plato at asi tues 05/may/09dave walton plato meeting rome tues 5/may/09 focal plane dave walton...
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Plato at ASI Tues 05/May/09 Dave Walton
Plato meeting Rome Tues 5/May/09
Focal Plane
Dave Walton UCL/MSSL, + Leicester University
Miguel Mas INTA/CAB + LIDAX (Javier Serrano mechanical + thermal)
Recent changes, current issues etc. in red
Plato at ASI Tues 05/May/09 Dave Walton
FPA: location in relation to telescope
Plato at ASI Tues 05/May/09 Dave Walton
TOU FLANGE
SUPPORT BIPODS (x4)
FEE Box
COLD PLATE
CCDS Assembly
PLATO – FPA & FEE Design Concept (2009-04-30)PLATO – FPA & FEE Design Concept (2009-04-30)
80mm
OPTICAL BENCH
MLI
Plato at ASI Tues 05/May/09 Dave Walton
PLATO – FPA & FEE Design Concept (2009-04-30)PLATO – FPA & FEE Design Concept (2009-04-30)
SUPPORT BIPOD
THERMAL STRAPS (x4)
Flex Cable
CCDs Support Plate
CCDCCD Base
Plato at ASI Tues 05/May/09 Dave Walton
SPACE
TOUHEATER
158K-168K
0.49 W-0.88W
COLD PLATE
FLEXCABLES (4mW/K)
2.51W-2.12 W
FEE
FPA 159K-169K
249K-308K
243K-303K
OB OB
MLI
158K-168K
PLATO – FPA & FEEThermal Performance (2009-04-30)PLATO – FPA & FEEThermal Performance (2009-04-30)
1.5W-1.9 W
1.0W
3.0W Temperature (pink): assumption
Temperature (blue): result
COLD-HOT CASES
243K-303K
Plato at ASI Tues 05/May/09 Dave Walton
1. Concept design based on FEE in an independent box on Cold Plate and FPA attached to TOU is shown
2. Two different thermal cases (cold & hot) have been analyzed
3. Thermal performance for both cases is according to requirements, but assumptions must be confirmed by system level
4. Spatial gradients across CCDs are about 0.1K
5. Temporal gradients on CCD shall mainly depend on TOU temporal gradient
6. If TOU temporal gradient is >1K/40 days (FPA Requirement), heaters on FPA will be required to comply with 1K/40 days gradient
PLATO – FPA & FEE Thermo-mechanical conclusions (2009-05-05)PLATO – FPA & FEE Thermo-mechanical conclusions (2009-05-05)
Plato at ASI Tues 05/May/09 Dave Walton
PLATO FPA Thermo-mechanical Design Mass BudgetPLATO FPA Thermo-mechanical Design Mass Budget
Mass Budget (per FPA, including FEE & CCDs)
ITEM MASS
CCDs 600
CCD Support Plate 110
FEE bracket 470
FEE lower cover 260
FEE 470
Thermal strap 88
TOTAL 1998
TOTAL with 20% margin 2398
Plato at ASI Tues 05/May/09 Dave Walton
CCD: Using Gaia for prototyping
Gaia CCD at MSSL
Plato CCD characteristics
• Flight: 42 telescopes, 4 CCDs per telescope -> 168 flight CCDs.
•Each CCD 3584x3584 18µm pixels.Full-frame (except for 2 bright-source telescopesusing same chip butframe transfer).Red-enhanced AR coating.
• Thin oxide and doping to increase full-well to ~1Me-.
Plato at ASI Tues 05/May/09 Dave Walton
Normal telescope electrical architecture
• 8 output ports multiplexed into 2 ADCs
Plato at ASI Tues 05/May/09 Dave Walton
Normal telescope: Time-multiplexing of CCDs
• In order to remain close to FEE power budget, may be necessary to unpower CCD output nodes when not active
Plato at ASI Tues 05/May/09 Dave Walton
Fast telescope electrical architecture
• Due to high duty cycle, 1 ADC per port required.• Similarly, unpowering of CCD output stages not possible• Therefore, power consumption significantly higher than normal telescope,
so just as well there are only two.
Plato at ASI Tues 05/May/09 Dave Walton
Normal and fast telescope power calculations
* Not using CCD dummy outputs * Normal telescope duty cycle: 4s each 25s
Power in mW, per telescope
NormalPower-cycled
NormalContinuous power
BUDGET FastContinuous power
BUDGET
FPA, 2ndary
314 717 1000 2925 2500
FEE, 2ndary
3530 5217 3000 11203 7000
TOTAL, primary
5491 8478 5700 20182 13600
Plato at ASI Tues 05/May/09 Dave Walton
CCD Procurement: Delivery rate
• Potentially 42 telescopes, -> 168 flight CCDs.
e2v confirm this is feasible in a 3-phase programme:Phase 1: Development activities – 18 monthsPhase 2: Evaluation activities and FM preparation – 18 monthsPhase 3: FM manufacturing – 6 month startup, 18 months delivery (~10 per month)Total duration: 5 years, so needs early planning.
• ESA have queried delivery rate, based on Gaia rate.
• Response from e2v:* Agree the device is somewhat larger. However, from Gaia experience, more than half of yield loss was not area-related (e.g. mechanical packaging).* Plato delivery rate higher than Gaia, but not by a huge margin (~10 per month). Can be accommodated: more an issue of planning the resources rather than e2v’s capacity. e2v’s existing capacity 16 per month.* Cyril Vetel (Astrium) very pleased with progress of Gaia CCD procurement.
• For further clarification, MSSL will set up a meeting with representatives from e2v, PPLC and ESA
Plato at ASI Tues 05/May/09 Dave Walton
CCD Procurement: Increased full-well / dynamic-range
• Following discussions with e2v, full-well increased by combination of thin oxide and doping profile.
• In Dave Morris’s note, he assumed a lower yield for thin oxide devices, and was satisfied that the delivery rate could be achieved. Recent tests by e2v of small area devices showed a similar yield to normal devices.
Plato at ASI Tues 05/May/09 Dave Walton
CCD Temperature
• PDD assumed TCCD ~-100 C (173 K).• Design/implementation simpler if TCCD ~-70 C (203 K).• PPLC now adopts baseline of <-70 C (<203 K).
Issues:• Dark current: Not a problem at these temperatures (much lower than other noise sources)• CTE effects from irradiation-induced traps: the principal reason for -100C in PDD. Being addressed by simulation, comparison with Corot, Integral data.
Plato at ASI Tues 05/May/09 Dave Walton
Summary/Status FPA/FEE
• Design, layout, thermal modelling and power consumption calculations are progressing.
• Thermal modelling for normal telescopes consistent with requirements.
• Power consumption within PPLC budget for normal telescopes. Higher for fast telescopes, but these have a small impact on total power.
• Fast telescopes should now be thermally modelled (power numbers now available).
• Dynamic-range / full-well increased after discussion with e2v.
• CCD supply rate analysed, considered realistic.
• OVERALL: No show-stoppers, FPA/FEE considered to be within conservative feasibility.
Plato at ASI Tues 05/May/09 Dave Walton
Reserve slides
Plato at ASI Tues 05/May/09 Dave Walton
Alternative layout: To ease mounting to optical bench and cold plate
Plato at ASI Tues 05/May/09 Dave Walton
PLATO FPA Thermomechanical Design Previous Design from LIDAXPLATO FPA Thermomechanical Design Previous Design from LIDAX
MASK
SHIM
CCDs + CCD SUPPORT PLATE
FPA HOUSING
FEE + FEE SUPPORT PLATE
COVER
THERMAL STRAP