The objective of the NASA OSAT Submillimeter Wave Sensors program is to develop components required for submillimeter wave heterodyne receiver systems and accurately characterize their performance. Performance requirements address the needs of NASA submillimeter space missions including the Submillimeter Astrophysics Mission (SAM) and the earth remote sensing EOS Microwave Limb Sounder (EOS MLS). Performance goals include extending technical capability to higher frequencies (1200 GHz in the near-term, 3000 GHz in the far-term), improving sensitivity an order of magnitude, and developing a viable array technology.
Near-term objectives include demonstration of astrophysics receivers near 600, 800 and 1200 GHz and Earth remote-sensing receiver capabilities at 640 GHz. Longer-term objectives include 1200 and 1800 GHz receivers for Earth remote-sensing programs, and receivers to 3000 GHz and receiver arrays for astrophysical applications.
OSAT Technology Contribution: Measuring and Understanding the Earth's Ozone Layer
Submillimeter Sensors Program Work Breakdown Structure (WBS).
Submillimeter Sensors Astrophysics Roadmap.
Submillimeter Sensors Earth Sensing Roadmap.
Submillimeter Sensing Superconductor-Insulator-Superconductor (SIS) Mixer Performance.
Quarterly Report for the first two quarters of fiscal year 1994 (October 1993 to March 1994).
The Center for Space Terahertz Technology at the University of Michigan is one of the eight NASA University Space Engineering Research Centers.