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Ground-Based Investigations with the Cryogenic Hydrogen MaserThe room temperature hydrogen maser is an active atomic oscillator used as a high-frequency-stability local oscillator for radio astronomy, metrology, and spacecraft navigation, and in tests of fundamental physics. The cryogenic hydrogen maser (CHM) operates at 0.5 K, employing superfluid helium-coated walls to store the masing hydrogen atoms. We are investigating whether the CHM may provide better frequency stability than the room temperature hydrogen maser: one to three orders of magnitude improvement may be possible because of greatly reduced thermal noise and larger signal power. Exceptional frequency stability will be required for spacecraft tracking in future deep-space missions, for space-based tests of relativity and gravitation, and for local (i.e., flywheel) oscillators used with absolute frequency standards such as laser-cooled atomic fountains and linear ion traps. These new devices are passive high-resolution frequency discriminators. Alone, they cannot function as superior atomic clocks; their effective operation depends on being integrated with an active local oscillator with excellent short term stability - such as that possible with the CHM.
Document ID
20020014431
Acquisition Source
Marshall Space Flight Center
Document Type
Contractor or Grantee Report
Authors
Walsworth, Ronald L.
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Mattison, Edward
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Vessot, Robert F. C.
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Date Acquired
September 7, 2013
Publication Date
December 1, 2001
Subject Category
Instrumentation And Photography
Funding Number(s)
CONTRACT_GRANT: NAG8-1434
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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