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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。 ZO$T/GE6% |^!@ 成像示意图 84cH|j`w 首先我们建立十字元件命名为Target K<(sqH ^PpFI 创建方法: k=
1+mG <7) 6*u 面1 : K7Tell\` 面型:plane N'.+ezZ;h 材料:Air "b7C0NE 孔径:X=1.5, Y=6,Z=0.075,形状选择Box bUL9*{>G )C6 7qY[P 1OS3Gv8jc~ 辅助数据: <-aI%'?* 首先在第一行输入temperature :300K, k] YGD emissivity:0.1; S3wH
M uS,$P34^oy `vBa.)u 面2 : W<l(C!{ 面型:plane {mGWMv 材料:Air l))IO`s=_ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box T0jJp7O NWj@iyi< kJFHUR 位置坐标:绕Z轴旋转90度, !%9I%Ak^ zf u78 Gjr2]t;E 辅助数据: 9B0"GEwrs lNAHn<ht 首先在第一行输入temperature :300K,emissivity: 0.1; r U5'hK
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I:=C %Ski5q Target 元件距离坐标原点-161mm; E3.s8}} )FPbE^s( "
z{w^k 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 :LG%8Z{R 4y.[tk5 1fZ:^|\ 探测器参数设定: H)tDfk sq\ K(S/D(\
FL 在菜单栏中选择Create/Element Primitive /plane k6S<46}h| Y?cw9uYB Q8i6kf! 2=EKAg=S O1,[7F.4g T(F8z5s5 元件半径为20mm*20,mm,距离坐标原点200mm。 gZv<_0N ;"z>p25=T 光源创建: O6]~5&8U. [DwB7l)O( 光源类型选择为任意平面,光源半角设定为15度。 <&iBR -&}E:zoe
%\0 Y1!Hw 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。 ) /'s&
D (P-<9y@ 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。 P_U-R%f y
rk#)@/m +&@0;zSga 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。 5>Q)8`@E X $f%Ss 创建分析面: iXFaQ E12k1gC` T^_9R; 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 ZI7<E se[};t: 0J~4
到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 3
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;hg# -wB AFr FRED在探测器上穿过多个像素点迭代来创建热图 C#>C59 cht#~d FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 "L]_NST 将如下的代码放置在树形文件夹 Embedded Scripts, S J5kA` S6]': {Y Ymt!Ic 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 )Yml'?V" \~PFD%]:3 绿色字体为说明文字, MXb(Z9)]kw 0N.*c '#Language "WWB-COM" YVT^}7# 'script for calculating thermal image map *C \O]r:' 'edited rnp 4 november 2005 OjZ@_V: N2>JG]G 'declarations )c/]
8KU Dim op As T_OPERATION RulIzv Dim trm As T_TRIMVOLUME 9[`6f8S_$ Dim irrad(32,32) As Double 'make consistent with sampling 9\F^\h{ Dim temp As Double -g0>>{M' Dim emiss As Double jJ|;Nwm<[ Dim fname As String, fullfilepath As String #^Y,,GA scdT/|(U$ 'Option Explicit r`2& o =R05H2hs Sub Main amRtFrc| 'USER INPUTS #XsqTK_nk nx = 31 o&]qjFo\m ny = 31 {%
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numRays = 1000 rfjQx]3pB minWave = 7 'microns (k?OYz]c maxWave = 11 'microns VI?[8@*Z sigma = 5.67e-14 'watts/mm^2/deg k^4 xk/(|f{L fname = "teapotimage.dat" om1 /9 ]arP6iN+ Print "" ,O}zgf*H; Print "THERMAL IMAGE CALCULATION" :O7J9K| )Ii=8etdv detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 v,jU9D\ 5M*p1^ > Print "found detector array at node " & detnode [Mi~4b mWh:,[o srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 ,f$RE6 *4ID$BmO Print "found differential detector area at node " & srcnode 9cLKb LE;c+(CAU GetTrimVolume detnode, trm ,0~=9dR detx = trm.xSemiApe 2,+H;Ypi! dety = trm.ySemiApe @bZb#,n] area = 4 * detx * dety d^7<l_u~ ! Print "detector array semiaperture dimensions are " & detx & " by " & dety >_@J&vC Print "sampling is " & nx & " by " & ny SC# FEkx&9] 'reset differential detector area dimensions to be consistent with sampling >(3y(1; pixelx = 2 * detx / nx [lf[J&}X pixely = 2 * dety / ny 5q\]] LV> SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False PYZ8@G Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 H_{Yr+p Q-\: u~ 'reset the source power 1peN@Yk2W SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) aa|xZ Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" \|M z'* fIu/*PFPVY 'zero out irradiance array K$4Ky&89
For i = 0 To ny - 1 v"`w'+ For j = 0 To nx - 1 n'SnqJ&} irrad(i,j) = 0.0 s^cHR1^ Next j {'/8{dS Next i +:b|I'S ?n}L+| 'main loop =vR>KE EnableTextPrinting( False ) MD +Q_ NOvN8.K% ypos = dety + pixely / 2 j*GYYEY For i = 0 To ny - 1 S;Vj5 xpos = -detx - pixelx / 2 |g~.]2az ypos = ypos - pixely dI`b AP;\ r'&VH]m EnableTextPrinting( True ) T!8,R{V]4 Print i GE|V^_|i EnableTextPrinting( False ) p &A3l 9BP-Iet 2gA6$s7 For j = 0 To nx - 1 T5ol2 YtFtU;{ xpos = xpos + pixelx yovC~ ]`LMyt0 'shift source Hd
:2 LockOperationUpdates srcnode, True )<%GHDWL GetOperation srcnode, 1, op {<V{0
s% op.val1 = xpos Z\n
nVM= op.val2 = ypos 06ZyR@.@v SetOperation srcnode, 1, op 6]M(ElV1H LockOperationUpdates srcnode, False l2i[wc"9 Z<`QDBN"4 'raytrace |Gz(q4 DeleteRays ,#nyEE CreateSource srcnode Mp}U>+8 TraceExisting 'draw s$A|>TOY _qr?v=,-A 'radiometry 'bTtdFvJ For k = 0 To GetEntityCount()-1 r+>gIX+Fl If IsSurface( k ) Then MGK%F#PM temp = AuxDataGetData( k, "temperature" ) qeypa! emiss = AuxDataGetData( k, "emissivity" ) af)L+%Q%R If ( temp <> 0 And emiss <> 0 ) Then V!uW\i/ ProjSolidAngleByPi = GetSurfIncidentPower( k ) u{J$]%C
frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) 4PR!OB irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi "_W[X End If f-^JI*hj S/V%<<[>p] End If 5y0N }} RGsgT ^ Next k bZLY#g7L" ]@0C1r Next j F P3{Rp XU_gvz Next i <v%Q|r EnableTextPrinting( True ) qx|~H'UuBN -e(e;e 'write out file G0)}?5L1J fullfilepath = CurDir() & "\" & fname 3s;^p,9
Y Open fullfilepath For Output As #1 x. 8fxogz Print #1, "GRID " & nx & " " & ny 5<YV`T{5Kl Print #1, "1e+308" ~wvu7 Print #1, pixelx & " " & pixely &.F]-1RN[ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 _\;0E!=p *PM#ngLX}r maxRow = nx - 1 T\q: maxCol = ny - 1 S"HdjEF7\ For rowNum = 0 To maxRow ' begin loop over rows (constant X) }p5_JXBV row = "" r'8qZJgm For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) ~bf4_5 row = row & irrad(colNum,rowNum) & " " ' append column data to row string c^3,e/H Next colNum ' end loop over columns a@!(o )> AT%6K. Print #1, row x n?$@ 0Xb,ne
7 Next rowNum ' end loop over rows bI+/0Xx Close #1 R#HVrzOO|T 2D UY4Ti Print "File written: " & fullfilepath [n4nnmM Print "All done!!" GHY+q{'#V_ End Sub fJOwE
g| 7>"dc+Fg 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: C~Hhi-Xl) BMug7xl" PzOnS 找到Tools工具,点击Open plot files in 3D chart并找到该文件 9fm9xTL 1_WP\@O SSxp!E' 打开后,选择二维平面图: #/_{(P ncqAof(/
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