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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。 @NHh-&;w s0kp(t!fiu 成像示意图 *6uccx7{ 首先我们建立十字元件命名为Target G=dzP}B'WA 6Rd4waj_,U 创建方法: 9
_d2u# iyskADS 面1 : EeIDlm0o 面型:plane IRdt:B|@ 材料:Air ~MpikBf 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ~5 ^Jv m s6H'}[E< 2wf&jGHs 辅助数据: 8HF^^Cva 首先在第一行输入temperature :300K, _n&Nw7d2
M emissivity:0.1; 5J5si<v25 K*6 "c.D 4<s.|W` 面2 : 9KSi-2?H 面型:plane xad`-vw 材料:Air @=J|%NO 孔径:X=1.5, Y=6,Z=0.075,形状选择Box |HazM9= @Mk`Tl ]B8
A 位置坐标:绕Z轴旋转90度, pYO =pL^Q MvVpp;bd R>'
%}|v/ 辅助数据: ]@q%dsz <@<rU:o=V 首先在第一行输入temperature :300K,emissivity: 0.1; =x~I'|%3 >rG>Bz^Pu zF&VzNR2 Target 元件距离坐标原点-161mm; 9I/b$$?D ^l &lwSRVt %pWn9 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 AerU`^ %>_[b, oy+|:[v:Fk 探测器参数设定: |dRVSVN {C1crp>q 在菜单栏中选择Create/Element Primitive /plane :qYp%Ub OLw]BJXYaE LZ*8YNp1' mh
}M|h5Im 9hp&HL)BOa Uqr>8|t? 元件半径为20mm*20,mm,距离坐标原点200mm。 =KRM`_QShg K!|eN_1A 光源创建: [K{{P|(q <}a?<):S 光源类型选择为任意平面,光源半角设定为15度。 O"m7r ds 'uPAG;)m PK*Wu<< 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*!R4yE; C J8|MK.oD 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。 _0H oJ Z~'t'.=z _k84#E0 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>5^:%3
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Q, 创建分析面: HR>Y?B{ CK* *RZ MlO OB 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。 oqrx7+0{ >KKWhJ ]8$8QQc<<5 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。 =~^b
-YoL.`s1 FRED在探测器上穿过多个像素点迭代来创建热图 kUT2/3Vi )ycI.[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。 N['DqS = 将如下的代码放置在树形文件夹 Embedded Scripts, L G}{ibB k
%I83,+ bWPsfUn# 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。 N:j7J &AiAd6 绿色字体为说明文字, 1\hLwG6Jj F>;Wbk&[| '#Language "WWB-COM" osV6= 'script for calculating thermal image map
A l[ZU 'edited rnp 4 november 2005 Z0gtliJ@ L*z=!Dpo 'declarations {kpad(E Dim op As T_OPERATION IQqUFP$8g Dim trm As T_TRIMVOLUME 5K vp% Dim irrad(32,32) As Double 'make consistent with sampling tBo\R?YRs Dim temp As Double hgU;7R,?ir Dim emiss As Double qHt/,w='Q Dim fname As String, fullfilepath As String K3&xe( l4C{LZ 'Option Explicit InP E_ h nydH-;cz Sub Main HoI6(t 'USER INPUTS :!gNOR6Lh nx = 31 /t5)& ny = 31 |Xt G9A> numRays = 1000 bWSN]]e1# minWave = 7 'microns AD?zBg Zu maxWave = 11 'microns %m&6'Rpfk sigma = 5.67e-14 'watts/mm^2/deg k^4 ~nZcA^b#DQ fname = "teapotimage.dat" c*KE3: *s6x Print "" Y6{^cZ!= Print "THERMAL IMAGE CALCULATION" <q63?Ms' 7QO/; zL detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 <G})$f'x2 Dfs^W{YA Print "found detector array at node " & detnode *85N_+Wv! fA=Z):w srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 "@ >6<(Ki (/y8KG3 Print "found differential detector area at node " & srcnode x $uhkP '-wmY?ZFxy GetTrimVolume detnode, trm ZTmy} @l detx = trm.xSemiApe Ft5A(P > dety = trm.ySemiApe v l"8Oi*r^ area = 4 * detx * dety ;|Cdq Print "detector array semiaperture dimensions are " & detx & " by " & dety '9\cIni0 Print "sampling is " & nx & " by " & ny Ny^ 1#R ^O|fw?, 'reset differential detector area dimensions to be consistent with sampling 9r%fBiSk pixelx = 2 * detx / nx OG$n C pixely = 2 * dety / ny ,Ckcc SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False o.Kn DY Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 EN m%(G$ AVT% AS 'reset the source power 2A_1 E\ SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) JFv70rBe Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ~J\qkQ
Vr2A7kq 'zero out irradiance array RELNWr For i = 0 To ny - 1 {Y~>&B5 For j = 0 To nx - 1 tN#C.M7.'7 irrad(i,j) = 0.0 r1!1u7dr
t Next j yr\ClIU Next i B=A!hXNa TdFU, 'main loop ^0]0ss;##R EnableTextPrinting( False ) #]h
X."b2 f:PlMv!{ ypos = dety + pixely / 2 5CK+\MK For i = 0 To ny - 1 BTAbDyH5 xpos = -detx - pixelx / 2 ^4=#,K ypos = ypos - pixely Q/o,2R gIo\^ktW EnableTextPrinting( True ) ni;)6,i Print i ^ITF* EnableTextPrinting( False ) +4yre^gC 1PY]Q{r 4cQP+ n For j = 0 To nx - 1 b<FE
O Z
./suR) xpos = xpos + pixelx Bx45yaT Fz#@ [1, 'shift source ,Zmjw@w LockOperationUpdates srcnode, True 8N&'n GetOperation srcnode, 1, op x2v0cR"KL op.val1 = xpos k4Q>J,k op.val2 = ypos V]|X
,G SetOperation srcnode, 1, op ,I"T9k-^ LockOperationUpdates srcnode, False *}2L4] S]3CRJU3` 'raytrace (dlp5:lQz
DeleteRays |]-Zz7N) CreateSource srcnode fd[N]I3 TraceExisting 'draw m%0-3c( }MaY:PMA 'radiometry \2@J^O1, For k = 0 To GetEntityCount()-1 o`f^ m If IsSurface( k ) Then :M(uP e=D temp = AuxDataGetData( k, "temperature" ) +b 6R emiss = AuxDataGetData( k, "emissivity" ) G&S2U=KdV% If ( temp <> 0 And emiss <> 0 ) Then Wt/;iq" ProjSolidAngleByPi = GetSurfIncidentPower( k ) Kk^*#vR frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) 44KoOY_ irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi -
lX4; End If 4Y(@
KUb 0+SDFh End If \3hA_{ w !(lcUdBd Next k SnE^\I^O SIp)& Next j .D@J\<,+l %`F;i)Zz Next i '=0}2sF> EnableTextPrinting( True ) l cl|o3yQ v+LJx 'write out file
GK/Po51 fullfilepath = CurDir() & "\" & fname H,} &=SCk Open fullfilepath For Output As #1 )-
W1Wtom Print #1, "GRID " & nx & " " & ny u"h/ERCa Print #1, "1e+308" xr'1CP Print #1, pixelx & " " & pixely MZGhN
brd Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 uHU@j(&c Ef] Hpjvp maxRow = nx - 1 X,Na4~JO( maxCol = ny - 1 e!5} #6Kd For rowNum = 0 To maxRow ' begin loop over rows (constant X) [v~,|N>w row = "" nJe}U# For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) _:Qh1 &h row = row & irrad(colNum,rowNum) & " " ' append column data to row string #,tT`{u1q Next colNum ' end loop over columns ?4':~;~ N|DfE{, Print #1, row H*0Y_H= h'"m,(a
Next rowNum ' end loop over rows x*Z'i<;B Close #1 C@XS s#Dj>Fej Print "File written: " & fullfilepath Om*QN]lGq Print "All done!!" wsmgkg End Sub os5$( *$=i1w 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: T >8P1p@A, f30J8n"k !Ubm 586! 找到Tools工具,点击Open plot files in 3D chart并找到该文件 D1rVgM -+ByK#<% ~YH?wdT 打开后,选择二维平面图: AA5G`LiT e)uC
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