DA-FC-MPAE-RP-286
Issue: 1
Revision: -
02/09/2008
Prepared by:
Thorsten Maue
Pablo Gutierrez
prepared by: Thorsten Maue (signature/date)
approved by: put name here (signature/date)
Iss./Rev. Date Pages affected Description Draft all first draft
Holder Issue/Revision D 1 2 Configuration File (Doc) MPS KMA Aye IB Büttner JB Bukatz UC Christensen RE Enge WG Goetz PGM Gutierrez-Marques HH Hartwig HUK Keller WK Kühne AN Nathues HP Perplies MR Richards RS Schäfer KS Schneider ISE Sebastian HIS Sierks MS Sperling ISZ Szemerey DLR Carsenty DLR Jaumann DLR Mottola IDA Fiethe IDA Michalik IDA Bubenhagen JPL Miller JPL Pavri OSC Violet Legend: A - Approval C - Copy U - Updated Pages
1. General aspects...................................................1 1.1 Scope .......................................................1 1.2 Introduction ................................................1 1.3 Applicable Documents ........................................1 1.4 Reference Documents .........................................1 2. Extra charge measurements.........................................2 2.1 FC1..........................................................2 2.1.1 DC014 ...................................................2 2.1.2 DC018 ...................................................3 2.1.3 Comparison of different parts of the CCD ................5 2.2 FC2.........................................................8 2.2.1 DC014 and DC018 ..........................................8 3. Operational log...................................................8
Figure 1: Histogram of pixels showing extra charge ..........................2 Figure 2: Accumulated histogramof pixels showing extra charge................3 Figure 3: Histogram of pixels showing extra charge (DC014 vs. DC018) ........4 Figure 4: Accumulated histogram of pixels showing extra charge (DC014 vs. DC018)............................................................4 Figure 5: Extra charge on FC1 with pre-clear.................................5 Figure 6: Accumulated histogram of lower left 256 x 256 pixels...............6 Figure 7: Accumulated histogram of upper right 256 x 256 pixels .............6 Figure 8: Accumulated histogram of lower left 256 x 256 pixels...............7 Figure 9: Accumulated histogram of lower left 256 x 256 pixels...............7 Figure 10: Accumulated histogramof pixelsshowing extra charge (FC1 vs. FC2)..8
This document reports the results of the operation of the Dawn Framing Cameras in the frame of DC018.
The Framing Camera test slot within DC018 was intended to be a verification that the measures identified to counter the phenomenon known as 'extra charge' were working properly.
To this end, both cameras were operated one at a time, performing the set of operations known as 'CCD mini cal'. This set includes some image acquisitions aimed at the detection and evaluation of extra charge.
Operationally, the test was a success: all 72 images were retrieved from each of the cameras with only the minor hiccups known to be tied to the pause and resume of continuous playback.
The functional performance of the extra charge countermeasures is reported in the section below.
Section 3 includes the operational log from the F]\C team.
no. document name document number, Iss./Rev. AD1
no. document name document number, Iss./Rev.
2.1.1 DC014
The extra charge measurements during DC014 where done with different pre illumination times, allowing the extra charge to accumulate prior to the exposure. Figure 1 shows the frequency of DNs all the 1024x1024 pixels. The six different graphs show the level of extra charge for six different illumination times (from bottom to top: 1.3s, 2.3s, 3.3s, 4.3s, 6.3s, 11.3s). The most effected pixels show extra charge of up to 200 DNs.
Figure 1: Histogram of pixels showing extra charge for FC1 in DC014
Figure 2 shows how many percent of the pixels show less DNs of extra charge as plotted on the y-axis (from top to bottom: 1.3s, 2.3s, 3.3s, 4.3s, 6.3s, 11.3s). In the best case 90% of all pixels have less than 20 DNs of extra charge.
Figure 2: Accumulated histogram of pixels showing extra charge for FC1 in DC014
2.1.2 DC018
With the new UDP for 'pre-clearing' the CCD uploaded in DC018, the minimum time between clearing the CCD and readout was reduced from 1.35 s to 0.200 s. This shorter illumination time allows less extra charge to accumulate. But since the extra charge charges on an exponential function, still most of the extra charge is present prior to the exposure (compare Figure 3 and Figure 4).
Figure 3: Histogram of pixels showing extra charge (DC014 vs. DC018) for FC1
Figure 4: Accumulated histogram of pixels showing extra charge (DC014 vs. DC018) for FC1
2.1.3 Comparison of different parts of the CCD
The varying flux of the cal lamp, depending on the location on the CCD, produces a signal of 15 DN/ms in the rightmost column and 5 DN/ms in the leftmost column. In addition to the nonuniform flux, the CCD even with uniform flat fields produces more extra charge in the upper right corner. This results in a distribution of the extra charge as seen in Figure 5.
Figure 5: Extra charge on FC1 with pre-clear
Two different squares of the whole 1024 x 1024 CCD were analyzed: The most affected 256 x 256 upper right pixels and the least affected 256 x 256 lower left pixels.
The lower left part of the CCD showed only.
Figure 6: Accumulated histogram of lower left 256 x 256 pixels of FC1 in DC014
Figure 7: Accumulated histogram of upper right 256 x 256 pixels of FC1 in DC014
Figure 8: Accumulated histogram of lower left 256 x 256 pixels of FC1 in DC018
Figure 9: Accumulated histogram of lower left 256 x 256 pixels of FC1 in DC018
2.2.1 DC014 and DC018
In both, DC014 and DC018 no traces of extra charge could be found in the data from FC2. Figure 10 shows the random distribution of noise on FC2 (left graph), maximum is less than 5 DNs, in comparison with the best case extra charge on FC1 (right graph) where 95% of the pixels show less than 25 DNs of extra charge.
Figure 10: Accumulated histogram of pixels showing extra charge (FC1 vs. FC2)
2008-08-25T22:15:00
EGSE server setup. Connection received at low speed
22:35:00 S/C changed to RT124 K
FC1 CCD 19 to 21 C
FC1 CCD heater duty cycle ~50%
FC1 CH -18.8 to -18.4 C
FC1 CH heater duty cycle ~15%
FC1 I/F -2.4 to -2.1 C
FC2 CCD 20 to 22 C
FC2 CCD heater duty cycle ~55%
FC2 CH -18.8 to -18.4 C
FC2 CH heater duty cycle ~15%
FC2 I/F -3.4 to -3.2 C
22:37:11 Radiated dz097a (ERT 23:16:22)
22:42:31 Radiated dz109a (ERT 23:21:42)
23:17:00 As expected, FC1 CCD heater is off
23:20:40 FC1 CCD -10 C
CH heater duty cycle on the rise
23:23:20 FC1 CCD -20 C
23:24:20 FC2 CCD heater is off
23:25:00 FC1 CCD -24.6 C
FC2 CCD 10.0 C
23:26:30 FC1 CCD -27.5 C
FC2 CCD 0.0 C
23:28:00 FC1 CCD -30.0 C
FC2 CCD -7.5 C
23:31:50 FC1 CCD -35.4 C
FC2 CCD -20.0 C
23:35:30 FC1 CCD -39.4 C
FC1 CCD heater duty cycle 0%
FC1 CH -18.8 to -18.4 C
FC1 CH heater duty cycle ~30%
FC1 I/F -2.4 to -2.1 C
FC2 CCD -27.5 C
FC2 CCD heater duty cycle 0%
FC2 CH -18.8 to -18.4 C
FC2 CH heater duty cycle ~25%
23:40:00 FC Off net
2008-08-26T18:56:26 Connection received at low speed
FC on Dawn Ops network
19:09:22 Radiated dz286g (ERT 19:48:32)
19:15:50 FC1 CCD -63.2 C
FC1 CCD heater duty cycle 0%
FC1 CH -18.9 to -18.3 C
FC1 CH heater duty cycle ~0.45%
FC1 I/F -2.5 to -2.4 C
FC2 CCD -64.2 C
FC2 CCD heater duty cycle 0%
FC2 CH -18.9 to -18.3 C
FC2 CH heater duty cycle ~40%
FC2 I/F -3.6 to -3.5 C
19:50:40 FC1 is on
FC1 Primary 28V current 0.288 A
After boot 0.355
The current profile matches that of a typical FC boot
19:55:00 The UDP library was properly patched
19:57:50 FEE is on
20:50:30 As in previous runs of CCD mini cal, the last images of the CALExtraChargeBlock (IDs 964 and 965) are dark because the cal lamp was switched off too early.
20:54:45 Door opened nominally
21:00:00 Filter wheel started to turn
21:10:00 FC1 CCD -53.6 C
FC1 CCD heater duty cycle 0%
FC1 CH -16.0 C
FC1 CH heater duty cycle 0%FC1 I/F +5.0 C
FC2 CCD -64.2 C
FC2 CCD heater duty cycle 0%
FC2 CH -18.8 to -18.4 C
FC2 CH heater duty cycle ~40%
FC2 I/F -1.2 C
21:12:20 Door closed nominally
21:17:40 FEE is off
23 images left for compression
21:30:40 Preliminary assessment of the early 60 s extra charge images already confirms an improvement by using the pre-clear. More detailed analysis is yet to come.
21:41:50 All images transmitted to VR8. SCET 21:21:16
22:09:10 Upon a first inspection of the images, no streaks were found. Mebsuta (Eps Gem) was easily identifiable as the brightest star, together with many other of lower brightness.
Milbus noise was visible on images 969 and 970 (F1), and in serial readouts.
Straylight due to Sun incidence was not visible. The angle between the sun and the boresight vector is 68.44 deg
22:28:30 FC1 is off. CCD heading for cruise temperature
FC1 CCD -18.2 C
FC1 CCD heaters duty cycle 70%
FC1 CH -18.9 C
FC1 CH heater duty cycle ~15%
FC1 I/F +5.0 C
FC2 CCD -64.2 C
FC2 CCD heaters duty cycle 0%
FC2 CH -18.3 C
FC2 CH heater duty cycle ~45%
FC2 I/F -0.3 C
The team is GO for upload of FC2 sequence dz296c
22:34:08 Radiated dz296c (ERT 23:13:18)
23:11:00
FC1 CCD -21.5 C
FC1 CCD heaters duty cycle ~50%
FC1 CH -18.3 C
FC1 CH heater duty cycle ~20%
FC1 I/F +1.2 C
FC2 CCD -64.2 C
FC2 CCD heaters duty cycle 0%
FC2 CH -18.3 C
FC2 CH heater duty cycle ~45%
FC2 I/F -1.2 C
23:16:00 FC2 is on. Current consumption is 0.269 A, then 0.349 A
23:17:20 FC2 is fully booted.
23:19:10 The UDP library was properly patched
23:21:10 FEE is on
2008-08-27T00:14:00 As in previous runs of CCD mini cal, the last images of the CALExtraChargeBlock (IDs 949 and 950) are dark because the callamp was switched off too early.
00:18:50 Door opened nominally
00:25:10 Filter wheel moved successfully
00:27:00 FC1 CCD -20.9 C
FC1 CCD heater duty cycle 50%
FC1 CH -18.3 C
FC1 CH heater duty cycle ~10%
FC1 I/F +0.5 C
FC2 CCD -55.2 C
FC2 CCD heater duty cycle 0%
FC2 CH -16.0 C
FC2 CH heater duty cycle 0%
FC2 I/F +4.5 C
00:36:20 Door closed nominally
00:41:20 FEE is off
21 images left for compression
Preliminary assessment of the images confirms that FC2 is free from extra charge.
The final packet of the last image of FC1 was apparently not received. It can probably be reconstructed offline from the data stream.
01:03:30 All images transmitted to VR8. SCET 00:43:17
01:27:30 As for FC1 all images were received except the last one, pending one packet.
On a preliminary inspection no streaks were found.
01:54:00 FC2 is off. CCD heading for cruise temperature
FC1 CCD 19.0 C
FC1 CCD heaters duty cycle 50%
FC1 CH -18.3 C
FC1 CH heater duty cycle ~15%
FC1 I/F +0.9 C
FC2 CCD -39.4 C
FC2 CCD heaters duty cycle 70%
FC2 CH -18.3 C
FC2 CH heater duty cycle 0%
FC2 I/F +4.1 C
After a final playback, the last packet(s) of FC2 data came to complete the last FC2 image.