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Implementation of the ESVM The output quality of the xerographic image is determined by the functionality of each subsystem. Monitoring the voltage on the photoconductor right after the charging station will help to characterize the photoconductor’s dark decay property as well as charge uniformity as the exposure input noise source. It can also be helpful in terms of creating a voltage vs. exposure level plot when the measurement is taken after exposure. Trek 344, the Electro-Static Voltage Meter (ESVM) as shown in Figure 1 is the measuring device. Its probe works like a capacitor that charges itself up to the same level as the object being measured. Therefore it allows potential on the photoconductor plate to be determined without physical contact. The probe (Figure 2) has to be placed 2mm from the surface of the photoconductor. It cannot be held by hand since it will charge itself up with respect to the object being measured; therefore, the probe needs to be positioned by a fixture. The solution is to use the old camera holder along with a probe mount (Figure 3) as the fixture since it can be easily adjusted and repositioned while staying at the same distance from the photoconductor. Readings of the charge will be taken immediately after charging and exposure station by two separate ESVMs. Figure 2 also shows the two locations for the probe placement. The material used for the probe mount is aluminum, ASTM 6061. Figure 1: the ESVM Figure 2: placement of the ESVM probes Figure 3: ESVM probe mount ESVM ADC The ESVM has a DC output that is 1/100 of what it is reading from the probe. This signal cannot be read directly by the DAQ since it only recognizes digital inputs. Therefore, an analog to digital converter (ADC) has to be designed in order for the DAQ to read the output of the ESVM. The simplest solution found was to use a voltage to frequency converting chip (LM331) as shown in Figure 4. This solution has not yet been implemented, however, preliminary tests have been conducted and output frequency does increase linearly with the input voltage. Figure 4: LM331 chip The operation of the LM331 chips is best understood by going through the operating cycle of the basic V-to-F converter, Figure 5, which consists of the simplified block diagram of the LM331 and the various resistors and capacitors connected to it. The voltage comparator compares a positive input voltage, V1, at pin 7 to the voltage, Vx, at pin 6. If V1 is greater, the comparator will trigger the 1-shot timer. The output of the timer will turn ON both the frequency output transistor and the switched current source for a period t=1.1 RtCt. During this period, the current i will flow out of the switched current source and provide a fixed amount of charge, Q = i x t, into the capacitor, CL. This will normally charge Vx up to a higher level than V1. At the end of the timing period, the current i will turn OFF, and the timer will reset itself. Now there is no current flowing from pin 1, and the capacitor CL will be gradually discharged by RL until Vx falls to the level of V1. Then the comparator will trigger the timer and start another cycle. The current flowing into CL is exactly IAVE = i x (1.1xRtCt) x f, and the current flowing out of CL is exactly Vx/RL . VIN/RL. If VIN is doubled, the frequency will double to maintain this balance. Even a simple V-to-F converter can provide a frequency precisely proportional to its input voltage over a wide range of frequencies. Figure 5: LM331 basic operation cycle The simple stand-alone V-to-F converter shown in Figure 6 includes all the basic circuitry of Figure 5 plus a few components for improved performance. A resistor, RIN=100 kΩ±10%, has been added in the path to pin 7, so that the bias current at pin 7 (−80 nA typical) will cancel the effect of the bias current at pin 6 and help provide minimum frequency offset. The resistance RS at pin 2 is made up of a 12 kΩfixed resistor plus a 5 kΩ(cermet, preferably) gain adjust rheostat. The function of this adjustment is to trim out the gain tolerance of the LM331, and the tolerance of Rt, RL and Ct. For best results, all the components should be stable low temperature-coefficient components, such as metalfilm resistors. The capacitor should have low dielectric absorption; depending on the temperature characteristics desired, NPO ceramic, polystyrene, Teflon or polypropylene are best suited. A capacitor CIN is added from pin 7 to ground to act as a filter for VIN. A value of 0.01 μF to 0.1 μF will be adequate in most cases; however, in cases where better filtering is required, a 1 μF capacitor can be used. When the RC time constants are matched at pin 6 and pin 7, a voltage step at VIN will cause a step change in fOUT. If CIN is much less than CL, a step at VIN may cause fOUT to stop momentarily. A 50Ωresistor, in series with the 1 μF CL, provides hysteresis, which helps the input comparator provide the excellent linearity. The output frequency followed this formula: 𝑓𝑜𝑢𝑡 = 𝑉𝑖𝑛 𝑅𝑆 1 2.09𝑉 𝑅𝐿 𝑅𝑡 𝐶𝑡 U1 R5 Rin 7 100k 5 2 Vin 3V Cin 0.1u 6 8 C2 1u Rs 12k RL 100k Rt Vs IN FRQOUT R/C REF IOUT 3 1 10k THRS VS Vlogic 5V LM331 15V 5.6k R4 50 Ct .01u 0 Figure 6: voltage to frequency converter schematic using LM331 Additional information on LM331 can be found on the following website http://www.national.com/ds/LM/LM231.pdf Charging Station Characterization The voltage experienced by the PC differs as the supplied voltages for the Gird and Corona change. An experiment was done to characterize the voltage viewed by the PC as a function of the supplied Grid and Corona Voltage. This was accomplished by placing the ESVM probe as shown in Figure 7. While changing the supplied voltages, the ESVM reading was hand copied. A 3D plot of the data is available in Figure 8. Figure 7: probe setting for charging station voltage measurement Voltage Experienced by PC vs. Corona and Grid Voltage Voltage Experienced by PC (V) 1200 1000 800 600 400 200 0 1 4 0.8 0.6 2 0.4 Grid Voltage (kV) 0.2 0 0 Corona Voltage (kV) Figure 8: voltage experienced by PC vs. Corona and Grid voltage Dark-Decay Analysis Dark decay is one of the properties of the PC. It is the amount of charge lost on a charged photoconductor without light exposure. This property is very important as it directly affects the image quality. Therefore, an experiment was done to characterize the dark-decay property of the PC. The PC was charged up using Grid voltage = 1.5kV and Corona voltage = 6kV. It is then moved above an ESVM probe to be measured. A graph of the voltage measured for 3 minutes after the photoconductor is charged shown in Figure 9 displays the dark decay characteristics of the photoconductor. PC Voltage Drop Due to Dark-Decay 1100 1050 1000 PC Voltage (V) 950 900 850 800 750 700 650 0 20 40 60 80 100 120 Time (sec) 140 Figure 9: PC voltage vs. time in a dark room 160 180 200 X-Y PC Voltage Measurement Measurement throughout the entire photoconductor plane after exposure system is one of the possibilities that can be done with the ESVM. The whole area can be measured with the photoconductor moving incrementally along the main drive direction (x-axis) while another servo (Figure 10) drives the probe back and forth in the y-axis. This method is going to be time consuming, thus prone to dark-decay effects. However, the dark-decay property of the photoconductor is known by the experiment from the previous section (Dark Decay Analysis). Therefore, the distorted image can be restored and this is explained in next section (Image Restoration after Exposure). Figure 10 The servo shown in Figure 10, MA2512W1-S2.5, needs to be mounted after the exposure system. It will be driven back and forth with the exact same setup as the main screw motor used to drive the PC. The ESVM probe will be mounted on the post of the servo. Every sample measurement the ESVM take will need to be accompanied by a time stamp for the reason of image restoration. The state machine needed to perform the task is shown in Figure 11 Figure 11: state machine for offline x-y measurement of PC voltage Data Restoration after Exposure In the possible offline process where the voltage across the entire PC plane is obtain by the ESVM, the signal will be a 1D series of voltages as described in the previous section (X-Y PC Voltage Measurement). Due to the nature of the process being time consuming, dark-decay effect will be significant. Therefore, the data restoration is required in order to obtain the correct voltage reading. Each voltage reading sample must has an time stamp indicating when it was measured for the restoration process to work properly. The following MatLab code is capable of simulating how dark-decay can affect the data as well as restoring the original value. The code first loads an image (Figure 12) and create the sampled image (Figure 13). It then creates the1D series of the voltage readings. Next the code creates a lookup table for the dark-decayed value with the corresponding original voltage and the time elapsed. It will use this table to simulate what the dark-decay data will look like (Figure 14). Figure 16 shows the series of the unaffected voltage in blue and the dark decayed reading in red. The code will then use the same table to restore the image as shown in Figure 15. Figure 15: restored image 1000 Figure 12: original image 950 900 850 800 750 Figure 13: sampled image 700 0 10 20 30 40 50 60 70 80 90 100 Figure 16: original (blue) and dark-decayed (red) samples Figure 14: dark-decayed image %the point of this program is to %demonstrate how to use the %dark decay data to restore the %image from the data value %measured by the ESVM in both %x and y direction %lower case letters %refer to continuous image %upper case letters %refer to sampled image clear all clc %creating an sampled ideal image, I i = double(imread('cameraman.tif')); XsampleN=30; YsampleN=50; [x,y]=size(i); Xinc=round(x./XsampleN-0.5); Yinc=round(y./YsampleN-0.5); n=1; for Y=1:YsampleN for X=1:XsampleN I(X,Y)=i(Xinc*X,Yinc*Y); n=n+1; end end figure; imshow(i,[min(min(i)),max(max(i))]) figure; imshow(I,[min(min(I)),max(max(I))]) %generate the 1D series of voltage %values read from ESVM, I1d(1,:) n=1; for Y=1:2:YsampleN for X=1:XsampleN I1d(1,n)=I(X,Y); n=n+1; end n=n+XsampleN; end n=1+XsampleN; for Y=2:2:YsampleN for X=XsampleN:-1:1 I1d(1,n)=I(X,Y); n=n+1; end n=n+XsampleN; end %assigning time field, t, to I1d(2,:) Xscan_time=2; %time it takes to scan across x-dir Yscan_time=2; %time it takes to scan across y-dir Xsps=Xscan_time/XsampleN; %second per sample in x-dir Ysps=Yscan_time/YsampleN; %second per sample in y-dir n=1; t=0; for Y=1:YsampleN for X=1:XsampleN I1d(2,n)=t; n=n+1; t=t+Xsps; end t=t-Xsps+Ysps; end %adding dark decay effect to I1d load LookUpTable.mat I1d(1,:)=... I1d(1,:)*.2+(1000max(I1d(1,:)*.2)); %normalize I1d(1,:) %setting values to the closed %there is from teh look up table for n=1:length(I1d) Diff=abs(SV-I1d(1,n)); Min=min(Diff); k=find(Diff<Min+1e-6); I1dNew(1,n)=SV(k); I1dInd(1,n)=k; end for n=1:length(I1d) Diff=abs(TF-I1d(2,n)); Min=min(Diff); k=find(Diff<Min+1e-6); I1dNew(2,n)=TF(k); I1dInd(2,n)=k; end %adding dark decay effect for n=1:length(I1d) I1dDD(1,n)=... LUT(I1dInd(2,n),I1dInd(1,n)); end I1dDD(2,:)=I1dNew(2,:); %removing dark decay effect from I1dDD for n=1:length(I1d) Diff=abs(TF-I1dDD(2,n)); Min=min(Diff); k=find(Diff<Min+1e-6); I1dR(2,n)=TF(k); I1dInd(2,n)=k; end for n=1:length(I1d) Diff=... abs(LUT(I1dInd(2,n),... :)-I1dDD(1,n)); Min=min(Diff); k=find(Diff<Min+1e-6); I1dR(1,n)=SV(k); %I1dR=1d recovered signal from dark decay end %wrap up the 1D signal to 2D to create image %image without dark decay fix n=1; for Y=1:2:YsampleN for X=1:XsampleN I2dDD1(X,Y)=I1dDD(1,n); n=n+1; end n=n+XsampleN; end n=1+XsampleN; for Y=2:2:YsampleN for X=XsampleN:-1:1 I2dDD1(X,Y)=I1dDD(1,n); n=n+1; end n=n+XsampleN; end figure; imshow(... I2dDD1,[min(min(I2dDD1))... ,max(max(I2dDD1))]) %image with dark decay fix n=1; for Y=1:2:YsampleN for X=1:XsampleN I2dR(X,Y)=I1dR(1,n); n=n+1; end n=n+XsampleN; end n=1+XsampleN; for Y=2:2:YsampleN for X=XsampleN:-1:1 I2dR(X,Y)=I1dR(1,n); n=n+1; end n=n+XsampleN; end figure; imshow(... I2dR,[min(min(I2dR)),... max(max(I2dR))]) figure; plot(I1d(2,:),I1d(1,:)); hold on; plot(I1d(2,:),I1dDD(1,:),'r') Voltage vs. Exposure Measurement A very important property of the PC is how much the voltage drop with respect to the change in exposure level. Therefore a test was conducted to obtain this information. The method involved in this experiment was to first create a gradient image (Figure 17) onto a transparency so that it can be used as the mask for the exposure system. The luminance was then measured across the mask. The ESVM probe placed after the exposure system was used to capture the voltage on the PC after it has been exposed to the gradient mask. The result is shown in Figure 18. Figure 17 600 500 Series1 Poly. (Series1) Voltage (V) 400 Power (Series1) 300 y = 2E-08x6 - 5E-06x5 + 0.0005x4 - 0.0286x3 + 0.8901x2 - 21.804x + 716.98 200 y = 839.76x-0.211 100 0 0 20 40 Luminance 60 80 100 (cd/m2) Figure 18 High Power System Rewiring The work done for the High Power System Rewiring was mainly for getting rid of the old control box. Removing the old control box required disconnecting and reconnecting all the wires that powers the entire Iron Butterfly’s subsystems. Documentation of the new high power system flow diagram and circuitry are shown in Figure 19 and Figure 20 respectively. Figure 19 Figure 20