aLIGO PSL VCO Amplifier Front Panel

Document #:

LIGO-D1201424-v1

Document type:

D - Drawings

Abstract:

The low-noise VCO used to drive the frequency shifting acousto-optic modulator does not provide enough RF power to obtain maximum diffraction efficiency from the Isomet 1205C-843. A Mini-Circuits ZHL-1-2W-N+ amplifier is used to boost the VCO output power.

Files in Document:

• PDF file (D1201424-v1.pdf, file is not accessible)

Other Files:

• AutoCAD file, page 1 (D1201424s1.dwg, file is not accessible)
• AutoCAD file, page 2 (D1201424s2.dwg, file is not accessible)
• FrontPanel Express file (D1201424-v1.fpd, file is not accessible)

ICS/JIRA Record:

• ICS_LINK

Topics:

• Fabrication

Authors:

• Peter King

Keywords:

PSL VCO

Notes and Changes:

This is the front panel for the PSL VCO RF amplifier.

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