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Solar 的代码
ss_proj.m
% SS_PROJ Projects all cell albedo contributions onto the solar cell normal
% in ECEF. This value is equivalent to the total perpendicular irradiance
% reaching the solar cell.
%
% P = ss_proj(re,
eclipse_resin_struts_integration.xml
Eclipse Resin Struts 集成开发 Step by step
中文
bAyARd@SolAR
原创培训资料
NA
1
solar.cpp
//SOLAR.CPP--Example from Chapter 3, "An Introduction to C++"
#include
#include
#include
struct planet {
char name[10];
float distance;
float radius;
slrgen.f
subroutine slrgen(j)
!! ~ ~ ~ PURPOSE ~ ~ ~
!! this subroutine generates solar radiation
!! ~ ~ ~ INCOMING VARIABLES ~ ~ ~
!! name |units |definition
!!
smeas.f
subroutine smeas
!! ~ ~ ~ PURPOSE ~ ~ ~
!! this subroutine reads in daily solar radiation data and assigns the
!! values to the proper HRUs
!! ~ ~ ~ INCOMING VARIABLES
solar.cpp
//SOLAR.CPP--Example from Chapter 3, "An Introduction to C++"
#include
#include
#include
struct planet {
char name[10];
float distance;
float radius;
solar.m
%SOLAR Solar irradiance spectra
%
% p = SOLAR(lambda)
%
% Return solar irradiance in W/m2/nm for wavelength specified.
% Lambda maybe a vector.
%
% Data from http://www.asdi.com/apps/arm.html, figu
http:^^solar.rtd.utk.edu^~china^china.html
Date: Wed, 15 Jan 1997 00:45:06 GMT
Server: Apache/1.1.1
Content-type: text/html
Content-length: 3701
Last-modified: Fri, 07 Jun 1996 02:16:58 GMT
Connection: Keep-Alive
Keep-Alive: timeout=15,
solar.cpp
//SOLAR.CPP--Example from Chapter 3, "An Introduction to C++"
#include
#include
#include
struct planet {
char name[10];
float distance;
float radius;
solar.m
%SOLAR Solar irradiance spectra
%
% p = SOLAR(lambda)
%
% Return solar irradiance in W/m2/nm for wavelength specified.
% Lambda maybe a vector.
%
% Data from http://www.asdi.com/apps/arm.html, figu