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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。 J%n#uUs Nu3gkIz5z- 成像示意图 m(o`; 首先我们建立十字元件命名为Target -%|
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d ; Bex;!1 创建方法: J5n6K$.d Hpa6;eT 面1 : <$K=3&:s8q 面型:plane )B+R|PZ, 材料:Air m.!LL]] 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 5D2mZ/ Vr Lp5?Bh j Neb*dPoK 辅助数据: hW'b'x< 首先在第一行输入temperature :300K, -#mN/ emissivity:0.1; O2?yI8|Jn 63J3NwFt m mZP; 面2 : mj'N)6ga 面型:plane v#d(Kj 材料:Air )+|wrK:*v 孔径:X=1.5, Y=6,Z=0.075,形状选择Box otfmM]f F(zCvT pUS: HJk| 位置坐标:绕Z轴旋转90度, xQU//kNL >2 #<tH0 I'^XEl? 辅助数据: 4n@>gW yz!L:1DG 首先在第一行输入temperature :300K,emissivity: 0.1; EpKZ.lCU $y,KDR7^ Fx}v.A5 Target 元件距离坐标原点-161mm; TB?'<hD: X lItg\R AZE%fOG<i 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 H\n6t-l vea{o35! *3E3,c8{A 探测器参数设定: jA;b2A]G 8+dsTX`|S 在菜单栏中选择Create/Element Primitive /plane 8{!|` b'f fa,:d8 a%BC{XX w'A *EWO <}A6 )=T 2;*G!rE&*` 元件半径为20mm*20,mm,距离坐标原点200mm。 re/u3\S A'7Y{oPHX 光源创建: p>\[[Md <*z'sUh+} 光源类型选择为任意平面,光源半角设定为15度。 QxaMe8( v;G/8>GRy 88X]Uw(+ 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。 4[gbRn' #o[n. 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。 UJDI[`2 `>g\gaQ Q?LzL(OioN 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。 U&:-Vf~& COm^ti-p 创建分析面: ^Ss<< j DEym&- #K@!jh)y^ 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。 I4w``""c lul ^`dMjeF 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。 42hG}Gt S1)g\Lv FRED在探测器上穿过多个像素点迭代来创建热图 p=eSJ* RrrlfF ms 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。 SeS ZMv 将如下的代码放置在树形文件夹 Embedded Scripts, |}e"6e% ,wg (}y' >7X5/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。 %La/E# Gdx%#@/ 绿色字体为说明文字, jqj}j2
9 c[X6!_ '#Language "WWB-COM" []N&,2O 'script for calculating thermal image map Sh-B! 'edited rnp 4 november 2005 k5bv57@ E=S_1 'declarations XPq`;<G Dim op As T_OPERATION \8a014 Dim trm As T_TRIMVOLUME ? N]bFW"t| Dim irrad(32,32) As Double 'make consistent with sampling -:L7iOzgD Dim temp As Double !IC
.0I` Dim emiss As Double -gC%*S5& Dim fname As String, fullfilepath As String v6aMYmenBH 'cQ`jWZQ 'Option Explicit x~8R.Sg ujX\^c Sub Main +JD^5J,-NJ 'USER INPUTS ~
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M3(^ nx = 31 <b\.d^=B ny = 31 h<?I?ZR0$ numRays = 1000 cw~GH minWave = 7 'microns wT;;B=u}G maxWave = 11 'microns F3Da-6T@ sigma = 5.67e-14 'watts/mm^2/deg k^4 "Ya;&F.' fname = "teapotimage.dat" AlrUfSBB s%>u[-9U Print "" n
Zx^ej\ Print "THERMAL IMAGE CALCULATION" Ud>hDOJ3 j`3IizN2 detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 I|>IV ?&1%&?cg9 Print "found detector array at node " & detnode aG@GJ@w l`0JL7 srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 >2mY% (lit^v,9 Print "found differential detector area at node " & srcnode EmP2r*"rb X88I|Z'HIh GetTrimVolume detnode, trm Ai)Q(] detx = trm.xSemiApe +{)V%"{u: dety = trm.ySemiApe Wk-.dJ area = 4 * detx * dety p<@+0Uw2 Print "detector array semiaperture dimensions are " & detx & " by " & dety \vj xCkg{ Print "sampling is " & nx & " by " & ny !a'{gw g8"{smP/ 'reset differential detector area dimensions to be consistent with sampling =*y{y)B^g pixelx = 2 * detx / nx f'S 0" pixely = 2 * dety / ny NH1|_2 SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 4HXNu, T' Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 4=* ml}RP Hpp;dG 'reset the source power %-!:$ 1; SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) | 8n,|%e Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" J/ vcP jz&= 8 'zero out irradiance array 63i&e/pv For i = 0 To ny - 1 u`*$EP-% For j = 0 To nx - 1 )[t3-' irrad(i,j) = 0.0 wLQM]$O Next j +w@/$datI Next i O}lqY?0* DB] ]6 'main loop VN@ZYSs EnableTextPrinting( False ) n6IN I~, :Sk<0VVd7 ypos = dety + pixely / 2 % o0.8qVJi For i = 0 To ny - 1 3e^'mT xpos = -detx - pixelx / 2 mO\=#Q> ypos = ypos - pixely 1g|6,J ;wr]_@<~ EnableTextPrinting( True ) )#cGePA Print i 'DH_ihZ EnableTextPrinting( False ) !un_JZD w{ x=e $4TawFf"nc For j = 0 To nx - 1 UDa\* TUO#6 xpos = xpos + pixelx !r0 z3^*N cFG%Ew@ 'shift source opxPK=kJ LockOperationUpdates srcnode, True VoUAFEcs GetOperation srcnode, 1, op `qbsDfq@ op.val1 = xpos MXpj_+@ op.val2 = ypos s|8_R; SetOperation srcnode, 1, op &$NVEmW-J LockOperationUpdates srcnode, False 9hs7B!3pc> 7Rom#Kl: raytrace ~E7=c3:" DeleteRays `\S~;O CreateSource srcnode F(:]lM| TraceExisting 'draw wsfn>w?!V o"A%dC_ 'radiometry ,b8B)VZ? For k = 0 To GetEntityCount()-1 '^M3g-C[Jg If IsSurface( k ) Then $;+`sVG temp = AuxDataGetData( k, "temperature" ) -zLxT emiss = AuxDataGetData( k, "emissivity" ) o#&;,9 If ( temp <> 0 And emiss <> 0 ) Then utwqP~ ProjSolidAngleByPi = GetSurfIncidentPower( k ) )c<5:c frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) ma26|N5 irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ~x}=lK N End If LaiUf_W #X s"]LQM1| End If uBC*7Mkm X<"W@ Next k g8w5X!Z
?en%m|}0 Next j >U$,/_uMNW :ITz\m Next i m)?cXM EnableTextPrinting( True ) /ZKO\q "ealYveu 'write out file i'9 fullfilepath = CurDir() & "\" & fname ]"M 4fA Open fullfilepath For Output As #1 H\<C@OkJS} Print #1, "GRID " & nx & " " & ny %@jv\J
Print #1, "1e+308" } Pc6_# Print #1, pixelx & " " & pixely sL tsvH# Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 t1
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cx maxRow = nx - 1 yeNC-U< maxCol = ny - 1 }3!.e For rowNum = 0 To maxRow ' begin loop over rows (constant X) b9([)8 row = "" 4o2C=?@( For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) ?<slB>8 row = row & irrad(colNum,rowNum) & " " ' append column data to row string Re
b^w, Next colNum ' end loop over columns rT
~qoA\ ,*V{gpC7 Print #1, row %-:6#bz _dq.hW7 Next rowNum ' end loop over rows !W8'apG&[ Close #1 kqA`d Os1(28rl Print "File written: " & fullfilepath _A\c 6# Print "All done!!" 7@Qz End Sub Y0U<l1(| R28h%KN 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: Rj%q)aw' W%.Kr-[?`o '
7>V4\" 找到Tools工具,点击Open plot files in 3D chart并找到该文件 7@rrAs-"Z C;;dCsiV5 avk0pY(n 打开后,选择二维平面图: $3%EKi 69,;=
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