我有一个问题,在经历了大量的挠头之后,我认为这是一个很小的数字在一个长-双。
我试图实现普朗克定律方程,在给定的波长范围和给定的温度之间,在1nm的间隔内生成一条正常化的黑体曲线。最终,这将是一个接受输入的函数,目前它是main(),变量由printf()固定并输出。
我在matlab和python中看到了一些例子,它们在一个类似的循环中实现了与我相同的等式,一点也不麻烦。
这是方程式

我的代码生成了一个不正确的黑体曲线:

我已经独立测试了代码的关键部分。在尝试通过在excel中将它分解成块来测试这个等式之后,我注意到它确实导致了非常小的数字,我想知道我的大数字的实现是否会导致这个问题?有人对使用C来实现方程有任何见解吗?这对我来说是一个新的领域,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';
}/*********************UPDATE 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,特别是理解数字存储在C (IEEE 754)中的方式,但我不认为这是问题所在,因为它只适用于重要的数字。我执行了大部分建议,但在这个问题上仍未取得进展。我怀疑Alexander在评论中可能是对的,改变单元和操作顺序可能是我需要做的,以使方程像matlab或python示例一样工作,但是我的数学知识还不够好。我把方程式分解成几块,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中运行时的等式变量值:

发布于 2017-03-25 10:39:36
感谢评论中的所有指点。对于其他在用C实现等式时遇到类似问题的人,我在代码中出现了一些愚蠢的错误:
由于最后一个(特别是我没有得到我预期的结果)(我的波长范围不适合绘制我正在计算的温度),这导致我假设方程的实现有问题,特别是我在考虑C中的大数/小数,因为我不理解它们。事实并非如此。
总之,在用代码实现它之前,我应该确保确切地知道在给定的测试条件下应该输出什么公式。我将努力使数学变得更舒服,特别是代数和量纲分析。
下面是作为一个函数实现的工作代码,您可以随意使用它来做任何事情,但是显然没有任何类型的保证等等。
blackbody.c
//
// Computes radiance for every wavelength of blackbody of given temprature
//
// INPUTS: int min wavelength to begin calculation from (nm), int max wavelength to end calculation at (nm), int temperature (kelvin)
// OUTPUTS: pointer to structure containing:
// - spectral radiance (Watts per steradian per meter squared per wavelength at 1nm intervals)
// - normalised radiance
//
//include & define
#include "blackbody.h"
//global variables
const double H = 6.626070040e-34; //Planck's constant (Joule-seconds) 6.626070040e-34
const double C = 299792458; //Speed of light in vacuum (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 calculate at (nm), to change this line 45 also need to be changed
bbresults* blackbody(int min, int max, double temperature) {
double new_valu, old_valu = 0; //variables for normalising result
bbresults *SPD;
SPD = malloc(sizeof(bbresults));
//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));
for (int i = 0; i < (max - min); i++) {
//Computes radiance for every wavelength of blackbody of given temperature
SPD->wavelength[i] = min + (interval * i);
SPD->radiance[i] = ((2 * H * pow(C, 2)) / (pow((SPD->wavelength[i] * nm_to_m), 5))) * (1 / (expm1((H * C) / ((SPD->wavelength[i] * nm_to_m) * K * temperature))));
//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 (int i = 0; i < (max - min); i++) {
//Normalise SPD
SPD->normalised[i] = SPD->normalised[i] / old_valu;
}
return SPD;
}blackbody.h
#ifndef blackbody_h
#define blackbody_h
#include <stdio.h>
#include <math.h>
#include <stdlib.h>
//typedef structure to hold results
typedef struct {
int *wavelength;
long double *radiance;
long double *normalised;
} bbresults;
//function declarations
bbresults* blackbody(int, int, double);
#endif /* blackbody_h */main.c
#include <stdio.h>
#include "blackbody.h"
int main() {
bbresults *TEST;
int min = 100, max = 3000, temp = 5000;
TEST = blackbody(min, max, temp);
printf("wavelength | normalised radiance | radiance |\n");
printf(" (nm) | - | (W per meter squr per steradian) |\n");
for (int i = 0; i < (max - min); i++) {
printf("%4d %Lf %Le\n", TEST->wavelength[i], TEST->normalised[i], TEST->radiance[i]);
}
free(TEST);
free(TEST->wavelength);
free(TEST->radiance);
free(TEST->normalised);
return 0;
}产出图:

https://stackoverflow.com/questions/43005206
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