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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。 V'^E'[Dd{ ,_M 成像示意图 w!|jL
$5L 首先我们建立十字元件命名为Target Y/<`C *Roqie 创建方法: 90Bn}@t=Q `e[>S 面1 : ;k:17&:8ue 面型:plane #V$h?`qhwr 材料:Air q@&6&cd 孔径:X=1.5, Y=6,Z=0.075,形状选择Box Dq[Z0"8 ^61;0 ?1.WF}X' 辅助数据: q}|_]R_y 首先在第一行输入temperature :300K, s H(io emissivity:0.1; n@$("p b*)F7{/Z t2LX@Q" 面2 : -P:o ^_)g 面型:plane XGb*LY+Db6 材料:Air 4DgH/Yo 孔径:X=1.5, Y=6,Z=0.075,形状选择Box {\vcwMUzZ D k<NlH zp "lRxatM 位置坐标:绕Z轴旋转90度, uk9!rE" nrV!<nNBk #h}a 辅助数据: H7
"r^s]D n{I1ZlEeh 首先在第一行输入temperature :300K,emissivity: 0.1; 1t/mq?z: `-w, 6 Mx Dqp; Target 元件距离坐标原点-161mm; L/?jtF:o {X10, jG`,k*eUrJ 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 a0&L,7mu<' $ftxid8 4Opf[3] 探测器参数设定: ]E$bK *?pnTQs^ 在菜单栏中选择Create/Element Primitive /plane cD t|v~ 9]vy#a# g(C/J9J ?c<uN~fC= xW|8-q &$heW, 元件半径为20mm*20,mm,距离坐标原点200mm。 Qp9QSyMs} BtrMv6 光源创建: <+UJgB
A- uD\rmO{ 光源类型选择为任意平面,光源半角设定为15度。 =I0J1Ob K'f^=bcI 3BSZz%va 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 i9Eh1A3Y hkOFPt& 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 D63?f\ pJJOy 4Uhh]/ 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 C;?<WtH +4+czfz 创建分析面: 7LB%7~{< 7 lSR m.FN ttkM 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 N;a' `l @&x'.2[nv nRyx2\Py+ 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 @~}~;}0x >abpse FRED在探测器上穿过多个像素点迭代来创建热图 .X5A7 m LLL;SNY FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 D&x.io 将如下的代码放置在树形文件夹 Embedded Scripts, M8IU[Pz4 a ?\:,5= 6~l+wu<$ 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。 TR%8O; ,/qY 9eh 绿色字体为说明文字, )NK#}c~5 oIniy{ '#Language "WWB-COM" $pIo`F _W 'script for calculating thermal image map DyCkz"1S 'edited rnp 4 november 2005 [_`@V4 *zMt/d*<& 'declarations ] &SmeTe Dim op As T_OPERATION Tz~a. h@ Dim trm As T_TRIMVOLUME Q!r&vQ/g Dim irrad(32,32) As Double 'make consistent with sampling 2St<m-& Dim temp As Double F2{SC?U Dim emiss As Double '#>Fe`[ Dim fname As String, fullfilepath As String 9Wg;M#c2Y| $1FnjL5u 'Option Explicit [dXa, bM2x
(E\O Sub Main v4K! BW 'USER INPUTS }=B~n0 nx = 31 * \B(- ny = 31 '-mzt~zGOY numRays = 1000 S..8,5mBH minWave = 7 'microns e}n(mq maxWave = 11 'microns h(^c5#. sigma = 5.67e-14 'watts/mm^2/deg k^4 Xpv<v[a fname = "teapotimage.dat" ^Nu j/ qL
<@PC.5 Print "" #*%?]B= Print "THERMAL IMAGE CALCULATION" 0+[3>N y0 ?a*w6,y. detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 {c~w
Ms# ?]aVRmL Print "found detector array at node " & detnode \T!,Z;zK `[e0_g\ srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 O.Y|},F !E|R3eX_ Print "found differential detector area at node " & srcnode l5]R*mR WYP\J1sy GetTrimVolume detnode, trm #s' `bF^ detx = trm.xSemiApe x iz+R9p dety = trm.ySemiApe ?NvE9+n area = 4 * detx * dety !1K.HdK Print "detector array semiaperture dimensions are " & detx & " by " & dety Y;iI=U Print "sampling is " & nx & " by " & ny O S#RCN* LK!sk5/ 'reset differential detector area dimensions to be consistent with sampling |`pBI0Sjo pixelx = 2 * detx / nx K:% MhH- pixely = 2 * dety / ny 9I`0`o"A SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False mY[*Cj3WJ Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 bSn={O"M %_!0V*X* 'reset the source power Ujqnl>l SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) gI9nxy Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ?* r SL`; `// 'zero out irradiance array deq5u> For i = 0 To ny - 1 a8v\H8@X For j = 0 To nx - 1 }2\Hg irrad(i,j) = 0.0 LpI4R Next j [ w-Tf& Next i T!Tp:&O- >;F}>_i 'main loop vbX.0f "n EnableTextPrinting( False ) 4F6I7lu TXT<6( ypos = dety + pixely / 2 i3KAJ@ For i = 0 To ny - 1 _/"e'@z xpos = -detx - pixelx / 2 t:P7ah ypos = ypos - pixely I+ 3qu= q2OF-.rE EnableTextPrinting( True ) <%W&xk Print i SUIu.4Mz EnableTextPrinting( False ) GT80k]e. MRZN4<}9 wDSwcNS For j = 0 To nx - 1 U3-MvI,Q ?R4u>AHS@ xpos = xpos + pixelx YXmy-o> $ %|b6Gr/& 'shift source '66nqJb* LockOperationUpdates srcnode, True t/%[U,m GetOperation srcnode, 1, op U%Hcck' op.val1 = xpos XbeT x op.val2 = ypos @MoCEtt SetOperation srcnode, 1, op &j/,8 Z* LockOperationUpdates srcnode, False *b!.9p K Sn
7h$ raytrace 44w
"U%+ DeleteRays @3 + CreateSource srcnode aqI m W TraceExisting 'draw <lU(9)
L;& {zc*yV\ 'radiometry x9t% For k = 0 To GetEntityCount()-1 S$P=;#r If IsSurface( k ) Then O<mA+yk temp = AuxDataGetData( k, "temperature" ) qlg.\H:W~ emiss = AuxDataGetData( k, "emissivity" ) jeO`45O If ( temp <> 0 And emiss <> 0 ) Then O*N:.|dUw ProjSolidAngleByPi = GetSurfIncidentPower( k ) EM1HwapD frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) w@YPG{"j irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi foY]RkW9 End If YACx9K H FPZ@6 End If V$iA3)7W% gx eu2HG Next k D vN0h(? Yt_t> Next j .b!HEi<F _5b~3K/V Next i 7fd,I% v EnableTextPrinting( True ) hYA1N&yz@ cg_tJ^vrY 'write out file !c0x^,iE fullfilepath = CurDir() & "\" & fname \<y|[ Open fullfilepath For Output As #1 P]2 /}\f Print #1, "GRID " & nx & " " & ny Cv&>:k0V Print #1, "1e+308" `r}a:w- Print #1, pixelx & " " & pixely .vIRz-S Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 &N3a`Ua $RHw6*COG maxRow = nx - 1 Z^J)]UL/ maxCol = ny - 1 (Hmh b}H For rowNum = 0 To maxRow ' begin loop over rows (constant X) vDR>
Q&/K row = "" W>,D$ For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) JE@3 UXg row = row & irrad(colNum,rowNum) & " " ' append column data to row string j xq89x Next colNum ' end loop over columns !wKNYe OMab! Print #1, row V=PK)FJ JuRWR0@` Next rowNum ' end loop over rows dDA&\BuS Close #1 %RzkP}1>E Ly1t'{"7 Print "File written: " & fullfilepath 5l(@p7_+ Print "All done!!" |="Y3}a End Sub })q8{Qj! NID2$ p 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: 5twG2p8 `Cy;/95m |h((SreO 找到Tools工具,点击Open plot files in 3D chart并找到该文件 >=1UhHFNI ZLf(m35 \!0~$?_)P 打开后,选择二维平面图: n2["Ln mO &##JZ
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