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K- band Focal Plane Array. K band History. Science workshop determined efficiency improvements necessary for K Band: weather, observing requests, mapping programs. - PowerPoint PPT Presentation
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K band History
• Science workshop determined efficiency improvements necessary for K Band: weather, observing requests, mapping programs.
• Only enough funds for the receiver only, so the project was de-scoped to seven pixels that meets science objectives as specified in the science case.– $1.2 M Total– $0.19 M Parts– $0.2 M Contingency– $0.83 M Labor
• The K band seven pixel focal plane array is the path finder instrument: a necessary first step and feasible considering time frame.
– Seven pixel array construction complete December, 2009 – Production use by November, 2010.
K band Focal Plane Array
• Science Driver → Map NH3
– Polarized without Rotation• Seven Beams → Limited by IF system• 1.8 GHz BW → Limited by IF system• 800 MHz BW → Limited by Spectrometer
K-band FPA Deliverables
• Frontend– Cryogenic Package for Seven Pixel Instrument– Seven Dual Circular Polarization K band Pixels – Modular Noise Calibration for each Pixel– Modular Downconverter for each Channel (14)– Monitor and Control Electronics– LO Distribution with Doubler for LO1A
• Software– Package for Engineering M&C – Observing Software Manager– Data Analysis Pipeline
• Cost per Pixel not including NRE.– $46,000 Parts (Dewar,EM parts, Isolator, HEMT Amp, WG parts, Noise Mod, IDM)– $2500 Labor Construction.– $2500 Software upgrades.
Focal Plane Coverage
simulated beam efficiencyvs. offset from center
1. Initial 7 elements above 68%beam efficiency (illuminationand spillover)
2. Expandable to as many as61 elements
3. beam efficiency of outermostelements would drop to ~60%.
4. beam spacing = 3 HPBWs
3 HPBW
K Band f = 22 GHz
28"
.177 HPBW/mm
= 13.36 mm88.9 mm
GBT Beam Spatial Coverage/ Resolution
GBT Aperture Spacing
Noise Temperature: 36 K max 18-26.5 GHz, 25 K over 75% of bandP1dB Headroom: 30 dB when Tant = 300 K
Noise Temperature and Headroom Limited byExisting Cryogenic LNA Design
Frequency Range: 18-26.5 GHz (17-27.5 GHz goal)
Cosine Taper Corrugated Feed Horn
K band OMT
K Band Single Pixel
Phase Shifter
Thermal Transition
OMT
Feed
Noise Module
HEMT
Isolators
Sliding Transition
Drawing of the 7 Pixel Design
KFPA Components
External Frame
Top Plate with 7 Feeds
Sliding Waveguide/Thermal Gap Assembly
Two downconverters are needed to implement the IF multiplexing scheme.The second downconverter simply omits the latter mixing stage.
Integrated Down Converter
Future FPA Developments Wish List
• Significantly enhanced spectrometer with this new array and existing IF system.
• New digital I.F. distribution system. (Spectrometer and technology dependent).
• Expanded focal plane array (perhaps at a different frequency: W band)