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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。 xI~AZ:m P=6d<no&< 成像示意图 &43c/TSb 首先我们建立十字元件命名为Target I,`;#Q)nx 8DY:a['-d 创建方法: Cl-P6NlR". OK8Ho" 面1 : ".waCt6 面型:plane WSN^iDS 材料:Air xkax 孔径:X=1.5, Y=6,Z=0.075,形状选择Box F",TP,X iyd$_CJ z q=D8 Nz 辅助数据: %KkC1.yu< 首先在第一行输入temperature :300K, G2?#MO emissivity:0.1; `j9\]50Z> -aS@y.z @"1Z;.S8V 面2 : u'Q82l&Y 面型:plane ,\c V,$ 材料:Air t[|t0y8 孔径:X=1.5, Y=6,Z=0.075,形状选择Box HGh
-rEh NsSZ?ky _aF8Us 位置坐标:绕Z轴旋转90度, ir>h3Zk N3aqNRwlk ZfH>UHft 辅助数据: .P/0`A{& qNP)oU92 首先在第一行输入temperature :300K,emissivity: 0.1; O(!;7v} L8!yP.3 i*m;kWu, Target 元件距离坐标原点-161mm; xW*Lceb &rD8ng+$ YG8V\4
SQ 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 *PV"&cx 9_iwikD c%^B
' 探测器参数设定: J -Lynvqm c s*E9 在菜单栏中选择Create/Element Primitive /plane 1'Q6l (=;'>*L( %.r\P@7/Q 2,`X@N`\ qHdUnW k'H[aYMA 元件半径为20mm*20,mm,距离坐标原点200mm。 O6)Po +6P[TqR 光源创建: : [328X2 v
@0G^z| 光源类型选择为任意平面,光源半角设定为15度。 U5H%wA['m 5 QuRwu_ s(5hFuyg 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。 C$~ly=@
zhd1)lgY 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。 CJ%'VijhD 0F%8d@Y2 ~ZSX84~@u 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。 ]k^?= O65`KOPn 创建分析面: +h+ 7Q'k ?O#,{ZZf= }Oc+EV-Z 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。 OUF%DMl4 :i?6#_2IC <nD@4J-A0 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。 .Y]0gi8z tzGQo5\ FRED在探测器上穿过多个像素点迭代来创建热图 k?&GL!? c1s& 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。 -V}xvSVg 将如下的代码放置在树形文件夹 Embedded Scripts, OObAn^bt xatq O!f37n-TB 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。 UCfouQ Cj *8?2+)5" 绿色字体为说明文字, 8P-ay<6 P658
XKE '#Language "WWB-COM" !37I2*+4 'script for calculating thermal image map i]?
Eq?k 'edited rnp 4 november 2005 >| ,`E
U\:Y*Ai 'declarations 7:pc%Ksq Dim op As T_OPERATION IJ2' Dim trm As T_TRIMVOLUME @XM*N7 Dim irrad(32,32) As Double 'make consistent with sampling y-nv#Ejr Dim temp As Double wzju)q S Dim emiss As Double 6P717[ Dim fname As String, fullfilepath As String 2p](`Y` cpP}NJb0;% 'Option Explicit ^O@eyP 6wWhM&Wd Sub Main =KOi#;1 'USER INPUTS pMHl<HH nx = 31 ^U5N!"6R ny = 31 v9*+@ numRays = 1000 ~&T U minWave = 7 'microns Oj _]` maxWave = 11 'microns /tj]^QspS sigma = 5.67e-14 'watts/mm^2/deg k^4 T[1iZ fname = "teapotimage.dat" [niFJIsc WXmfh Print "" Vlz\n Print "THERMAL IMAGE CALCULATION" .G\](% a'jUM+D; detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 nfHjIYid DoQ^caa@ Print "found detector array at node " & detnode bH/4f93Nb I]W7FZ=o srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 i@?|vu mih}?oi Print "found differential detector area at node " & srcnode {c_bNYoE sGhw23 GetTrimVolume detnode, trm -+1O*L! detx = trm.xSemiApe 0~RD@>] dety = trm.ySemiApe E7\K{] area = 4 * detx * dety $%DoLpE> Print "detector array semiaperture dimensions are " & detx & " by " & dety 2?q>yL! Gz Print "sampling is " & nx & " by " & ny TCRTC0_}k 2yn"K| 'reset differential detector area dimensions to be consistent with sampling {v]L|e%{ pixelx = 2 * detx / nx B<r0y pixely = 2 * dety / ny )4B`U(%M~ SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False X/:V{2 Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 K
|=o - |}z5ST% 'reset the source power EIQ3vOq6 SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) X[dfms;H Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" _";w*lg} & tT6.@kH 'zero out irradiance array _ncBq;j{ For i = 0 To ny - 1 <lIm==U<- For j = 0 To nx - 1 i*:QbMb irrad(i,j) = 0.0 )r{Wj*u Next j e`={_R{N Next i K2x2Y= DVhBZ!u9 'main loop CUH u= EnableTextPrinting( False ) w%qnH e9 RN)XIf$@_ ypos = dety + pixely / 2 lmHQ"z 3G For i = 0 To ny - 1 ~HGSA( xpos = -detx - pixelx / 2 80lhhqRC ypos = ypos - pixely h.#:7d(g EoPvF`T EnableTextPrinting( True ) R_/;U&R Print i RRS)7fFm EnableTextPrinting( False ) 0M;El2
P$ s(Gs?6}>T AYY(<b For j = 0 To nx - 1
zo@vuB. Pah@d!%A xpos = xpos + pixelx WcSvw e< @$(w 'shift source r-$xLe7a LockOperationUpdates srcnode, True )C?H m^# GetOperation srcnode, 1, op MMKN^a"GA op.val1 = xpos
\8C<nh op.val2 = ypos AFL'Ox]0 SetOperation srcnode, 1, op <B|b'XVH2 LockOperationUpdates srcnode, False Ln&~t(7 =dNE1rdzNa 'raytrace T:kliM"z DeleteRays qB_s<cpn> CreateSource srcnode J1O1! . TraceExisting 'draw wX2U
AP>n-Z| 'radiometry $s}w23nB For k = 0 To GetEntityCount()-1 jq]5Y^e If IsSurface( k ) Then R- >~MLeK] temp = AuxDataGetData( k, "temperature" ) x#SE%j? emiss = AuxDataGetData( k, "emissivity" ) g$e|y#Ic$ If ( temp <> 0 And emiss <> 0 ) Then z@e(y@ ProjSolidAngleByPi = GetSurfIncidentPower( k ) C1_0 9Vc frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) 3S_H&>K irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi M}X ` End If H%l-@::+$ LYYz=oZOE! End If ~v\
W[ QlB9m2XB Next k .
U6(>6- u*%mUh Next j }[|9vF"g.y |$IL:W6 Next i u8JH~b EnableTextPrinting( True ) LyvR].p=5* egA*x*8 'write out file {06-h %qr fullfilepath = CurDir() & "\" & fname ?QFxds Open fullfilepath For Output As #1 Zl9 Print #1, "GRID " & nx & " " & ny j<!dpt Print #1, "1e+308" qm/>\4eLt Print #1, pixelx & " " & pixely $LuU Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 $2*_7_Qb qY%|Uo maxRow = nx - 1 4=^Ha%l maxCol = ny - 1 4|%Y09"lv For rowNum = 0 To maxRow ' begin loop over rows (constant X) -32P}58R row = "" Zbre5&aU For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) ]Kjt@F"; row = row & irrad(colNum,rowNum) & " " ' append column data to row string p8j4Tc5tQ> Next colNum ' end loop over columns E7R%G OH dKEy6C"@ Print #1, row a,4GE' 2K/t[.8 Next rowNum ' end loop over rows -a|b.p Close #1 F(/<ADx tR9iFv_ Print "File written: " & fullfilepath I&i6-xp Print "All done!!" $FT6c@&y End Sub Jo[&y, R*cef 在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: Or$"f3gq O\cc=7 'tkQz 找到Tools工具,点击Open plot files in 3D chart并找到该文件 &X~8S/nPAw F> Ika=z, k9H}nP$F 打开后,选择二维平面图: $$p +~X T; [T`
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