NASA SBIR 2018-I Solicitation

Proposal Summary


PROPOSAL NUMBER:
 18-1- S1.03-5363
SUBTOPIC TITLE:
 Technologies for Passive Microwave Remote Sensing
PROPOSAL TITLE:
 Low-Loss Millimeter-Wave Isolators for Cryogenic Systems
SMALL BUSINESS CONCERN (Firm Name, Mail Address, City/State/Zip, Phone)
Micro Harmonics Corporation
20 South Roanoke Street, Suite 202
Fincastle , VA 24090-3102
(540) 473-9983

Principal Investigator (Name, E-mail, Mail Address, City/State/Zip, Phone)
David Porterfield
david@mhc1.com
20 South Roanoke Street, Suite 202 Fincastle, VA 24090 - 3102
(434) 409-4044

Business Official (Name, E-mail, Mail Address, City/State/Zip, Phone)
Diane Kees
Diane@mhc1.com
20 South Roanoke Street, Suite 202 Fincastle, VA 24090 - 3102
(540) 473-9983
Estimated Technology Readiness Level (TRL) :
Begin: 5
End: 6
Technical Abstract

Ferrite based isolators are useful for controlling standing waves in a wide variety of millimeter-wave (MMW), and terahertz (THz) systems. A good example of their usefulness is found in high frequency local oscillator systems. These systems typically comprise a lower frequency oscillator driving a cascade of frequency multipliers. Standing waves arise due to impedance mismatches between the highly tuned components. This in turn gives rise to dips or even nulls in the output of the multiplier chain. The standing waves are often mitigated with complicated impedance matching techniques that are implemented on a case-by-case basis at a great cost in time and money. By using suitable isolators, the standing waves could be suppressed at a fraction of the time and cost.

The high insertion loss of these components renders them unsuitable for use in most MMW systems. The typical insertion loss of a WR-6.5 isolator (110-170 GHz) is more than 3 dB. The problem is worse at higher bands. Micro Harmonics Corporation has recently developed a revolutionary new line of isolators with significantly reduced insertion loss. Our WR-8 and WR-6.5 isolators have a measured insertion loss of less than 1 dB over most of the waveguide band. By April of this year, a full line of low-loss isolators covering bands from WR-12 (60-90 GHz) through WR-3.4 (220-325 GHz) will be available. 

Many NASA instruments are designed for use at cryogenic temperatures. However, cryogenically rated isolators are currently unavailable at frequencies above 40 GHz. Isolators designed for room temperature operation have poor isolation at cryogenic temperatures due to changes in the ferrite properties. The isolators must be fundamentally redesigned for cryogenic use. We propose to develop high-frequency isolators optimized for cryogenic temperatures that exhibit significantly reduced loss and improved isolation and bandwidth making them useful for many of the instruments now being developed for NASA missions.

Potential NASA Applications

Isolators are useful in a wide range of NASA systems including the heterodyne receivers used in Marvel, VESPER, MACO and SIRICE. They find potential application in the local oscillator (LO) chains for the high-resolution heterodyne array receivers at 1.9 THz used in the Stratospheric Observatory for Infrared Astronomy (SOFIA) and the Stratospheric Terahertz Observatory (STO-2) and the 4.7 THz multiplied local oscillator source for the observation of neutral oxygen.

Potential Non-NASA Applications

Isolators are broadly used in scientific instruments for plasma diagnostics (ITER), chemical spectroscopy, biomaterial analysis, and radio astronomy. There are applications in military systems such as compact range radar, imaging systems, covert communications systems, and chemical and bio-agent detection systems. There are applications in biomedical systems for the real time analysis of skin diseases, portal security scanners, high frequency data links and industrial process control systems.


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