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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。 |qmu_x\ 8_tK4PwP 成像示意图 HP3lz,d 首先我们建立十字元件命名为Target ,~OwLWi-|X Ko&>C_N 创建方法: o\3L}Y MgNU`` 面1 : }`,t$NV` 面型:plane j&Wl0 材料:Air +i2}/s@JJ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box #[`:'e JaL%qco .sj^{kGE 辅助数据: ?)1{)Erf8x 首先在第一行输入temperature :300K, 3YFU*f, emissivity:0.1; < !dqTJos
By9*1H2R ^WNrGF 面2 : <c,u3cp 面型:plane A3S<..g2 材料:Air 52,m:EhL 孔径:X=1.5, Y=6,Z=0.075,形状选择Box )8UWhl= fIwV\,s Hqn#yInA7~ 位置坐标:绕Z轴旋转90度, /gu%:vq }=8B* 66I"=: 辅助数据: Ts ^"xlK n_(/JE> 首先在第一行输入temperature :300K,emissivity: 0.1; ;F~LqC$ cvfr)K[0 d~`x )B( Target 元件距离坐标原点-161mm; mA*AeP_$ 'Ub
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2 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 HOE_S!N !H irhDN 3MY(<TGX 探测器参数设定: NCk r /#! F>-B3x 在菜单栏中选择Create/Element Primitive /plane DJ(q
7W :h&fbBH I9mvte P3nb2. [-;_ZFS{ "gne_Ye. 元件半径为20mm*20,mm,距离坐标原点200mm。 IS#FiH '
)?f{ 光源创建: &xY^OCt D[mSmpjE6& 光源类型选择为任意平面,光源半角设定为15度。 weE/TW\e wm$}Pch =|%Cu& 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。 $ n+w$CI) 5c^Z/
Jl$c 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。 !\"5rNy bVL9vNK CFqJ/'' 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。 k?z98 >4 K!'AkTW+- 创建分析面: x7<\]94 rZfN+S,g OV%Q3$15 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 kWe{r5C7 &*7?)eI!i MwR0@S}* 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 0LfU=X0#7 jGEt+\"/QJ FRED在探测器上穿过多个像素点迭代来创建热图 a e*Mf7 \yd
s5g!: FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 f"9q^ 将如下的代码放置在树形文件夹 Embedded Scripts, \z$p%4`E@ ;IVDr: <0QH<4 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。 1e>s{ NDs!a 绿色字体为说明文字, sp5eVAd HVP"A3}KC '#Language "WWB-COM" &%s8L\? 'script for calculating thermal image map HE'2"t[a 'edited rnp 4 november 2005 -Y*bSP)\ Gu'rUo3Do 'declarations 9$Xu,y Dim op As T_OPERATION cu% C" Dim trm As T_TRIMVOLUME o4%y>d) Dim irrad(32,32) As Double 'make consistent with sampling GHsilba Dim temp As Double t: IN,Kl4 Dim emiss As Double
l"!Ko G7 Dim fname As String, fullfilepath As String )@L'wW <IC~GqXv 'Option Explicit A%^w^f 59!Fkd3 Sub Main :k3Nt5t! 'USER INPUTS aAA9$ nx = 31 ]]&M@FM2z ny = 31 W3;#fa:[L numRays = 1000 ^~$)F_`" minWave = 7 'microns *=wYuJ# maxWave = 11 'microns 9(L)&S{4K sigma = 5.67e-14 'watts/mm^2/deg k^4 x,otFp fname = "teapotimage.dat" qR8u$2}NY .>mr%#p Print "" :LQ5u[g$\ Print "THERMAL IMAGE CALCULATION" .'rW.'Ft dpFVN[\oK detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 }Y*VAnY6; i-'9AYyw Print "found detector array at node " & detnode #~=hn8 ph_4q@ srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 #fL8Kq .p=sBLp8 Print "found differential detector area at node " & srcnode +8#_59;x h^*4}GU GetTrimVolume detnode, trm }4{fQ`HT detx = trm.xSemiApe S_T1y dety = trm.ySemiApe 1|?05<8 area = 4 * detx * dety x&`~R>5/ Print "detector array semiaperture dimensions are " & detx & " by " & dety w,Lvt
} Print "sampling is " & nx & " by " & ny T`9u!#mT= z)xSN;x 'reset differential detector area dimensions to be consistent with sampling ? B E6 pixelx = 2 * detx / nx "F}'~HWZp pixely = 2 * dety / ny :gB[O>'<m SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False <N`J`J-[ Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 PI~1GyJr@; 0V{(Ru.O 'reset the source power 2<][%> ' SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) vNeCpf Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" =1u@7Bh cwuO[^S} 'zero out irradiance array a3VM' For i = 0 To ny - 1 3VUWX5K? For j = 0 To nx - 1 !bD@aVf?5 irrad(i,j) = 0.0 d @*GUmJ Next j 5|I[>Su Next i v|ck>_"
. Wfz\`y 'main loop 7]BW[~77 EnableTextPrinting( False ) {\z({Wlb] V=X:= ypos = dety + pixely / 2 TP}h~8 /; For i = 0 To ny - 1 8:o<ry xpos = -detx - pixelx / 2 ~-#yOu
,w ypos = ypos - pixely A+&xMM2Wj WH$e2[+Y EnableTextPrinting( True ) 6AP~]e 8 Print i 8`]=C~G EnableTextPrinting( False ) [<,~3oRu `?y<>m* ^@"H1 For j = 0 To nx - 1 Pe_!?:vF 5I,gBT|B xpos = xpos + pixelx c.|l-zAeX _oB_YL;,* 'shift source DS2)@ LockOperationUpdates srcnode, True pCu!l#J GetOperation srcnode, 1, op $x#FgD(iI op.val1 = xpos m$LVCB op.val2 = ypos KT.?Xp:z SetOperation srcnode, 1, op NJ MJ LockOperationUpdates srcnode, False @O}7XRJ_8 ;oNhEB:F raytrace 8*SP~q DeleteRays <N(oDa U CreateSource srcnode EQe5JFR TraceExisting 'draw m))<!3 vNW jH!' 'radiometry |3{&@7 For k = 0 To GetEntityCount()-1 fRvAKz|rL If IsSurface( k ) Then *<'M!iRC temp = AuxDataGetData( k, "temperature" ) QJW`}`R emiss = AuxDataGetData( k, "emissivity" ) $ C0TD7= If ( temp <> 0 And emiss <> 0 ) Then 7$k8%lI;> ProjSolidAngleByPi = GetSurfIncidentPower( k ) Y=*P
8pg frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) f&x0@Q/eON irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi o:Zd1"Z End If hKlZi!4J WV"jH9"[ End If )B!d,HKt; +<.\5+ Next k }sxn72, CodSJ, Next j + q''y +jqj6O@Tjr Next i S :8OQI EnableTextPrinting( True ) 6S.~s6o, ~/IexQB& 'write out file &*&?0ov^" fullfilepath = CurDir() & "\" & fname "Jy~PcJZ1 Open fullfilepath For Output As #1 [<wbbvXR Print #1, "GRID " & nx & " " & ny =C
f(B<u Print #1, "1e+308" O {k:yVb Print #1, pixelx & " " & pixely eX2<}'W< Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 pGIe=Um0W ArI]`h'W maxRow = nx - 1 !RlC~^
- maxCol = ny - 1 uO >x:*^8 For rowNum = 0 To maxRow ' begin loop over rows (constant X) @("}]/O
V: row = "" On1v<SD$[ For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) 0m+8P$)C% row = row & irrad(colNum,rowNum) & " " ' append column data to row string `BnP[jF Next colNum ' end loop over columns cX
A t:m GIv){[i Print #1, row z]Acs &!y]:CC{ Next rowNum ' end loop over rows ^ft]b2i Close #1 Jbp5'e
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bK% Print "File written: " & fullfilepath {5Eyr$ Print "All done!!" j5%qv(w End Sub nDlO5 pe"d 3AlqBXE"Z< 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: :w?7j_p# ~2/{3m{3 A qi+&|80T. 找到Tools工具,点击Open plot files in 3D chart并找到该文件 GJ}.\EaAJ HPa|uDVv 9b6!CNe! 打开后,选择二维平面图: [BBpQN.^q6 dALK0U
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