| 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。 (!zM\sF :EHQ .^
成像示意图 oh\,OW 首先我们建立十字元件命名为Target 1kFjas`g X ,
ZeD 创建方法: vjK, I9 it}-^3AM 面1 : =7jEz+w# 面型:plane #ooc)), 材料:Air F$Pp]"82'm 孔径:X=1.5, Y=6,Z=0.075,形状选择Box kV)'a :m`/Q_y"
4;<DJ.XlN= 辅助数据: rihlae5Kz 首先在第一行输入temperature :300K, olty4kGD$V emissivity:0.1; @-6?i) ,IjdO(?TC v]bAWo 面2 : FMS2.E 面型:plane *T4ge|zUc 材料:Air h~ha 孔径:X=1.5, Y=6,Z=0.075,形状选择Box <-)9>c:k q|{tQJfYg Fk$@Yy+}e 位置坐标:绕Z轴旋转90度, ,L%p 60PYCqWc
E~He~wHWe 辅助数据: M {x ie t<lyg0f 首先在第一行输入temperature :300K,emissivity: 0.1; ,OB&nN t> >eo8 L?f qcW{ Target 元件距离坐标原点-161mm; 3wNN<R qJMp1DC
@3 "DBJ 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 @,vv\M0)p )6G+ tU' =eYO;l
y3 探测器参数设定: >4'21,q n\~yX<;X3 在菜单栏中选择Create/Element Primitive /plane I"V3+2e )dg UmN
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lt%-m@#/ w:R]!e_6\9 SRk7gfP*q 元件半径为20mm*20,mm,距离坐标原点200mm。 AzX(~Qc 6SAQDE 光源创建: Na;t#, =+Tsknq 光源类型选择为任意平面,光源半角设定为15度。 :eLLDp< %0(>!SY !L$oAqW 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。 Bcm=G"" +2(PcJR~ 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。 |
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b ke</x+\F 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。 4+,*sn ndt8=6p
创建分析面: /
GZV_H%v c$.T<r)Z Nuo<` 6mV@ 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 C9+Dw#-fV ~l4Q~'
<v-92? 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 A'(k
Yc X)FQ%(H< FRED在探测器上穿过多个像素点迭代来创建热图 LQ|<3] .Px,=56$X 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。 Jz2q\42q 将如下的代码放置在树形文件夹 Embedded Scripts, $q=hcu |W/Hi^YE2
XAGiu;<,= 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 <#!8?o&i akY6D]M 绿色字体为说明文字, gGD]t;<u D`5:
JR-{ '#Language "WWB-COM" +0)5H>h 'script for calculating thermal image map UvoG<; 'edited rnp 4 november 2005 _2x uzmz0 7{8)ykBU^ 'declarations 4O9tx_<JG Dim op As T_OPERATION RH1U_gp4 ] Dim trm As T_TRIMVOLUME @V*au: Dim irrad(32,32) As Double 'make consistent with sampling sV;qpDXX Dim temp As Double !vi4*
@: Dim emiss As Double &s_}u%iC Dim fname As String, fullfilepath As String ~n)]dFy !WDn7j'A 'Option Explicit VdYOm +._f.BRmX. Sub Main J78Qj[v 'USER INPUTS S:DcfR=a nx = 31 :1%VZvWk* ny = 31 UeC 81*XZ numRays = 1000 !k ;[^> minWave = 7 'microns C5d/)aC maxWave = 11 'microns XWJ0=t&} sigma = 5.67e-14 'watts/mm^2/deg k^4 4{uJ||! fname = "teapotimage.dat" G;Pt|F?c vQE` c@^{ Print "" h/w] Print "THERMAL IMAGE CALCULATION" WIhIEU7 / #zh6=.,7 detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 1/F<T MX%|hIOpr Print "found detector array at node " & detnode 9iiU,}M`j ~r7DEy|+ srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 1j_aH#Fz: m3 x!*9h Print "found differential detector area at node " & srcnode |8b$x| B /6?tgr GetTrimVolume detnode, trm 1ZGQhjcx detx = trm.xSemiApe $,!dan<eA dety = trm.ySemiApe !^rITiy area = 4 * detx * dety ZC>`ca Print "detector array semiaperture dimensions are " & detx & " by " & dety .oW~:mY Print "sampling is " & nx & " by " & ny ~M|NzK_9 zSX' 'reset differential detector area dimensions to be consistent with sampling i|::vl pixelx = 2 * detx / nx Uj
y6vgU; pixely = 2 * dety / ny +^o3}` SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False [0(
E>vm Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 UeIqAG 8 C{U[w^X 'reset the source power x|P<F 2L SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) T=iZ9w Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" hvwnG>m\ W,L>'$#pM 'zero out irradiance array 1`7]C+Pv For i = 0 To ny - 1 e\+~ For j = 0 To nx - 1 |>m# m*{S irrad(i,j) = 0.0 BHiw!S< Next j 6jQ&dN{=qB Next i AOq9v~)z- N
P0Hgd 'main loop ;RTrRh0v EnableTextPrinting( False ) Z:r$;`K/ pEqr0Qwh ypos = dety + pixely / 2 [7ek;d;'t For i = 0 To ny - 1 ^+Y-=2u: xpos = -detx - pixelx / 2 rA>A=, ypos = ypos - pixely 96([V|5K 9, sCJ5bb" EnableTextPrinting( True ) _tWfb}6;Zb Print i 2*3B~" EnableTextPrinting( False ) hc31+TL LmT[N@>" ._F6- pl For j = 0 To nx - 1 9cx!N,R t ,sQ0atk7ma xpos = xpos + pixelx V"D<)VVA AU${0#WV_ 'shift source N";dG 3 LockOperationUpdates srcnode, True 6#lC(ko' GetOperation srcnode, 1, op i32_ZB Z?y op.val1 = xpos Ot8S'cB1,$ op.val2 = ypos d
>wmg*J SetOperation srcnode, 1, op +X|m>9 LockOperationUpdates srcnode, False
EY[Q% xs83S.fHg raytrace 3R$CxRc: DeleteRays AD4L`0D CreateSource srcnode Jr*S2z<* TraceExisting 'draw O'yjB$j W;)FNP|MT 'radiometry Rs(CrB/M For k = 0 To GetEntityCount()-1 <PuB3PEvV If IsSurface( k ) Then spoWdRM2 temp = AuxDataGetData( k, "temperature" ) 9OO_Hp#|9 emiss = AuxDataGetData( k, "emissivity" ) &j~|3 If ( temp <> 0 And emiss <> 0 ) Then c#4L*$ViF ProjSolidAngleByPi = GetSurfIncidentPower( k ) +e3WwUx frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) P.H/H04+ irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ~IJZM`gN End If K
{1ZaEH &4Iqm( End If lN`_0 nluyEK Next k q MT.7n: [E
:`jY Next j K1wN9D{t' FsPDWy&x Next i {ALBmSapK" EnableTextPrinting( True ) ;h(;( -L4G WJ~.- 'write out file UC
LjR<} fullfilepath = CurDir() & "\" & fname UEYM;$_@4o Open fullfilepath For Output As #1 E{]|jPdr Print #1, "GRID " & nx & " " & ny X!A]V:8dk Print #1, "1e+308" cPBy(5^ Print #1, pixelx & " " & pixely `J7Lecgo Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 7[.Q.3FL E<G@LT maxRow = nx - 1 5\kZgXWIh maxCol = ny - 1 AL$Ty For rowNum = 0 To maxRow ' begin loop over rows (constant X) w5/X{ row = "" kpreTeA] For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) {s^ryv_} row = row & irrad(colNum,rowNum) & " " ' append column data to row string $^D(% Next colNum ' end loop over columns HtXBaIl\ byj mH Print #1, row VOK$;s'9} mW(_FS2%, Next rowNum ' end loop over rows 'UG}E@G Close #1 WQmiG=Dw^ ~Z/ `W` Print "File written: " & fullfilepath A=[f>8 Print "All done!!" ^?.:} End Sub Jz3<yQ-
T]Td4T! 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: 5!Mp#lO y#Sw>-zRq LW
3J$Am 找到Tools工具,点击Open plot files in 3D chart并找到该文件 2yO)}g FJ |b@A:8ss h+u|MdOY\ 打开后,选择二维平面图: V5@[7ncVf E9*?G4P{l
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