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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。 LR!%iP "L`BuAB 成像示意图 hO{&bY0 首先我们建立十字元件命名为Target 0VNpd~G$ ?u;m
],w! 创建方法: 9o6[4Q} -sdzA6dp 面1 : b<#zgf 面型:plane ;&f(7 Q+T_ 材料:Air e6H}L:; 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ~%
t'}JDZ 1*$6u5.=F 1zG6^U 辅助数据: *93=}1gN 首先在第一行输入temperature :300K, w-$iKtb. emissivity:0.1; >?)_, KL P*>?/I`G 6R8>w, 面2 : BFP@Yn~k 面型:plane 6[RTL2&W 材料:Air ]q4LNo 孔径:X=1.5, Y=6,Z=0.075,形状选择Box y1~
QKz 2M\7j *?C8,;=2r 位置坐标:绕Z轴旋转90度, #O,w{S JY"J} lKU{jWA 辅助数据: )?B-en\ $bF+J8%D 首先在第一行输入temperature :300K,emissivity: 0.1; ,'t&L] uPN^o.,/. VPuo!H Target 元件距离坐标原点-161mm; *SI,K)BP &e3}Vop Y*Ay=@z=y 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 =h=-&DSA ;"e55|d9I i$}G[v<4 探测器参数设定: hH-!3S2' QhAYCw2 在菜单栏中选择Create/Element Primitive /plane
._;It198f n ~ &ssFC d!Ws-kzE &z*4Uij `('Up? EV* |\ te 元件半径为20mm*20,mm,距离坐标原点200mm。 X}h}3+V "Wk K1u 光源创建: vO"E4s 4DP<)KX 光源类型选择为任意平面,光源半角设定为15度。 /:BC<]s j5[>HL NU{eoqaT 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。 =%>E8)Jb ?$<~cD" Sw 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 t4~?m{ `'mRGz7t \>w 2D 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 VC Ay~, qT4`3nH: 创建分析面: kDE:KV<"c 8Jp?@qt=$ z5<&}Vh;P 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。 zH~g5xgh @^-f+o )liNjY@ 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。 IsFL"Vx i1b3>H*3 FRED在探测器上穿过多个像素点迭代来创建热图 _x`:Ne? 4IM_6
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。 :,/
\E 将如下的代码放置在树形文件夹 Embedded Scripts, sv "GX<+ *l0i}"T^_ )^)|b5, 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。 o@} qPvt0 $m+Pl[s 绿色字体为说明文字, Hb^ovc0 NX]6RZr- '#Language "WWB-COM" eR3MU]zF 'script for calculating thermal image map cyL|.2, 'edited rnp 4 november 2005 `sRys oW OQyZ' 'declarations iq8Hq)I] Dim op As T_OPERATION #X5Tt ; Dim trm As T_TRIMVOLUME ,p..h+l Dim irrad(32,32) As Double 'make consistent with sampling Dl}va Dim temp As Double j{/wG:: Dim emiss As Double W%9"E??c Dim fname As String, fullfilepath As String L>57eF)7 IueI7A 'Option Explicit
)$2h:dw_ z KG]7 Sub Main KDDx[]1Q 'USER INPUTS -#AO4xpI nx = 31 kh>i#9Ie ny = 31 '1\UFz numRays = 1000 cavzXz minWave = 7 'microns a -5#8 maxWave = 11 'microns l~*d0E-$ sigma = 5.67e-14 'watts/mm^2/deg k^4 AAc2u^spx fname = "teapotimage.dat" |X~vsM0 MPsm)jqX Print "" LQ"xm Print "THERMAL IMAGE CALCULATION" %-NG eN8 $[(FCS detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 qKuHd~M{ 1 mi sPJO&QD Print "found detector array at node " & detnode 8RVeKnpXTV 93Qx+oK] srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 *eUxarI ]=]`Mnuxb Print "found differential detector area at node " & srcnode `SYq/6$VEH 0:>C v<N GetTrimVolume detnode, trm CH=k=)() ] detx = trm.xSemiApe i$'#7U dety = trm.ySemiApe DEKO]i area = 4 * detx * dety Z3A"GWY Print "detector array semiaperture dimensions are " & detx & " by " & dety 8PW3x-+ Print "sampling is " & nx & " by " & ny =,W~^<\" ]-u>HO g\ 'reset differential detector area dimensions to be consistent with sampling |\q@XCGei pixelx = 2 * detx / nx LBhDP5qF pixely = 2 * dety / ny 5cC)&}I SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 95 X6V Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 T7XbbU a[V4EX1E 'reset the source power J`A )WsKkb SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) 'Z^KpW Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" &uu69)u '\B!1B>T 'zero out irradiance array bRc~e@ For i = 0 To ny - 1 p/&s-GF For j = 0 To nx - 1 K>`*JJ, irrad(i,j) = 0.0 1|#j/ Next j ]=0$-ImQ@x Next i vtf`+q m9f[nT 'main loop |K$EULzz EnableTextPrinting( False ) ::G0v #N|A@B5x ypos = dety + pixely / 2 Gv}~ For i = 0 To ny - 1 VWE`wan< xpos = -detx - pixelx / 2 'tzN.p1O ypos = ypos - pixely aboA9pwH H-Or EnableTextPrinting( True ) ~-2q3U Py Print i ]A dL EnableTextPrinting( False ) ,[ M^rv i@spd5. wE09% For j = 0 To nx - 1 ST^{?Q ao)8ie xpos = xpos + pixelx !5h@uar `}&}2k 'shift source -#"7F:N1 LockOperationUpdates srcnode, True Z "g6z#L& GetOperation srcnode, 1, op bmGtYv op.val1 = xpos AoN|&o op.val2 = ypos 7W\aX*] SetOperation srcnode, 1, op _f~m&="T! LockOperationUpdates srcnode, False /s~&$(d59o BpZ17"\z raytrace RiM!LX DeleteRays UG<`m] CreateSource srcnode `?xE-S
;Pn TraceExisting 'draw ]k.'~Syz cu$i8$?t 'radiometry ` z!?!"= For k = 0 To GetEntityCount()-1 9q
f=P3 If IsSurface( k ) Then LuW^Ga"E temp = AuxDataGetData( k, "temperature" ) 1q;r4$n emiss = AuxDataGetData( k, "emissivity" ) B#;0{ If ( temp <> 0 And emiss <> 0 ) Then (J/!9NS: ProjSolidAngleByPi = GetSurfIncidentPower( k ) G .k\N(l frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) Z:s:NvFX irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi WL/9r
*jW End If hO}nc$S %oEvp{I End If OLM}en_L #mcU);s Next k \mp5G&+/Q 1*J#:|({(
Next j gdfG3d$4 y153ax Next i p?zh4:\F+ EnableTextPrinting( True ) !`F^LXGA ;Q} H'Wg, 'write out file
j8"2K^h= fullfilepath = CurDir() & "\" & fname j>t*k!db Open fullfilepath For Output As #1 t.E3Fh!o Print #1, "GRID " & nx & " " & ny "sU ~| Print #1, "1e+308" '=eE6=m^K Print #1, pixelx & " " & pixely =3?"s(9 Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 Um'r6ty @n:.D9 maxRow = nx - 1 ;NzS;C' maxCol = ny - 1 M~&X?/8 For rowNum = 0 To maxRow ' begin loop over rows (constant X) eEG]JH row = "" 6C|]Fm For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) *=ymK* row = row & irrad(colNum,rowNum) & " " ' append column data to row string %/x%hs;d Next colNum ' end loop over columns Bpw<{U ]/{987 Print #1, row !,3U_! !HP/`R Next rowNum ' end loop over rows {<3>^ o|" Close #1 h*GU7<F:a $"&U%3 Print "File written: " & fullfilepath dECH/vJ^ Print "All done!!" |r=.}9
- End Sub 9&`ejeD H\Jpw 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: pD>^Dfd K2GcU_*t N%.DjH 找到Tools工具,点击Open plot files in 3D chart并找到该文件 1"82JN|! [o,S.!W8 WrGz` 打开后,选择二维平面图: *t+E8)qL \!tS|h
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