| infotek |
2022-01-24 09:30 |
十字元件热成像分析
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。 DQXcf*R L)F4)VL
成像示意图 Udn Rsp9S 首先我们建立十字元件命名为Target QQV8Vlv" ivq(eKy 创建方法: ku]?"{Xx `\\s%}vZ*T 面1 : \6?a 面型:plane '#LzQ6Pn 材料:Air ZBY2,%nAo 孔径:X=1.5, Y=6,Z=0.075,形状选择Box '&Y_,-i K@cWg C
7/QK"0 辅助数据: OM\1TD/- 首先在第一行输入temperature :300K, {CBb^BP emissivity:0.1; LOfw
#+]d P3|s}& _]4p51r0 面2 : kln)7SzPuk 面型:plane a oU" 材料:Air <YU4RZ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box gz[3 xH~ 0D@ $ fDqT7}L 位置坐标:绕Z轴旋转90度, A7+ZY, *w*>\ZhOm
JOt(r}gU 辅助数据: 6V JudNA
w 0= 首先在第一行输入temperature :300K,emissivity: 0.1; ycc G>%>r LAf#Rco4 !^su=c Target 元件距离坐标原点-161mm; msfE; &*+$38XE^
~:T@SrVI 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 o&%v"#H2 %ZWt 45A =NC??e { 探测器参数设定: !.mR]El{K h`1<+1J9 在菜单栏中选择Create/Element Primitive /plane MAFdJ+n# +c<iVc|
]&Y^ F.$z7ee@ .aY$-Y< TQ4L~8 元件半径为20mm*20,mm,距离坐标原点200mm。 a!: N
C /^nIOAeE 光源创建: JJ?rVq1g H@xS<=:lM 光源类型选择为任意平面,光源半角设定为15度。 Sf*v#? r@zT!.sc! .UL2(0 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。 P%e7c, '_.qhsS 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。 V2T%tn;rp e
c]kt' g_syGQ\ 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。 B1nm?E 0i %w65)BFQ 创建分析面: j%nN*ms ZJBb%d1; [h;I)ug[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。 VrZfjpV $Xlr@)%
!9/`PcNIpy 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 ~bb6NP;'L :\"0jQ.y| FRED在探测器上穿过多个像素点迭代来创建热图 -GPBX? vNs%e/~vj FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 _<.VP 将如下的代码放置在树形文件夹 Embedded Scripts, IXa~,a H71 )>FAtE
p)/e;q^ 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 gE\ ^ vaB
VR>!Ch 绿色字体为说明文字, Ie^Ed` 'M"z3j]m-, '#Language "WWB-COM" IVSC7SBiT 'script for calculating thermal image map apa&'%7 'edited rnp 4 november 2005 9#:nlu9 M+
%O-B 'declarations 3O$l;|SX Dim op As T_OPERATION tz;o6,eb Dim trm As T_TRIMVOLUME u5}:[4N%I Dim irrad(32,32) As Double 'make consistent with sampling # `E Dim temp As Double 9S]pC?N]E Dim emiss As Double |cY HH$ Dim fname As String, fullfilepath As String Ln,<|,fZN # atq7tX 'Option Explicit ESV./~K G^)]FwTs Sub Main `S|F\mI~
'USER INPUTS 4%r?(C0x nx = 31 ,g7O ny = 31 3pWav
1" numRays = 1000 )?[7}(4jI minWave = 7 'microns YM_ [ maxWave = 11 'microns cwzkA,e@ sigma = 5.67e-14 'watts/mm^2/deg k^4 ?`?Tg&W fname = "teapotimage.dat" ]gPx%c Hu<]*(lK% Print "" -"nkC Print "THERMAL IMAGE CALCULATION" n zaDO-2! Gxe)5,G detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 G^d3$7 [IOI&`?D Print "found detector array at node " & detnode o4FHR+u<M p+=zl`\=| srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 tjtvO@?1- R5=J :o Print "found differential detector area at node " & srcnode S&UP;oc ; j.d GetTrimVolume detnode, trm 8wkhbD|; detx = trm.xSemiApe xFp$JN dety = trm.ySemiApe k)>H=?mI area = 4 * detx * dety ~>>_`;B Print "detector array semiaperture dimensions are " & detx & " by " & dety _@B? Print "sampling is " & nx & " by " & ny %W D^0U| $5 G(_ 'reset differential detector area dimensions to be consistent with sampling 2Ty]s~ pixelx = 2 * detx / nx Wd;t(5Xl pixely = 2 * dety / ny 1<m`38' SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False s&nat4{B Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 Gf.ywqE$Y$ ZskX!{ 'reset the source power V6dq8Z"h SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) xwD` R* Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" #>aq'47j u
$-&Im< 'zero out irradiance array Fya*[)HBo For i = 0 To ny - 1 ZOPK For j = 0 To nx - 1 n[DRX5OxR' irrad(i,j) = 0.0 _$$.5?4 Next j xT&~{,9 Next i yrEh5v: P,] ./m\J 'main loop k
?KJ8 EnableTextPrinting( False ) 5OWyxO3{ V $I8iVGL ypos = dety + pixely / 2 e]1'D For i = 0 To ny - 1 5;KJ0N*- xpos = -detx - pixelx / 2 &mtt,]6C_ ypos = ypos - pixely ShC$ue?Q P0>2}/;o EnableTextPrinting( True ) /Yi4j,8!| Print i ep"{{S5g EnableTextPrinting( False ) T=YVG@fm? 7Q|<6210 ^dLu#,; For j = 0 To nx - 1 ,(q]
$eOZ fWJpy#/^*K xpos = xpos + pixelx b|.Cqsb
8?LT*>! 'shift source O#;sY`fy_M LockOperationUpdates srcnode, True U:8]G GetOperation srcnode, 1, op f$^wu~ op.val1 = xpos A"pQOtrm\k op.val2 = ypos Z4Q]By:/L SetOperation srcnode, 1, op 1A'eH:$ LockOperationUpdates srcnode, False DcBAncsK sm'_0EUg raytrace #%QHb,lhl DeleteRays %`k [xz CreateSource srcnode N4,oO H~ TraceExisting 'draw nxhlTf>3 jC[_uG 'radiometry 0fX` >-X For k = 0 To GetEntityCount()-1 {E%c%zzQ If IsSurface( k ) Then J/P[9m30[ temp = AuxDataGetData( k, "temperature" ) eZa7brC| emiss = AuxDataGetData( k, "emissivity" ) C~4SPCU If ( temp <> 0 And emiss <> 0 ) Then |oU I2<" ProjSolidAngleByPi = GetSurfIncidentPower( k ) 36{OE!,i frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) T1$p%yQH irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi rM.Pc?Z End If nZnqXclzxn .?s jr4 End If
3}s]F/e G@Z%[YNw Next k )B
$Q wi+Qlf Next j Pl/Xh03E ByP<-Deh Next i Mm*V;ADF EnableTextPrinting( True ) U -OD y'`7zJ 'write out file D"aK;_W@h fullfilepath = CurDir() & "\" & fname <QvVPE}z Open fullfilepath For Output As #1 $"NH{%95} Print #1, "GRID " & nx & " " & ny
)nf%S+KV Print #1, "1e+308" Mj1f;$ Print #1, pixelx & " " & pixely D$4GNeB+# Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 4vi?9MPz v`QDms,{ maxRow = nx - 1 ^@8XJ[C,_ maxCol = ny - 1 *cM=>3ws/ For rowNum = 0 To maxRow ' begin loop over rows (constant X) hd'fWFWN row = "" B|a <=~ For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) D+;4|7s+ row = row & irrad(colNum,rowNum) & " " ' append column data to row string \?t8[N\_[( Next colNum ' end loop over columns ?bM%#x{e ?jfh'mCA Print #1, row ,nL~?h-Zh ;"IWm<]h;- Next rowNum ' end loop over rows 8tSY|ME Close #1 ij:a+T ;taZixOH Print "File written: " & fullfilepath Z<>gx m< Print "All done!!" Y>aVnixx< End Sub 1Q
FsT *:d``L 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: BMO,eQcB &Qda| C ibfuR 找到Tools工具,点击Open plot files in 3D chart并找到该文件 \?v&JmEU >WZ%Pv* A@|Z^T: 打开后,选择二维平面图: P=EZ6<c3& Ht+ro Y
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