-
UID:317649
-
- 注册时间2020-06-19
- 最后登录2025-04-02
- 在线时间1761小时
-
-
访问TA的空间加好友用道具
|
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。 qHAZ)Tz t[L_n m5- 成像示意图 QA=G+1x 首先我们建立十字元件命名为Target U\crp
T` @Lp;p$G` 创建方法: AK7IPftlH Sqc
r
- 面1 : x]1G u 面型:plane hkK+BmMj\ 材料:Air ?u*gKI 孔径:X=1.5, Y=6,Z=0.075,形状选择Box D8w:c6b & o2F4 F5*NK!U 辅助数据: b1("(,r/` 首先在第一行输入temperature :300K, y([""z3<w emissivity:0.1; {*X8!P7C u:6PAVW? QG|KZ8uO 面2 : 13:yaRo 面型:plane )ZyEn% 材料:Air h{$mL#J 孔径:X=1.5, Y=6,Z=0.075,形状选择Box NI@$" +c8cyx:^f "agc*o~!F 位置坐标:绕Z轴旋转90度,
R%(ww n@hf{hA[a sSh=Idrx 辅助数据: S%+$ 01/? 首先在第一行输入temperature :300K,emissivity: 0.1; %XpYiW#AK /~4wM#Yi8 r_5k$u( Target 元件距离坐标原点-161mm; -w0U}Te^ qrWeV8ur+ TAkM-iyH] 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 QGWfF,q S$=e %c &TpzJcd" 探测器参数设定: h-^7cHI} B\/"$" 在菜单栏中选择Create/Element Primitive /plane d%"?^e 8-A *Jc ndsu}:my rvdhfM!-A S.!0~KR:U .^?^QH3 元件半径为20mm*20,mm,距离坐标原点200mm。 cH5@Jam $'9b,- e 光源创建: nA!Xb'y& WWO@ULGY 光源类型选择为任意平面,光源半角设定为15度。 ][ ,NNXrc& Gk.;<d v4:g*MD?~ 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 q ;@:,^ A?
=(q 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 nvJ2V$ qep<7 QO [jOvy>2K] 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。 5]Wkk~a !kPZuU`T 创建分析面: ?pT\Ft V $WOiXLyCk xaiA? 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 U 0$?:C+? J!%cHqR m[@7!.0=
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。 `7;I*| `OY_v=} FRED在探测器上穿过多个像素点迭代来创建热图 B{D!5{t F-=W7 D:[c 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。 _]W
}6?i 将如下的代码放置在树形文件夹 Embedded Scripts, B!Ss
35< c'9-SY1'~ -H@Gyw
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。 7qyv.{+ Qi_De
'@ 绿色字体为说明文字, b,?@_*qv+ zLG5m]G4D '#Language "WWB-COM" )xJo/{? 'script for calculating thermal image map .K`^n\T
t 'edited rnp 4 november 2005 k)2L<Lmn 94=aVM\>> 'declarations J,8Wo6 Dim op As T_OPERATION 67uUeCW Dim trm As T_TRIMVOLUME Unl6?_ Dim irrad(32,32) As Double 'make consistent with sampling u1?1x Dim temp As Double %hYol89F Dim emiss As Double TP6iSF Dim fname As String, fullfilepath As String 9s5PJj "u VfJbexYT 'Option Explicit hM!D6: t EDm,Y Sub Main sK#)wjj\^ 'USER INPUTS P=)&]Pz nx = 31 D4:c)} ny = 31 2?]NQE9lA numRays = 1000 @wWro?s'p minWave = 7 'microns -{
Ng6ntS maxWave = 11 'microns _T\~AwVc< sigma = 5.67e-14 'watts/mm^2/deg k^4 *k$ ":A fname = "teapotimage.dat" &Rgy/1 DA[s k7 Print "" =] R_6# Print "THERMAL IMAGE CALCULATION" a95QDz UB3b detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 t3TnqA r?e)2l~C8j Print "found detector array at node " & detnode E%CJM+r! $-dz1} srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 q4XS
E, _,hhO Print "found differential detector area at node " & srcnode Z4\$h1tl c}nXMA^^ GetTrimVolume detnode, trm d7xd" detx = trm.xSemiApe 83*"58 dety = trm.ySemiApe M(,npW area = 4 * detx * dety J$)lYSNE Print "detector array semiaperture dimensions are " & detx & " by " & dety aqTMOWyeu Print "sampling is " & nx & " by " & ny I'URPj:t 7o$4ov;T 'reset differential detector area dimensions to be consistent with sampling ,UFr??ZKm
pixelx = 2 * detx / nx pN+lC[C pixely = 2 * dety / ny @_&@M~ u SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False %N!2 _uk5 Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 D`=hP(y^ Ybr&z7# 2 'reset the source power ,!"\L~6 SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ;c5Q" Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" Z3K~C_0Cnu e[t+pnRh 'zero out irradiance array b469 For i = 0 To ny - 1 lNSB "S For j = 0 To nx - 1 hJ0)"OA5 irrad(i,j) = 0.0 U?u0|Y+ Next j \lVX~r4 Next i M[ea!an Ju$vuEO 'main loop g;U f? EnableTextPrinting( False ) {`0GAW)q pq`Bg`c ypos = dety + pixely / 2 f`X#1w9 For i = 0 To ny - 1 Ak!l}d xpos = -detx - pixelx / 2 Z:|2PQ4 ypos = ypos - pixely 7d0E9t;W Z6<vLc EnableTextPrinting( True ) f
Q.ea#xh^ Print i ]k[y#oB EnableTextPrinting( False ) Aj06"ep s9 '*Vm RHo|&.B;+ For j = 0 To nx - 1 9,|&+G$ y%CaaK=V3 xpos = xpos + pixelx oI9Jp` Ws[[Me,= 'shift source NJb5HoYZ LockOperationUpdates srcnode, True fL7ym,? GetOperation srcnode, 1, op irNGURLm op.val1 = xpos DiF=<} >x op.val2 = ypos 'vO+,- SetOperation srcnode, 1, op %=J<WA6\ LockOperationUpdates srcnode, False %Uk]e5Hu XJ;kyEx3=O raytrace Pm]6E[zC DeleteRays `,
?T;JRc CreateSource srcnode p1p4t40<l TraceExisting 'draw I(r ^q" K ;2tY+I 'radiometry O$B]#]L+ For k = 0 To GetEntityCount()-1 rvRtR/*?j If IsSurface( k ) Then 9V&%_.Z temp = AuxDataGetData( k, "temperature" ) JcxhI]E emiss = AuxDataGetData( k, "emissivity" ) ,[IN9W If ( temp <> 0 And emiss <> 0 ) Then 5fS89?/? ProjSolidAngleByPi = GetSurfIncidentPower( k ) p8F5b8]* frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) yKEE @@}\ irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi `Nnqdc2 End If =:(8F*Q ,D-VC{lj End If @RKw1$BA m?hC!n> Next k .Ev i Qz;2RELz Next j 95giqQ(N RRy3N
)HR Next i DJlY~}v#_ EnableTextPrinting( True ) @W|}|V5 ;pdW7 'write out file +<Ot@ luE fullfilepath = CurDir() & "\" & fname `P9vZR; Open fullfilepath For Output As #1 s% `o Print #1, "GRID " & nx & " " & ny A(#hyb# Print #1, "1e+308" eHG**@"X Print #1, pixelx & " " & pixely NS"hdyA Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 :NHh`@0F +ib72j%A maxRow = nx - 1 d|5u<f5 maxCol = ny - 1 |r5|IA For rowNum = 0 To maxRow ' begin loop over rows (constant X)
]SpUD row = "" uj_uj! For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) pdsjX)O+f row = row & irrad(colNum,rowNum) & " " ' append column data to row string ,WbO8#z+ Next colNum ' end loop over columns @#ih;F rWF~aec Print #1, row ^<xpp.eY 0o[p<<c* Next rowNum ' end loop over rows X""<5s'0 Close #1 >:5/V0;, _I+#K M Print "File written: " & fullfilepath ;ej;<7+ Print "All done!!" nn$,|/ End Sub ;7&RmIXKh' v]gJ 7x 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: 3+"z 5#+!|S[PK j&)+qTV 找到Tools工具,点击Open plot files in 3D chart并找到该文件 "y/GK1C a9}cpfG=) (Ac
'}O 打开后,选择二维平面图: X:+;d8rCy cEO g
|