SBIR-STTR Award

Three-Stage Cryocooler Cold Head for Advanced Heterodyne Sensors
Award last edited on: 11/3/2024

Sponsored Program
SBIR
Awarding Agency
NASA : JPL
Total Award Amount
$1,056,497
Award Phase
2
Solicitation Topic Code
S16.07
Principal Investigator
Darren King

Company Information

CU Aerospace LLC

3001 Newmark Drive
Champaign, IL 61822
   (217) 239-1703
   cuaerospace@cuaerospace.com
   www.cuaerospace.com
Location: Single
Congr. District: 13
County: Champaign

Phase I

Contract Number: 80NSSC22PB004
Start Date: 7/20/2022    Completed: 1/25/2023
Phase I year
2022
Phase I Amount
$156,499
Future advanced heterodyne sensors for submillimeter-wave receivers require 50 to 100 mW of cooling at 15 to 20 K for the sensor, and 1 to 2 W cooling at 80 to 120 K for the local oscillator, with size and input power suitable for use in a Small Sat. A 3-stage pulse tube cryocooler is well-suited for this type of application, offering a simple, reliable option with TRL 5 heritage in a larger cryocooler size, and allowing a design optimized to the sensor’s cooling and temperature requirements. CU Aerospace (CUA) will use innovative materials and low cost cold head design and assembly, coupled with Lockheed Martin’s (LM) industry-leading multi-stage pulse tube expertise, to provide NASA with a compact, affordable cryocooler for submillimeter detectors. Our team proposes to: 1) Perform a thorough thermodynamic trade study of 2-stage and 3-stage cold head configurations optimized to provide simultaneously 50-100 mW cooling at 15-20 K and 1-2 W cooling at 80-120 K, to achieve high efficiency, low mass, and compact packaging. Different regenerator materials and heat exchanger configurations will be included in the trade study. 2) Additively manufacture using Direct Metal Laser Sintering an optimized finned heat exchanger and demonstrate its capability to survive thermal cycling when press-fit into a cold head flange. 3) Generate a solid model of the cold head during Phase I so that it is ready for procurement, assembly, and testing in Phase II. 4) Continue the process of qualifying CUA to provide flight cold head subassemblies for future LM Space programs as a way to reduce cost and schedule. This work will leverage the MDA SBIR Phase II as well as CU Aerospace’s past flight hardware development and delivery on programs such as Propulsion Unit for Cubesats (PUC) delivered to the Air Force. Potential NASA Applications (Limit 1500 characters, approximately 150 words): Three-stage cryocoolers are generally required when cooling to 15-20 K as required by heterodyne sensors. Staged pulse tubes are ideally suited for space applications because adding stages does not add moving parts, such as with Stirling or Brayton coolers, so reliability remains high. NASA heterodyne sensors, as well as other instruments requiring temperatures from 10-30K would benefit from a low-mass, reliable 3-stage pulse tube cryocooler to improve mission capability. Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words): Multiple-stage cryocoolers can benefit all cryogenic space applications by cooling secondary components and intercepting parasitic heat loads at higher temperature, reducing power and mass. Applications including remote sensing satellite constellations, weather satellite constellations, earth science instruments, and deep space astrophysics instruments can all benefit from multiple-stage cooling. Duration: 6

Phase II

Contract Number: 80NSSC23CA089
Start Date: 6/1/2023    Completed: 5/31/2025
Phase II year
2023
Phase II Amount
$899,998
Future advanced heterodyne sensors for submillimeter-wave receivers require 50 to 100 mW of cooling at 15 to 20 K for the sensor, and 1 to 2 W cooling at 80 to 120 K for the local oscillator, with size and input power suitable for use in a Small Sat. During Phase I, a detailed cryocooler configuration trade study was completed, and the 3-stage pulse tube configuration driven by the Lockheed Martin (LM) Midi compressor was selected based on efficiency and adaptability. An assessment of innovative regenerator materials and direct metal laser sintering (DMLS) additively-manufactured heat exchanger materials was completed, and the decision was made to include DMLS in the design, while keeping the advanced regenerator material as an option as a future improvement. Cooling powers of 100 mW at 20 K and 2 W at 120 K were selected, with 47 W compressor ac power predicted. A solid model of the 3-stage cold head was then generated in Phase I. CU Aerospace (CUA) will use innovative materials and low cost cold head design and assembly, coupled with LM’s industry-leading multi-stage pulse tube expertise, to provide NASA with a compact, affordable cryocooler for submillimeter detectors. Our team proposes to: 1) Refine the 3-stage cold head solid model design initiated in Phase I, optimized to provide simultaneously 100 mW cooling at 20 K and 2 W cooling at 120 K, to improve manufacturability and decrease cost compared with heritage LM multi-stage cold heads. 2) Procure all hardware necessary to assemble the 3-stage cold head, and the gas transfer line to connect it to a LM-owned Midi compressor. 3) Assemble and weld 3-stage cryocooler cold head, perform proof pressure testing and leak testing. 4) Integrate cold head with LM Midi compressor and perform cryocooler performance testing over a range of operating conditions, varying the input power, ambient temperature and 1st, 2nd and 3rd stage temperatures to fully characterize cryocooler performance. Anticipated

Benefits:
Three-stage cryocoolers are generally required when cooling to 15-20 K as required by heterodyne sensors. Staged pulse tubes are ideally suited for space applications because adding stages does not add moving parts, such as with Stirling or Brayton coolers, so reliability remains high. NASA heterodyne sensors, as well as other instruments requiring temperatures from 10-30K would benefit from a low-mass, reliable 3-stage pulse tube cryocooler to improve mission capability. Multiple-stage cryocoolers can benefit all cryogenic space applications by cooling secondary components and intercepting parasitic heat loads at higher temperature, reducing power and mass. Applications including remote sensing satellite constellations, weather satellite constellations, earth science instruments, and deep space astrophysics instruments can all benefit from multiple-stage cooling.