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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。 k:#!zK} sW'AjI 成像示意图 Y0dEH^I 首先我们建立十字元件命名为Target cj|80$cSA W ]?G}Q; 创建方法: g63(E,;;J J7Hl\Q[D1 面1 : @&3EJ1 面型:plane i0kak`x0 材料:Air Q}K"24`= 孔径:X=1.5, Y=6,Z=0.075,形状选择Box m{cGK`/\ CMG&7(MR H0gbSd+ 辅助数据: /1V xc 6 首先在第一行输入temperature :300K, ^]0Pfna+N emissivity:0.1; o!Ieb {14fA)`% p\tm:QWD; 面2 : *-=(Q`3 面型:plane Y^;ovH~ ve 材料:Air N06OvU2>xU 孔径:X=1.5, Y=6,Z=0.075,形状选择Box S.94edQ }mYx_=+VX F Q7T'G![ 位置坐标:绕Z轴旋转90度, t?-n*9,#S 8f)?{AX0 z2_*%S@ 辅助数据: =_ ./~ HU8900k+ 首先在第一行输入temperature :300K,emissivity: 0.1; ~Z?TFg
L:pYn_ r?lf($D* Target 元件距离坐标原点-161mm; 2~1SQ.Q<RY JPc+rfF 0y" $MC v 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 FxtQXu-g r6MMCJ|G P}y +G| 探测器参数设定: 9~5uaP$S RXpw! 在菜单栏中选择Create/Element Primitive /plane Pg0x/X{t n.`($yR_ {W=%U|f dGYn4i2k? :0j?oY~e z0p*Z& 元件半径为20mm*20,mm,距离坐标原点200mm。 8 S:w7Hr +,TRfP
Fb 光源创建: -aPg#ub |mdVdD~go 光源类型选择为任意平面,光源半角设定为15度。 h5{'Q$Erl <;eW=HT+uq ?cBwPetp 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。 hYT0l$Ng uy[At+%zg 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 0_95|3kc [fya)} 6y%qVx#! 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 (lBCO?`fx dUeN*Nq&(, 创建分析面: E"\<s3 DkY4MH? q1$N>;& 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。 ]_mb7X> N_kMK UN;H+gNnN 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。 -[4T Xy|So|/bKd FRED在探测器上穿过多个像素点迭代来创建热图 P_dCR VuhGx:Xl 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。 knu,"< 将如下的代码放置在树形文件夹 Embedded Scripts, #l\=}#\1Wb U2tV4_ e 1y4|{7bb 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。 x*/tyZg6 T6y\| 绿色字体为说明文字, !=*g@mgF o8V5w!+# '#Language "WWB-COM" 4x=v?g& 'script for calculating thermal image map a+[KI 'edited rnp 4 november 2005 tzWSA-Li AP n| \ 'declarations >Eyt17_H"n Dim op As T_OPERATION Go`vfm"S Dim trm As T_TRIMVOLUME )al]*[lY Dim irrad(32,32) As Double 'make consistent with sampling f
O}pj: Dim temp As Double =57>!) Dim emiss As Double 2@n{yYwy Dim fname As String, fullfilepath As String Dzpq_F!;V lK?uXr7^ 'Option Explicit dc+>m,3$ }/0X'o Sub Main 7X`g,b! 'USER INPUTS <prk8jSWV nx = 31 1*P~!2h ny = 31 /QK6Rac- numRays = 1000 %+aCJu[k(z minWave = 7 'microns L4@K~8j7 maxWave = 11 'microns bQzZy5, sigma = 5.67e-14 'watts/mm^2/deg k^4 L\6M^r
> fname = "teapotimage.dat" -V*R\,> x77*c._3v Print "" :(E@Gf Print "THERMAL IMAGE CALCULATION" a{ L%7 JinUV6cr detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 mxvp3t \ 8 `v-<J Print "found detector array at node " & detnode h/QXPdV 3H'sHuK"X srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 aj-Km`5r} l]
K3Y\#bP Print "found differential detector area at node " & srcnode =}<IfNA [$ubNk;!z GetTrimVolume detnode, trm #>a\>iKQ2q detx = trm.xSemiApe bt@<
ut\ dety = trm.ySemiApe ")1:F> area = 4 * detx * dety vSGH[nyCY Print "detector array semiaperture dimensions are " & detx & " by " & dety @JiLgIe` Print "sampling is " & nx & " by " & ny H9Gh>u]} PF0_8,@U 'reset differential detector area dimensions to be consistent with sampling +N]J5Ve-`t pixelx = 2 * detx / nx /m!BY}4W pixely = 2 * dety / ny .97])E[U SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False Gf%~{@7=u Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 [>vLf2OID .o6Or:L 'reset the source power V%t.l SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) 8$]1M,$r Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" h7*J9[$ ,=uD^n: 'zero out irradiance array &.F4b~A7 For i = 0 To ny - 1 i9:C4',sw0 For j = 0 To nx - 1 ;gD})@ irrad(i,j) = 0.0 K$z2YJ% Next j xEa\f[.An Next i ;'gWu \Zb;'eDv 'main loop 2/U.|*mH EnableTextPrinting( False ) ;t)3F 3h]g}&k ypos = dety + pixely / 2 k<z)WNBf For i = 0 To ny - 1 d.aS{;pse xpos = -detx - pixelx / 2 `T1 ypos = ypos - pixely V~qNyOtA] I !-
U'{ EnableTextPrinting( True ) gZVc 5u< Print i \a<wKTkn EnableTextPrinting( False ) ufj,T7g^ #j;^\rSv- UklUw For j = 0 To nx - 1 ; cNv\t D2#ZpFp"h xpos = xpos + pixelx >:SHV W &.3"Uo\# 'shift source Xa[.3=bV? LockOperationUpdates srcnode, True NCveSP GetOperation srcnode, 1, op `4r 3l S op.val1 = xpos 9p85Pv [M= op.val2 = ypos 53_Hl]#qZ SetOperation srcnode, 1, op zg>zUe
bA LockOperationUpdates srcnode, False cF*TotU_m `Uq#W+r, raytrace #{0HYg?(f DeleteRays -au^;CM CreateSource srcnode eNh39er TraceExisting 'draw bt SRtf 'I|v[G$l 'radiometry _r#Z}HK For k = 0 To GetEntityCount()-1 _!#@@O0p/h If IsSurface( k ) Then 'JtBZFq temp = AuxDataGetData( k, "temperature" ) #Bze,?@ emiss = AuxDataGetData( k, "emissivity" ) _=r6=. If ( temp <> 0 And emiss <> 0 ) Then e
v}S+!|U ProjSolidAngleByPi = GetSurfIncidentPower( k ) hXw]K" frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) SZ7:u895E irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi A.F%Ycq End If '$Dn t
mntp End If yNBQGSH rCEyQ)R_} Next k 2F;y;l% _>?\DgjH Next j _{ue8kGt Mc
lkEfn Next i (le9q5Qr. EnableTextPrinting( True ) B^=-Z8 ejKucEgD 'write out file _`$qBw.Nx fullfilepath = CurDir() & "\" & fname cdH>n) Open fullfilepath For Output As #1 Vsr.=Nd= Print #1, "GRID " & nx & " " & ny >dXGee>'M Print #1, "1e+308"
Q>qUk@ Print #1, pixelx & " " & pixely (M|Dx\_ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 d7^}tM u~N?NW Q maxRow = nx - 1 HdI8f!X'TG maxCol = ny - 1 Ep_HcX` For rowNum = 0 To maxRow ' begin loop over rows (constant X) Z{.8^u1I row = "" UBKu/@[f@ For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) @)+AaC#- row = row & irrad(colNum,rowNum) & " " ' append column data to row string W-f=]eWg Next colNum ' end loop over columns f^ZRT@`O ,]C;sN%~} Print #1, row C.:<-xo 2ACCh4(/P Next rowNum ' end loop over rows eu|YCYj)g Close #1 8$cLG*=h4 hF?1y `20 Print "File written: " & fullfilepath KM0ru Print "All done!!" j3oV+zZ49 End Sub qx(xvU9 ~Gp[_ %K 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: B4/>H| @n/\L< |