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简介:本文是以十字元件为背景光源,经过一个透镜元件成像在探测器上,并显示其热成像图。 ]$xN`O4W{ (Tbw@BFk 成像示意图 =c1t]%P, 首先我们建立十字元件命名为Target hrZ=8SrW Qf<@
:T* 创建方法: P{{U *5Aq\g,n 面1 : gsD0N^ 面型:plane -'wFaW0%I 材料:Air B(l8&
孔径:X=1.5, Y=6,Z=0.075,形状选择Box %yJ
$R2%*y <&Q(I+^ qTd6UKg 辅助数据: 0s+pcqOd^ 首先在第一行输入temperature :300K, w=K!U] emissivity:0.1; CDRkH)~$ dXvp-oi n>[" h2 面2 : 1-6[KBQ8 面型:plane ^V5g[XL2 材料:Air @2eV^eO9 孔径:X=1.5, Y=6,Z=0.075,形状选择Box o;\c$|TNU IP
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位置坐标:绕Z轴旋转90度, .dStV6 Ohe*m[ LnY`f -H 辅助数据: wEp*j+Mmce H6Qb]H.C 首先在第一行输入temperature :300K,emissivity: 0.1; ;;cPt44s hD I}V1) KWzJ Target 元件距离坐标原点-161mm; "2FI3M= `x'vF# pS
C5$a( 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 R]8^
@i1 1E'/! | j^&{5s 探测器参数设定: E
02l=M 4X^{aIlshk 在菜单栏中选择Create/Element Primitive /plane ; Da[jFP tm[e?+Iq `4N{x.N ['l.]k-b} @T6Z3Zj} tEE1`10Mt 元件半径为20mm*20,mm,距离坐标原点200mm。 J|D$ $4j$c|S! 光源创建: 5W29oz}-S Y=- ILN(" 光源类型选择为任意平面,光源半角设定为15度。 _\y%u_W i$Sq.NU *i>?YT 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 49("$! sivd@7r\Fa 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 53w@ 1p[Z`m*9 /#,3JU$w 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 O!c b- eyiGe1^C 创建分析面: UI,i2<& aeBA`ry"B )E2^G)J$W 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 Po:)b 4p%=8G| qPc"A!-i 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 !QB(M@1 ~
}<!ON; FRED在探测器上穿过多个像素点迭代来创建热图 d/57;6I_ 4ZZ/R?AiK FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 "^~>aVuXf 将如下的代码放置在树形文件夹 Embedded Scripts, '<v/Gl\ KvM}g2" *1Lkde@|{ 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 ?d -$lI j|u6TG 绿色字体为说明文字, !U@?Va~Zn 4}~zVT0'~ '#Language "WWB-COM" 4gTD HQP 'script for calculating thermal image map `z=I}6){ 'edited rnp 4 november 2005 GYD` |$r|DX1[ 'declarations Q&Rj)1! Dim op As T_OPERATION s^/<6kwO Dim trm As T_TRIMVOLUME *N0R3da Dim irrad(32,32) As Double 'make consistent with sampling 4No!`O-!& Dim temp As Double *j,5TO-j Dim emiss As Double 4s!rrDN Dim fname As String, fullfilepath As String ldJ:A*/M6 Q1G?e,Q 'Option Explicit iB Ld*B|#K o,!r t1&0 Sub Main X5'QYZ6kv 'USER INPUTS 2VOdI nx = 31 V}#2pP ny = 31 R~,*W1G6sF numRays = 1000 .TN9N minWave = 7 'microns a*}ZT,V maxWave = 11 'microns CW(]6s u{ sigma = 5.67e-14 'watts/mm^2/deg k^4 zS*X9|p fname = "teapotimage.dat" bF88F_ '"H'#%RU Print "" H1PW/AW Print "THERMAL IMAGE CALCULATION" ^X%{]b K tQy@d_a=y detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 _5^p+ zMT0ToG Print "found detector array at node " & detnode 7Q<xC ;as4EqiK srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 ;r[@;2p*( &~+lXNXF Print "found differential detector area at node " & srcnode [@OXvdTV #\G{2\R GetTrimVolume detnode, trm 6]dK, detx = trm.xSemiApe Kc= &jCn dety = trm.ySemiApe FAVw80?5k area = 4 * detx * dety &|7pu= Print "detector array semiaperture dimensions are " & detx & " by " & dety !2WRxM Print "sampling is " & nx & " by " & ny r"OVu~ND [X.sCl| 'reset differential detector area dimensions to be consistent with sampling 8t!/Op? pixelx = 2 * detx / nx v\#69J5.>) pixely = 2 * dety / ny @x">e][B SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False %|[+\py$Q Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 />(e.)f y; Up@.IG 'reset the source power *5iNw_& SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) &ZgB b Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" mh>)N" 4,kT4_&, 'zero out irradiance array N^A&DrMF For i = 0 To ny - 1 fr8:L!9 For j = 0 To nx - 1 F{\MIuoy irrad(i,j) = 0.0 |s
:b9sfA Next j 5QU7!jbI Next i Wa%Zt*7 }3cOZd_,t 'main loop <;:M:{RZY EnableTextPrinting( False ) \3(d$_:b :e:jILQ[ ypos = dety + pixely / 2 2~+_T For i = 0 To ny - 1 r#wMd9]) xpos = -detx - pixelx / 2 0n+Wv@/ ypos = ypos - pixely yzW9A=0A) Q*mzfsgr EnableTextPrinting( True ) jQOY \1SR Print i Af5O;v\ EnableTextPrinting( False ) QIVpO /@ ,x}p1EZ L)JpMf0 For j = 0 To nx - 1 /u{ 9UR[g u1O?` xpos = xpos + pixelx
.Ya]N+r* ^EE3E' 'shift source uBw1Xud[YI LockOperationUpdates srcnode, True Q4r)TR , GetOperation srcnode, 1, op ?J,hv'L] op.val1 = xpos ?c0OrvM op.val2 = ypos e&?o SetOperation srcnode, 1, op P0,)
Gw LockOperationUpdates srcnode, False 0\O*\w? n.p6+^ES raytrace ZurQr} DeleteRays u&1n~t` CreateSource srcnode :<4:h.gO8 TraceExisting 'draw oHdss;q ;AK;% 'radiometry J6/Mm7R For k = 0 To GetEntityCount()-1 bvzeUn If IsSurface( k ) Then h7<Zkf temp = AuxDataGetData( k, "temperature" ) \ Xow#@[ emiss = AuxDataGetData( k, "emissivity" ) O{rgx~lLJt If ( temp <> 0 And emiss <> 0 ) Then _ In[Z?P} ProjSolidAngleByPi = GetSurfIncidentPower( k ) C#[YDcp4 frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) u}hQF$a" irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi .g_BKeU End If [4sI<aH !xyO End If =wHHR1e saQA:W; Next k R4GmUCKB= <T{2a\i 4f Next j !/, 6+2Ru oomB/"Z Next i [,)yc/{* EnableTextPrinting( True ) |xyr6gY @54, I 'write out file i"2[OM\j7 fullfilepath = CurDir() & "\" & fname #<|5<U Open fullfilepath For Output As #1 FU/yJy Print #1, "GRID " & nx & " " & ny Yi1*o? Print #1, "1e+308" ZeD; Print #1, pixelx & " " & pixely +hL+3`TD#H Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 E"!C3SC [ pisjfNT`o maxRow = nx - 1 q/-8sO}q maxCol = ny - 1 e_s9E{( For rowNum = 0 To maxRow ' begin loop over rows (constant X) !U.Xb6 row = "" fI(u-z~, For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) z)"7qqA row = row & irrad(colNum,rowNum) & " " ' append column data to row string ^~}|X%q3 Next colNum ' end loop over columns T0n=nC}< 9{@ #tx Print #1, row ""l_&3oz G%~=hEK0 Next rowNum ' end loop over rows rks+\e}^Z Close #1 ~8~B VwZ_ $~c?qU Print "File written: " & fullfilepath GgkljF@{} Print "All done!!" yyZH1A End Sub "8|y Wh[+cH"M 在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: :Z(?Ct&8 Srj%6rgsB p%e!&:! 找到Tools工具,点击Open plot files in 3D chart并找到该文件 0-cqux2U |qbCmsY5/ !
{lcF% 打开后,选择二维平面图: I7b(fc-r `EVTlq@<
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