Differences between revisions 10 and 11
⇤ ← Revision 10 as of 2019-07-17 15:09:21 →
Size: 551
Editor: KiwamuIzumi
Comment:
← Revision 11 as of 2019-07-17 15:10:07 → ⇥
Size: 531
Editor: KiwamuIzumi
Comment:
Deletions are marked like this. Additions are marked like this.
Line 7: Line 7:
 . 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]]		  * 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]]

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

  • Measured freq. noise (klog 6552)

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)