-
UID:317649
-
- 注册时间2020-06-19
- 最后登录2025-12-11
- 在线时间1894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。 Y,"MQFr(o hCoLj6Vx 成像示意图 1KR|i" 首先我们建立十字元件命名为Target /'_ RI RL)3k8pk 创建方法: ASU\O3%% y$No o)Z 面1 : I*R$*/) 面型:plane -Dm.z16 材料:Air ? UDvFQ& 孔径:X=1.5, Y=6,Z=0.075,形状选择Box */e5lRO\ y5D?Bg|M 0qUap*fvC 辅助数据: ABDUp: 首先在第一行输入temperature :300K, )t=u(:u] emissivity:0.1; =eLb"7C#0 Y-{BY5E. L2$L.@ 面2 : A:J{ 面型:plane Y--8v#t 材料:Air bD-Em#> 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ?0%TE\I8 6+z]MT itgO#(g$Q 位置坐标:绕Z轴旋转90度, >D#}B1(! E-iBA (H 1*CWHs 辅助数据: 6x{IY a$O]'}]` 首先在第一行输入temperature :300K,emissivity: 0.1; wKbymmG (32nI?)a 3:#rFb Target 元件距离坐标原点-161mm; .)zISa*Xy !c($ C Q0_W<+` 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 Cw5K* EQ$9IaY. VrxH6 Y 探测器参数设定: 0Wm-`ZA elB 8 在菜单栏中选择Create/Element Primitive /plane WfNMyI 74(J7 VAt9JE;# y*(j{0yd eR`<9KBH L|w-s4L 元件半径为20mm*20,mm,距离坐标原点200mm。 .Tv(1HAc2l
e5]AB 光源创建: 4]
1a^@? elgQcJ99 光源类型选择为任意平面,光源半角设定为15度。 oy: MM Yk?q7xuT w\*/(E<:
我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 E%B Gf}h %T\x~) 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 eMzCAO N@)~j+Pz o hlVc%a 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 R?s\0 >t(@?*ZFT 创建分析面: ~\,6C1M 1}*; |9eY
R 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 ^ni_%`Ag xltu
g## eUlb6{!y? 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 Jx w<* eS:e#>( FRED在探测器上穿过多个像素点迭代来创建热图 n`xh/vGm# G1tp FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 ~#\#!H7 将如下的代码放置在树形文件夹 Embedded Scripts, p ]=;t" GR
`ncI$z 4&fnu/,Z 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。 GYxI$y0: F9w&!yW: 绿色字体为说明文字, W^Y0>W~ uD5yw#` '#Language "WWB-COM" 926oM77 'script for calculating thermal image map =U2n"du 'edited rnp 4 november 2005 yTiqG5r yfQE8v+ 'declarations k1zt| Dim op As T_OPERATION 2"mj=}y6 Dim trm As T_TRIMVOLUME rK|&u
v*b Dim irrad(32,32) As Double 'make consistent with sampling ulJYJ+CC! Dim temp As Double ZQA
C&: Dim emiss As Double ]i2\2MTW8 Dim fname As String, fullfilepath As String
5AU3s n4y6Ua9m{ 'Option Explicit wkA!Jv% B)8Hj).@B Sub Main K9'*q3z 'USER INPUTS I3Xh[% -! nx = 31 "\?G ny = 31 |LH*)GrD*t numRays = 1000 Ct+% minWave = 7 'microns Qe.kNdT+_ maxWave = 11 'microns IQ~7vk() sigma = 5.67e-14 'watts/mm^2/deg k^4 ',Pk>f]AB- fname = "teapotimage.dat" VTfaZ/e. 4[ 0?F!% Print "" g>P9hIl Print "THERMAL IMAGE CALCULATION" 6qpV53H F*:NKT d detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 T?{9Z o{W]mr3D Print "found detector array at node " & detnode ABmDSV5i \RyA}P5S srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 b)^ZiRW`` Nj&%xe>]. Print "found differential detector area at node " & srcnode ld:alEo ?u!AHSr( GetTrimVolume detnode, trm X>8?p'* detx = trm.xSemiApe G>>u#>0 dety = trm.ySemiApe V_622~Tc/[ area = 4 * detx * dety w1(06A}/ Print "detector array semiaperture dimensions are " & detx & " by " & dety }h h^U^ia Print "sampling is " & nx & " by " & ny _rd j,F8 }(EOQ2TI 'reset differential detector area dimensions to be consistent with sampling dU^<7 K:S pixelx = 2 * detx / nx Ab<Ok\e5 pixely = 2 * dety / ny Jd"s~n<>K SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False q'@Ei4 Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 JM lhBh :";D.{|| 'reset the source power E wsq0D SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) >=:T
ZU Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" %kFELtx 7qK0!fk5 'zero out irradiance array 9|A-oS For i = 0 To ny - 1 f<altz_\q For j = 0 To nx - 1 <;E[)tv irrad(i,j) = 0.0 RXS| -_$ Next j U]U)' Next i w[oQ}5?9' 5=h'!|iY 'main loop *u;">H*BW EnableTextPrinting( False ) ]O=S2Q =C>`}%XT} ypos = dety + pixely / 2 EZumJ." For i = 0 To ny - 1 1(7.V-(G xpos = -detx - pixelx / 2 wW! r}I# ypos = ypos - pixely &W<>^C2v j*~dFGl) EnableTextPrinting( True ) 6aZt4Lw2\ Print i n!eqzr{ EnableTextPrinting( False ) <*Kh=v 'BdmFKy1 eGe[sv"k For j = 0 To nx - 1
QXxLe* Q] yT xpos = xpos + pixelx OG^WZ.YU Q}?N4kg 'shift source %*6oUb LockOperationUpdates srcnode, True LLn{2,jfQ GetOperation srcnode, 1, op H@2"ove-uC op.val1 = xpos Ma=6kX] op.val2 = ypos tGO[A#9a SetOperation srcnode, 1, op Ie&b<k LockOperationUpdates srcnode, False feI[M;7u +>WC^s raytrace JQ/t, v$G DeleteRays KjwY'aYwr: CreateSource srcnode
&QOWW} TraceExisting 'draw <.=#EV^i j
#I:6yA3 'radiometry ?%xhe For k = 0 To GetEntityCount()-1 NBqV0>vR If IsSurface( k ) Then H
MjeGO.i temp = AuxDataGetData( k, "temperature" ) ,8=`* emiss = AuxDataGetData( k, "emissivity" ) Q),3&4pM If ( temp <> 0 And emiss <> 0 ) Then lKV\1(` ProjSolidAngleByPi = GetSurfIncidentPower( k ) i+X2M-[Ls frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) 5h|m4)$ irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi !&a;P,_Fb End If \n*7#aX/ /y9J)lx End If I)XOAf$6 EAD0<I<>
Next k % L ># Od!F: < Next j 9o`7Kc/g s!hI:$J. Next i ]/o12pI EnableTextPrinting( True ) x!C8?K=| T}t E/ 'write out file =CKuiO.j fullfilepath = CurDir() & "\" & fname '6o`^u> Open fullfilepath For Output As #1 1qLl^DW Print #1, "GRID " & nx & " " & ny i+)}aA Print #1, "1e+308" [*9YIjn Print #1, pixelx & " " & pixely !]rETP_ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 :>P4L,Da] UR1JbyT maxRow = nx - 1 S$jV|xKB maxCol = ny - 1 r:c@17 For rowNum = 0 To maxRow ' begin loop over rows (constant X) *^@#X-NG row = "" 2JiAd*WK For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) <'}b*wUB row = row & irrad(colNum,rowNum) & " " ' append column data to row string n^iNo Next colNum ' end loop over columns :Su #xI <?LfOSdMs^ Print #1, row *2,e=tY> #+K
Kvk Next rowNum ' end loop over rows &2io^AP Close #1 pHen>BA[ ([,vX"4 Print "File written: " & fullfilepath OU,PO2xX9 Print "All done!!" Pt6hGSo. End Sub _{LN{iqDv G$;]
?g 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: L$+d.=] }W:*aU jl.okWuiY 找到Tools工具,点击Open plot files in 3D chart并找到该文件 {W5ydHXy I 1 b 1B)Y;hg6& 打开后,选择二维平面图: H96BqNoO q&XCX$N
|