PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel...
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Transcript of PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel...
![Page 1: PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA)](https://reader030.fdocuments.net/reader030/viewer/2022032709/56649ec55503460f94bd0c51/html5/thumbnails/1.jpg)
PLATO Main Electronics Units (MEU)based on inputs from P. Plasson and the system team
J. Miguel Mas-Hesse
Centro de Astrobiología (CSIC-INTA)
![Page 2: PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA)](https://reader030.fdocuments.net/reader030/viewer/2022032709/56649ec55503460f94bd0c51/html5/thumbnails/2.jpg)
PLATO Kick Off November 2010 J. Miguel Mas-Hesse 2
On-board data processing: Introduction
Stellar field PLATO image
• DPS goal: automatically process and extract accurate stellar light curves from the raw, messy CCD images.
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 3
On-board data processing: baseline concept
• The normal-telescopes onboard data processing system will be formed by:
– 4 CCD + 1 FEE per focal plane (telescope)• 32 telescopes
– 1 Data Processing Unit (DPU) per 2 focal planes• 16 DPU boards
– 4 DPUs per 1 Main Electronics Unit (MEU)• 4 MEU boxes
– 1 Instrument Control Unit (ICU) per 4 MEUs• 1 ICU (+ 1 fully redundant ICU)
![Page 4: PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA)](https://reader030.fdocuments.net/reader030/viewer/2022032709/56649ec55503460f94bd0c51/html5/thumbnails/4.jpg)
PLATO Kick Off November 2010 J. Miguel Mas-Hesse 4
On-board data processing: architecture
1 N-DPU for 2 N-cameras
F-cameras
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 5
On-board data processing: architecture
Present MEU baseline concept:
+ 1 DPU per 2 focal planes+ 1 single DPU PSU box, external to the MEU’s
To ICU-M To ICU-R
SpW
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 6
PLATO MEU: FEE – DPU SpW link
• FEE – DPU link baseline:– 2 SpaceWire links per FEE (100 Mbps)
• Alternative:– 1 SpaceWire link per FEE (200 Mbps)
• Feasibility has to be demonstrated.
SpW 100 Mbps
![Page 7: PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA)](https://reader030.fdocuments.net/reader030/viewer/2022032709/56649ec55503460f94bd0c51/html5/thumbnails/7.jpg)
PLATO Kick Off November 2010 J. Miguel Mas-Hesse 7
On-board data processing: architecture
![Page 8: PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA)](https://reader030.fdocuments.net/reader030/viewer/2022032709/56649ec55503460f94bd0c51/html5/thumbnails/8.jpg)
PLATO Kick Off November 2010 J. Miguel Mas-Hesse 8
On-board data processing: architecture
![Page 9: PLATO Main Electronics Units (MEU) based on inputs from P. Plasson and the system team J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA)](https://reader030.fdocuments.net/reader030/viewer/2022032709/56649ec55503460f94bd0c51/html5/thumbnails/9.jpg)
PLATO Kick Off November 2010 J. Miguel Mas-Hesse 9
PLATO MEU: operation
Window Extraction
up to 330.000 stars / 25 sec
FullimageAcquisition x 82 images / 6.25 sec
Data correction and LC extraction
Masks & window positions
updating
6.25 sec
6.25 sec
6.25 sec
5400sec
• Target count for 2 x 4 CCD per DPU (to be processed every 25 sec.):
Nominal sample 2x(110.000 stars/telescope) = 220.000 stars/DPU Extended sample (+50% margin) = 330.000
stars/DPU Background win. 2 x 400 Imagettes up to 2 x 2.000 Offset windows 2 x 2 x 4 half-row (2.255 pixels) Smearing rows 2 x 4 x 10 overscan rows
• Total memory requirement, including 50% margin on star count: 250 Mbytes per DPU
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 10
PLATO MEU: CPU load
• The CPU load has been estimated for various processors, based on current baseline for number of stars + extraction algorithms. At this phase the %CPU load should be ≤ 50%.
• The present concept seems feasible, but:– with 1 DPU/2 telescopes, no margin on star counts acceptable.
– with 1 DPU/telescope an extended sample with +50% margin in star counts could be considered, if required. .
Weighted mask photometry assumed
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 11
PLATO MEU: open points
SpaceWire
Router(M)
SpaceWire
Router(R)
Power Supply(M + R)
N-DPU #1
N-DPU #2
N-DPU #3
N-DPU #4
SpW
MEU
SpW
To redundant ICU
To main ICU
235 kbps
235 kbps
235 kbps
235 kbps
<1 Mbps
Test I/F - SpW
180 Mbps(2 x 64 x 1.4)
4 Mpx/s
SpWI/F
ADC
ADC
FEE #14510 px
4510
px
SpWI/F
ADC
ADC
FEE #24510 px
4510
px
SpWI/F
ADC
ADC
FEE #34510 px
4510
px
SpWI/F
ADC
ADC
FEE #44510 px
4510
px
Power Distribution
HK
Cmd
28 V, Cmd from S/CM + R
Backup concept:
+ 1 DPU board per telescope+ 4 DPUs per MEU+ 8 MEU More powerful, but too heavy
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 12
PLATO MEU: open points
Baseline Alternative
Number of telescopes per DPU
2 1
MEU-PSU 1 MEU-PSU box for 4 MEU boxes
4 MEU-PSU inside each MEU box
FEE / DPU number of SpaceWire links
2 SpaceWire links per FEE (100 Mbps)
1 SpaceWire links per FEE (200 Mbps)
FEE DPU image transfer mechanism and protocol
RMAP DMA transfer tables
DPU Boot mechanism Boot Software in PROM Pure RMAP hardware boot
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PLATO Kick Off November 2010 J. Miguel Mas-Hesse 13
PLATO: next steps
• The industrial MEU definition study is starting now.
• Goals: – Definition and dimensioning of the N-DPUs
• Global architecture, choice of processors, number of SpaceWire data links, location of PSUs, mass, power comsumption,…
• Trade off on algorithms potential increase of complexity
– Development of simulators/breadboards for critical interfaces
• Spacewire link FEE – DPU
Final design within mass and power budgets, but compliant with scientific requirements!