Differences between revisions 2 and 12 (spanning 10 versions)
⇤ ← Revision 2 as of 2009-12-30 05:30:00 →
Size: 498
Editor: RanaAdhikari
Comment:
← Revision 12 as of 2013-02-23 03:55:47 → ⇥
Size: 1640
Editor: RanaadhikariATligoDOTorg
Comment:
Deletions are marked like this. Additions are marked like this.
Line 1: Line 1:
== This page is obsolete. We should copy Rich's Transmon QPD design. ==
[[https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=13998 | https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=13998]]
----
Line 8: Line 12:
The basic idea is to make an updated version of Jay's circuit ([[http://www.ligo.caltech.edu/%7Ejay/drawings/d980325-c1.pdf|D980325-C1]]):
 1. Use voltage regulators. Is there something better than the 7915/7815 ?
 1. Maybe use a different op-amp. The OP497 in Jay's circuit is a good part, but not modern. We want to use something that's not going obsolete soon.
 1. Use metal film resistors.
 1. Allow for whitening in the head via some jumpers. Possibly also give slow DC ouputs.
Line 9: Line 18:
----
=== Choice of Quadrant Photodiode ===
The QD50 and QD100 are commonly used in LIGO for DCPDs. They are Silicon based and have active areas of 50 mm^2^ and 100 mm^2^, respectively. R = 0.5 A/W @ 900 nm.
Line 10: Line 22:
=== Noise ===
This is the input referred current noise calculated with LISO - OP497 w/ a 100k transimpedance resistor:<<BR>>
{{attachment:qpd-op497.png}}

Next, we look at the noise using the XXNNN quad opamp:
Line 13: Line 30:
 1. Application note attachment:AN_940.pdf on selection of low noise opamps.  1. Application note [[attachment:AN_940.pdf]] on selection of low noise opamps.

This page is obsolete. We should copy Rich's Transmon QPD design.

https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=13998

This page describes the design of a new quadrant photodetector.

The main applications are for DC beam sensing and optical lever servos. These are non-critical applications.

The DC beam sensing ones are mainly for beams on the PSL and IO optics. We should also add a QPD to each of the ISC readout paths.

The basic idea is to make an updated version of Jay's circuit (D980325-C1):

  1. Use voltage regulators. Is there something better than the 7915/7815 ?
  2. Maybe use a different op-amp. The OP497 in Jay's circuit is a good part, but not modern. We want to use something that's not going obsolete soon.
  3. Use metal film resistors.
  4. Allow for whitening in the head via some jumpers. Possibly also give slow DC ouputs.

Choice of Quadrant Photodiode

The QD50 and QD100 are commonly used in LIGO for DCPDs. They are Silicon based and have active areas of 50 mm2 and 100 mm2, respectively. R = 0.5 A/W @ 900 nm.

Noise

This is the input referred current noise calculated with LISO - OP497 w/ a 100k transimpedance resistor:
qpd-op497.png

Next, we look at the noise using the XXNNN quad opamp:

  1. Application note AN_940.pdf on selection of low noise opamps.

Electronics/QuadrantPhotodetectorDesign (last edited 2013-02-23 03:55:47 by RanaadhikariATligoDOTorg)