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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。 U,+kV?Z aIZ@5w"7 成像示意图 M>0=A 首先我们建立十字元件命名为Target U\
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ia 创建方法: Bl% {C 首先在第一行输入temperature :300K,emissivity: 0.1; 6k42>e*p =5%jKHo+9z #'^p-Jdm Target 元件距离坐标原点-161mm; xp1
+C{ ,<|EoravH 27E6S)zv 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 bI@+Or I4
Tc&b TpZ) wC 探测器参数设定: BYVp~!u 7-w
+/fv 在菜单栏中选择Create/Element Primitive /plane }o=R7n% zScV 9,H1 &.=d,XKN 9
o-T#~i _xAdvr' W fbwo2qe@K 元件半径为20mm*20,mm,距离坐标原点200mm。 phl5E:fIKx `\q4z-<- 光源创建: [G[HQ)A {;Mcor3 光源类型选择为任意平面,光源半角设定为15度。 +tdt>)a idPkJf/ cpFw]w%] 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。 %9-).k -G;4['p 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。 {^"c>'R -YA1Uk @a>+r1 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。 *u
3K8"XZ ilayU 创建分析面: > g8;x# u~1[nH: }/(fe`7: 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。 kd|@. q'3= m{_\@'q 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。 x~j% "]kaaF$U% FRED在探测器上穿过多个像素点迭代来创建热图 26o68U8&y S=krF yFw 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。 BA A)IQF 将如下的代码放置在树形文件夹 Embedded Scripts,
@5acTYQ DD"]as"# /ta-jOcRH& 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。 hP`3Ao Z)62/`C) 绿色字体为说明文字, -g;iMqh# w;}P<K '#Language "WWB-COM" :~zK0v" 'script for calculating thermal image map ,U],Wu) 'edited rnp 4 november 2005 3UslVj1u u{ JAC! 'declarations {/XzIOO;b Dim op As T_OPERATION D7[ 8*^ Dim trm As T_TRIMVOLUME iZgv
VH Dim irrad(32,32) As Double 'make consistent with sampling ysGK5kFz Dim temp As Double KNQX\-= Dim emiss As Double P9G c)$6{p Dim fname As String, fullfilepath As String d01bt$8> _9Iz'-LgB 'Option Explicit EXS
1.3> BtVuI5*h Sub Main IObGmc 'USER INPUTS zK k;&y|{ nx = 31 db@i*Bf ny = 31 (/v(.t numRays = 1000 Cb x/ minWave = 7 'microns u~bk~3.I maxWave = 11 'microns F.c,F R2 sigma = 5.67e-14 'watts/mm^2/deg k^4 Zh{Pzyp fname = "teapotimage.dat" 9p+DAs{i nP0|nPWz# Print "" &h`s:Y Print "THERMAL IMAGE CALCULATION" c,!Ijn\;( l<(MC R* detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 Fv.}w_ ht!o_0{~ Print "found detector array at node " & detnode Wf-i)oc4I / /3iai srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 7xO
=:* ;R@zf1UYA Print "found differential detector area at node " & srcnode -3_-n*k! (Z,v)TOXjV GetTrimVolume detnode, trm |XtN\9V. detx = trm.xSemiApe *_!nil 3(i dety = trm.ySemiApe $!G7u<`na area = 4 * detx * dety 8jMw7ti Print "detector array semiaperture dimensions are " & detx & " by " & dety -ce N}Cb3 Print "sampling is " & nx & " by " & ny 1}Tbp_ UP58Cln* 'reset differential detector area dimensions to be consistent with sampling =;l.<{<VH pixelx = 2 * detx / nx E2Q;1Re@ pixely = 2 * dety / ny K#%L6=t$< SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False =$X5O&E3' Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 p3&/F=T;) V\W?@V9g- 'reset the source power g1@zk$ SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) dPc*!xrq Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" f<=<:+ s+#gH@c 'zero out irradiance array Xx~OZ^t&Vn For i = 0 To ny - 1 n!2"pRIi For j = 0 To nx - 1 yS[:C
2v irrad(i,j) = 0.0 4c_TrNwP Next j g
j8rrd| Next i W-qec IlVz 5#R 'main loop !trt]?*- EnableTextPrinting( False ) E2 Q[ q6bi{L@/R ypos = dety + pixely / 2 ,|D_? D)U For i = 0 To ny - 1 umaF}}-Q{ xpos = -detx - pixelx / 2 Nj$3Ig"l ypos = ypos - pixely jVC`38| |]1-ck! EnableTextPrinting( True ) I<`K;El' Print i %PRG;kR EnableTextPrinting( False ) P"Lk(gY #` Q3Z}C J3fk3d`2 For j = 0 To nx - 1 t~H'Ugv^ ##+|zka!U xpos = xpos + pixelx X; I:i%- b#`XmB 'shift source ]VtVw^ ir LockOperationUpdates srcnode, True 0{^@kxV GetOperation srcnode, 1, op DDxbIkt op.val1 = xpos #?\$*@O op.val2 = ypos VT8PV5z SetOperation srcnode, 1, op /j/,@,lw7z LockOperationUpdates srcnode, False Veo*-sl ZUePHI-dP raytrace
J@sH(S DeleteRays a\;1%2a CreateSource srcnode s~
||Vv! TraceExisting 'draw FJXYKpY[r rH*1bDL 'radiometry F*m^AFjs For k = 0 To GetEntityCount()-1 $mdmuUIy-3 If IsSurface( k ) Then 3<}\{ jT temp = AuxDataGetData( k, "temperature" ) O<7Q>m emiss = AuxDataGetData( k, "emissivity" ) !~Vo'ykwx' If ( temp <> 0 And emiss <> 0 ) Then wNo2$>* ProjSolidAngleByPi = GetSurfIncidentPower( k ) <Hd8Jd4f frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) }<R,)ZV^G irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi H'KCIqo
End If j5Kw0Wy7 `EKmp|B_p_ End If )4:K@ KYE)#<V}@ Next k ,;;7+|` s B!#`kh Next j <Qg).n>;z ]Z\Z_t Next i # &zM.O1Q EnableTextPrinting( True ) 3y^PKIIrt W*J_PL9j 'write out file mm}y/dO~} fullfilepath = CurDir() & "\" & fname L\0;)eJ#M Open fullfilepath For Output As #1 zs/4tNXw Print #1, "GRID " & nx & " " & ny -55[3=# Print #1, "1e+308" UWU(6J|Fk Print #1, pixelx & " " & pixely eTg8I/)%B Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 di.yh3N$ a8 X}r. maxRow = nx - 1 o;'E("!<Z maxCol = ny - 1 +kA>^ For rowNum = 0 To maxRow ' begin loop over rows (constant X) /{1s U}k- row = "" ga?:k,xv For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) Ov$>CA row = row & irrad(colNum,rowNum) & " " ' append column data to row string hcn$uyP Next colNum ' end loop over columns uqz HS>GM #jrtsv] Print #1, row SEf RU` G5WQTMzf& Next rowNum ' end loop over rows V52>K$j Close #1 r ^=rs!f@ Sg%h}]~ Print "File written: " & fullfilepath l7h6R$7; 0 Print "All done!!" rX7GVg@H End Sub *y+N-uq TxJoN]Z. 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: oW}nr<G{< vHJOpQmt~ _+!@c6k)ra 找到Tools工具,点击Open plot files in 3D chart并找到该文件 ./]xn is~"yE7 [T
|P|\M 打开后,选择二维平面图: mpr_AL!ZO~ 4nsc`Hu
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