-
UID:317649
-
- 注册时间2020-06-19
- 最后登录2026-02-26
- 在线时间1928小时
-
-
访问TA的空间加好友用道具
|
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。 f$'2}'.!$ P<fnLQ9 成像示意图 OnWx#84 首先我们建立十字元件命名为Target aC<KN:TN6 PoIl>c1MS 创建方法: z(\4M==2O .Udj@{ 面1 : ?i`l[+G 面型:plane _Ob@` 材料:Air &[hLzlrg 孔径:X=1.5, Y=6,Z=0.075,形状选择Box e]Zngt?b 0
&GRPu27 +,2Jzl'- 辅助数据:
&ZTr 首先在第一行输入temperature :300K,
iS?42CV emissivity:0.1; >s` J5I! cv/_r#vN q%5eVG 面2 : "l >Igm 面型:plane 2On_'^O 材料:Air G/v/+oX 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ?3O9eZY@ I7&_Xr W0=O+0$^ 位置坐标:绕Z轴旋转90度, {vo +gRYYv i>[_r,-\[ R=Tqj,6 辅助数据: j:w{;(1=W qp}Ma8+ 首先在第一行输入temperature :300K,emissivity: 0.1; 7r{83_B CB&iI' srV.)Ur Target 元件距离坐标原点-161mm; 2!Bd2 -rKO
)} )z8!f}:De= 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 Pf F=m' pMs
AyCAk $#|gLVOQ 探测器参数设定: Cg616hyut r",]Voibd 在菜单栏中选择Create/Element Primitive /plane 6DZ),F,M d(:3 -8N|xQ378 r_YIpnJ Yhp]x vzn{h)D 元件半径为20mm*20,mm,距离坐标原点200mm。 y ?G_y >q7BVF6V| 光源创建: :pRpvhm Y4IGDY* 光源类型选择为任意平面,光源半角设定为15度。 A6oq.I0 }KD;0t4 b~BIz95 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。 K 0hu:1l) AfC>Q!-w 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。 DKVT(#@T t!K*pM f+.T^es 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。 OMk5{-8B `m.eM 创建分析面: U4G}DCU 3DaQo0N N S#TW 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。 iE.-FZc na^sBq?\ {J5JYdK 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。 FecktD= 1p'Le! FRED在探测器上穿过多个像素点迭代来创建热图 a iCn"j an2AX%u 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。 Dr;iQkGP
将如下的代码放置在树形文件夹 Embedded Scripts, tvd0R$5} h O
emt 6bBdIqGb} 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。 Z X~
_g@
+%\oO/4Fs 绿色字体为说明文字, $mGvJ*9 #%@MGrsK '#Language "WWB-COM" -6sW6;Q 'script for calculating thermal image map $<p8TtI=YQ 'edited rnp 4 november 2005 0J~Qq]g :c8n[+5 'declarations
fa.0I~ Dim op As T_OPERATION 6b~28 Dim trm As T_TRIMVOLUME {0!#>["< Dim irrad(32,32) As Double 'make consistent with sampling [0[M'![8M Dim temp As Double 0iEa[G3 Dim emiss As Double r.0oxH'] Dim fname As String, fullfilepath As String 7-_vY[)/ vw<K}z 'Option Explicit 2q}.. `B8tmW# Sub Main ;3C:%!CdA] 'USER INPUTS N~ANjn/wL nx = 31 V,%L~dI ny = 31 DG;y6#|p numRays = 1000 fRTo.u minWave = 7 'microns bl/,*Wx:4. maxWave = 11 'microns /NF# +bx sigma = 5.67e-14 'watts/mm^2/deg k^4 1px\K8 fname = "teapotimage.dat" b]gY~cbI8 uHNpfKnZ Print "" jw6Tj;c Print "THERMAL IMAGE CALCULATION" (P6vOo v[<Bjs\q5 detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 0=v{RQ;W4 z 2/!m[U Print "found detector array at node " & detnode 8n4V
cu t^EhE srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 VanB>|p6 #l1Q e` Print "found differential detector area at node " & srcnode f"&Xr!b.h UBO^EVJ GetTrimVolume detnode, trm YnV/M,U detx = trm.xSemiApe 3}&ZOO dety = trm.ySemiApe &~5=K area = 4 * detx * dety >CgO<\ Print "detector array semiaperture dimensions are " & detx & " by " & dety >{Rb 3Z] Print "sampling is " & nx & " by " & ny h[XGC=% yZ}d+7T} 'reset differential detector area dimensions to be consistent with sampling <M[U#Q~?~e pixelx = 2 * detx / nx Uz8hANN0_ pixely = 2 * dety / ny Tvf~P w SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 6!EYrX}rI[ Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 FuP/tTMU1a Zzd/K^gg 'reset the source power aw}+'(?8] SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) kRIB<@{ Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" EH`0 :h";c" 'zero out irradiance array zREJ#r For i = 0 To ny - 1 9EF~l9`'U For j = 0 To nx - 1 F'J [y"~_ irrad(i,j) = 0.0 ]@xL=%
Next j :_d3//| Next i 0kCQ0xB[a5 qjC_*X! 'main loop oJaAM|7uv EnableTextPrinting( False ) p4/$EPt)lY .?#uxd~> ypos = dety + pixely / 2 J l7z|Q S For i = 0 To ny - 1 & QZV q" xpos = -detx - pixelx / 2 @eQld\h' ypos = ypos - pixely zsTbdF _GbE^ EnableTextPrinting( True ) -Fwh3F4g Print i J^H=i)A EnableTextPrinting( False ) kC^.4n
om QXk"?yT`E L]zNf71RD For j = 0 To nx - 1 oK-!(1A- 8l xY]UT xpos = xpos + pixelx sj9D -gKpL\ 'shift source B7"Fp LockOperationUpdates srcnode, True \K`jCsT GetOperation srcnode, 1, op YQ,tt<CQ op.val1 = xpos _Dq Qfc% op.val2 = ypos kr_oUXiX SetOperation srcnode, 1, op Hql5oA LockOperationUpdates srcnode, False y1(P<7:t? 8Uj: raytrace .Dv=pB,u DeleteRays {^&k!H2 CreateSource srcnode +J40wFI:y TraceExisting 'draw anx&Xj|=.F NV!4(_~ 'radiometry 9A;6x$s For k = 0 To GetEntityCount()-1 @P70W<< If IsSurface( k ) Then DPPS?~Pq temp = AuxDataGetData( k, "temperature" ) %aLCH\e emiss = AuxDataGetData( k, "emissivity" ) IvSn>o If ( temp <> 0 And emiss <> 0 ) Then G\mKCaI8 ProjSolidAngleByPi = GetSurfIncidentPower( k ) iB{xvyR frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) ^('cbl irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi )<LI%dQ:'l End If =K6c; 2}`R"MeS End If b{HhS6<K? jT"r$""1d Next k FU]4oKx BHiOQ0Fs Next j P7>IZ >bw 4I.1D2 1jA Next i $eCGez<E EnableTextPrinting( True ) Y2vj}9jK {h^c 'write out file BQU/Qo DY fullfilepath = CurDir() & "\" & fname j1F w
U Open fullfilepath For Output As #1 fIEw(k<* Print #1, "GRID " & nx & " " & ny r9;` Print #1, "1e+308" _@|fva&s,; Print #1, pixelx & " " & pixely T:n<db,Px Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 zn[QvY kC|Tubs( maxRow = nx - 1 n'3u ]~7^ maxCol = ny - 1 KZ4zF For rowNum = 0 To maxRow ' begin loop over rows (constant X) (.
H]| row = "" {tmKCG For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) =f4<({9 row = row & irrad(colNum,rowNum) & " " ' append column data to row string |<2
*v-a Next colNum ' end loop over columns |Pf(J;'[ 2|s<[V3rP- Print #1, row zze z~bv7: >@:667i,`
Next rowNum ' end loop over rows wzxdVn
'S Close #1 ?+Hp?i$1 @4@PuWI0- Print "File written: " & fullfilepath To^#
0 Print "All done!!" Y'&8L'2Z[ End Sub `;}H% :r^klJ(m 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: ?to1rFrU 5R"2Wd RCCv>o 找到Tools工具,点击Open plot files in 3D chart并找到该文件 c G*(C tU(y~)] E{I)]h 打开后,选择二维平面图: dWjx"7^ 'Y ,1OK
|