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= Prototype model =
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 * Designed by Y. Enomoto (2018), inspired by LIGO low noise VCOs. [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=8968| JGW-D1808968]]

=== Frequency Noise ===
 * Worse than the specification for the non-divided phase noise ([[http://klog.icrr.u-tokyo.ac.jp/osl/?r=7425|klog 7425]]).
 . {{attachment:7425_20181218132925_lnvcopn2.png|Measured freq. noise (klog 7425) | width=400}}

=== Tuning Range ===


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 . Designed by Y. Enomoto (2018), inspired by LIGO low noise VCOs.

 . [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=8968| Prototype VCO JGW-D1808968]]

= Production model =
 . Sophisticated version of the endeavour model.
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 . Sophisticated version of the prototype model.

Low Noise VCOs

Descriptions

Low phase noise, a center frequency of 70 MHz, actuation range of several 100 kHz, aaa dBm output


Prototype model


  • Designed by Y. Enomoto (2018), inspired by LIGO low noise VCOs. JGW-D1808968

Frequency Noise

  • Worse than the specification for the non-divided phase noise (klog 7425).

  • Measured freq. noise (klog 7425)

Tuning Range


Endeavour model


  • Sophisticated version of the prototype model.

Bill of Materials

KAGRA/Subgroups/MIF/AEL/LowNoiseVCOs (last edited 2019-11-12 11:32:54 by KiwamuIzumi)