - min); i++) {
//Normalise SPD
SPD->normalised[i] = SPD->normalised[i] / old_valu;
//for debug perposes
printf("%d %Le %Lf\n", SPD->wavelength[i], SPD->radiance[i], SPD->normalised[i]);
}
return 0; //later to be swaped to 'return SPD';
}
/************************更新 2017 年 3 月 24 日星期五 23:42************************ *****/
到目前为止,感谢您的建议,许多有用的指针特别是了解数字在 C ( IEEE 754 ) 中的存储方式,但我认为这不是这里的问题,因为它仅适用于有效数字。我实施了大部分建议,但在这个问题上仍然没有进展。我怀疑评论中的 Alexander 可能是对的,我可能需要更改操作的单位和顺序才能使方程式像 matlab 或 python 示例一样工作,但我的数学知识不足以做到这一点。我把方程分解成几块,仔细看看它在做什么。
//global variables
const double H = 6.6260700e-34; //Planck's constant (Joule-seconds) 6.626070040e-34
const double C = 299792458; //Speed of light in vacume (meters per second)
const double K = 1.3806488e-23; //Boltzmann's constant (Joules per Kelvin) 1.3806488e-23
const double nm_to_m = 1e-9; //conversion between nm and m
const int interval = 1; //wavelength interval to caculate at (nm)
const int min = 100, max = 3000; //max and min wavelengths to caculate between (nm)
const double temprature = 200; //temprature (K)
//typedef structure to hold results
typedef struct {
int *wavelength;
long double *radiance;
long double *normalised;
} results;
//main program
int main()
{
//setup a static results structure and a pointer to point to it
static results SPD_data, *SPD;
SPD = &SPD_data;
//allocate memory based on wavelength bounds
SPD->wavelength = malloc(sizeof(int) * (max - min));
SPD->radiance = malloc(sizeof(long double) * (max - min));
SPD->normalised = malloc(sizeof(long double) * (max - min));
//break equasion into visible parts for debuging
long double aa, bb, cc, dd, ee, ff, gg, hh, ii, jj, kk, ll, mm, nn, oo;
for (int i = 0; i < (max - min); i++) {
//Computes radiance at every wavelength interval for blackbody of given temprature
SPD->wavelength[i] = min + (interval * i);
aa = 2 * H;
bb = pow(C, 2);
cc = aa * bb;
dd = pow((SPD->wavelength[i] / nm_to_m), 5);
ee = cc / dd;
ff = 1;
gg = H * C;
hh = SPD->wavelength[i] / nm_to_m;
ii = K * temprature;
jj = hh * ii;
kk = gg / jj;
ll = exp(kk);
mm = ll - 1;
nn = ff / mm;
oo = ee * nn;
SPD->radiance[i] = oo;
}
//for debug perposes
printf("wavelength(nm) | radiance(Watts per steradian per meter squared)\n");
for (int i = 0; i < (max - min); i++) {
printf("%d %Le\n", SPD->wavelength[i], SPD->radiance[i]);
}
return 0;
}
xcode中运行时的方程变量值: