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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。 lf9mdbm PAy/"R9DT- 成像示意图 xTGdh 首先我们建立十字元件命名为Target AxAbU7m %7v!aJ40 创建方法: 2v\<MrL NY3/mS3w 面1 : VprrklZ 面型:plane n8.Tag(# 材料:Air Gl6M(<f\5 孔径:X=1.5, Y=6,Z=0.075,形状选择Box -Q MO*PY DedY(JOvB ^Z>Nbzr{ 辅助数据: <HfmNhI85( 首先在第一行输入temperature :300K, U3^3nL-M9 emissivity:0.1; }8Yu"P${Y hRI?>an laQ{nSVBm 面2 : ?'^dYQ4 面型:plane ~vscATQ 材料:Air ]j+J^g 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 2u%YRrp |@Ze{\
pmuT7*<19 位置坐标:绕Z轴旋转90度, *3A)s
O H$k2S5,,z l_i&8*=Px 辅助数据: FT
Ytf4t =5q_aK#i 首先在第一行输入temperature :300K,emissivity: 0.1; %hVI*p3 ~F.kgX .!)i Target 元件距离坐标原点-161mm; _W zrL +:/t y41~ 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 NI85|*h ,DD}o D}OhmOu3 探测器参数设定: >9Z7l63+} 2v`Q;%7O 在菜单栏中选择Create/Element Primitive /plane fn,
YH eZ|_wB'r xs^wRE_ :NynNu' ^ pNA_s!S -u^f;4|u 元件半径为20mm*20,mm,距离坐标原点200mm。 'B;n&tJ
$QnsP#ePN 光源创建: YM&i <N8z<o4rku 光源类型选择为任意平面,光源半角设定为15度。 .s%dP.P:i1 Gx;-1 srryVqgS 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 ]2rCn}; M~g{}_0Z 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 jP\5bg-} M:t"is >9,LN;Ic 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 9.wZhcqqU Vx%!j& 创建分析面: D77s3AyHK TGZr
[ ot,=.%O 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 Rnw v/) """pe+Y g(l:>=g]? 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 kC
iOcl*$ H`nd | FRED在探测器上穿过多个像素点迭代来创建热图 vT#m 8Kg / hYFOZ 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。 ->'xjD 将如下的代码放置在树形文件夹 Embedded Scripts, +wcif- {'6-;2&f +&[X7r< 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。 $pajE^d4V p7Z/%~0v: 绿色字体为说明文字, CcZM0 XnB-1{a1 '#Language "WWB-COM" g^)) 'script for calculating thermal image map SN;_.46k 'edited rnp 4 november 2005 h]WW?. :'sMrf_EA 'declarations |XJ|vQGU Dim op As T_OPERATION A\v]ZN4 Dim trm As T_TRIMVOLUME A5~OHmeK Dim irrad(32,32) As Double 'make consistent with sampling Ebp=du Dim temp As Double %UB+N8x`a Dim emiss As Double %[OZ;q& X Dim fname As String, fullfilepath As String ~:N 1[ <tv"I-2 'Option Explicit 6SEq 2 ztC>*SX Sub Main 0}q*s! 'USER INPUTS WQv`%%G2> nx = 31 O+=C8 ny = 31 R) J/z numRays = 1000 P9M. J^< minWave = 7 'microns Ph17(APt,Q maxWave = 11 'microns 9-EdT4=r, sigma = 5.67e-14 'watts/mm^2/deg k^4 |3Bmsd/3 fname = "teapotimage.dat" aK--D2@}i q{pa _ Print "" is`~C Print "THERMAL IMAGE CALCULATION" +0M0g_sk qcoTt~\ detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 ycrM8Mu
3 ?pV!`vp^{ Print "found detector array at node " & detnode _CG
ED{b@ #,;Q|)AD:e srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 qP72JxT _*n
4W^8 Print "found differential detector area at node " & srcnode (f
sfs2ki H GetTrimVolume detnode, trm |)%;B% detx = trm.xSemiApe s ?|Hw|j dety = trm.ySemiApe $j"BHpN area = 4 * detx * dety z)%]#QO Print "detector array semiaperture dimensions are " & detx & " by " & dety Ag}P Print "sampling is " & nx & " by " & ny =gHUY&sPu8 okH*2F(- 'reset differential detector area dimensions to be consistent with sampling !rff/0/x" pixelx = 2 * detx / nx N]&:xd5 pixely = 2 * dety / ny @k\npFKQm SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False {=9"WN Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 !mK}Rim~ ,YF1*69 'reset the source power GxA[N SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) hx8. Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" z,(.` %h :i*
=s}cv 'zero out irradiance array PBgU/zVn For i = 0 To ny - 1 R,m|+[sl For j = 0 To nx - 1 0+Q;a irrad(i,j) = 0.0 "8/BVW^bv Next j &S8,-~U Next i [!U!
Z'i m=V69
a# 'main loop Cps'l EnableTextPrinting( False ) Uac.8wQh t<MO~_`! ypos = dety + pixely / 2 WZcAwYB For i = 0 To ny - 1 U P*5M xpos = -detx - pixelx / 2 #^xj"}o@ ypos = ypos - pixely )jm!^m H Yw7* EnableTextPrinting( True ) EC7)M}H Print i q:9CFAX0= EnableTextPrinting( False ) *`V r P K,dEa<p E6fs& For j = 0 To nx - 1 ozW\` rbI 7
3' xpos = xpos + pixelx ~{l @ :]9CdkaU 'shift source LKYcE;n LockOperationUpdates srcnode, True S+GW}?! GetOperation srcnode, 1, op lCGEd 3 op.val1 = xpos {}"a_L&[; op.val2 = ypos DtkOb,wY SetOperation srcnode, 1, op ;Hn>Ew LockOperationUpdates srcnode, False CQH^VTQ TbgIr raytrace c=33O,_ DeleteRays t""d^a#Dp CreateSource srcnode *|6*jU TraceExisting 'draw Q$A;Fk}- I$*LMzve 'radiometry \ \g Aa-}: For k = 0 To GetEntityCount()-1 E6#")2C~ If IsSurface( k ) Then O&r9+r1` temp = AuxDataGetData( k, "temperature" ) C5~
+"#B emiss = AuxDataGetData( k, "emissivity" ) e(vnnv?R{ If ( temp <> 0 And emiss <> 0 ) Then &90pKs ProjSolidAngleByPi = GetSurfIncidentPower( k ) 5Vlm?mPU frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) fr8hT(,s) irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ! l"*DR End If "s7}eWM*a aMaqlqf End If B
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Next k p+16*f9,^ CmdPa!4) Next j JY$+<`XM j<}y( ~ Next i + {WZpP},v EnableTextPrinting( True ) c"zE 7x.]
9J 'write out file '3
JVUHn fullfilepath = CurDir() & "\" & fname @-.Tgpe@a Open fullfilepath For Output As #1 '%*/iH6<U{ Print #1, "GRID " & nx & " " & ny W/u_<\ Print #1, "1e+308" Og?P5&C"9D Print #1, pixelx & " " & pixely 6<No_x |_ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 Za7!n{?0
!qTP maxRow = nx - 1 D'Uv7Mis maxCol = ny - 1 ;upYam" For rowNum = 0 To maxRow ' begin loop over rows (constant X) qm"AatA row = "" I|_U|H!` For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) p?sFX$S row = row & irrad(colNum,rowNum) & " " ' append column data to row string 4q\gFFV4 Next colNum ' end loop over columns G@rV9 q5~"8]Dls Print #1, row :xC1Ka%~ Pl&x6\zL Next rowNum ' end loop over rows o(g}eP,g} Close #1 ogG:Ai)90 As(6E}{S Print "File written: " & fullfilepath +d=8 /3O% Print "All done!!" _A6e|(.ll End Sub XRXQ
7\n A4Tjfc,rx9 在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: pI}6AAs}Z OD).kP}s^ LNF|mS\+D 找到Tools工具,点击Open plot files in 3D chart并找到该文件 ~2O1$o u v[<;z(7Qk z W*Z 打开后,选择二维平面图: ef:YYt{|q )u.%ycfeV
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