4.6 Article

Generation of 103.75 GHz CW Source With 5.10-16 Frequency Instability Using Cryogenic Sapphire Oscillators

Journal

IEEE MICROWAVE AND WIRELESS COMPONENTS LETTERS
Volume 22, Issue 2, Pages 85-87

Publisher

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/LMWC.2011.2181347

Keywords

ATACAMA; cryogenic sapphire oscillators (CSO); CW source; doubler; EHF; high-q; mm-wave; multiplication; oscillator; sapphire; SKA; stability; synthesis; very long baseline interferometry (VLBI)

Funding

  1. Australian Research Council [DP0878108, FL0992016]
  2. Australian Research Council [DP0878108] Funding Source: Australian Research Council

Ask authors/readers for more resources

We report the generation of millimeter wave signals with frequency instability of a few parts in 10(16). Such performance was achieved at 103.750 GHz by frequency multiplication of two nominally identical 12.969 GHz oscillators based on liquid helium cooled sapphire dielectric resonators. The multiplication stages were shown to only add a small amount of noise at averaging times less than 10 s, resulting in a minimum of frequency instability of 5 x 10(-16) at 20 s averaging time. Such ultra-stable signal sources operating at frequencies of 100 GHz are very important for many applications including high frequency radio astronomy.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available