LIGO Contamination Control Plan
- Document #:
- LIGO-E0900047-v1
- Document type:
- E - Engineering documents
Other Versions:
| LIGO-E0900047-v23
17 Sep 2020, 06:57 |
| LIGO-E0900047-v22
27 Mar 2014, 11:12 |
| LIGO-E0900047-v21
01 Nov 2013, 12:22 |
| LIGO-E0900047-v13
06 Sep 2011, 18:09 |
| LIGO-E0900047-v12
13 Jul 2011, 10:45 |
| LIGO-E0900047-v11
10 Mar 2011, 11:17 |
| LIGO-E0900047-v9
14 Jun 2010, 10:45 |
| LIGO-E0900047-v8
25 Mar 2010, 08:40 |
| LIGO-E0900047-v7
23 Nov 2009, 15:32 |
| LIGO-E0900047-v6
21 Oct 2009, 10:38 |
| LIGO-E0900047-v5
15 Oct 2009, 14:50 |
| LIGO-E0900047-v4
18 Aug 2009, 09:50 |
| LIGO-E0900047-v2
07 Jul 2009, 14:13 |
| LIGO-E0900047-x0
20 Feb 2009, 14:38 |
- Abstract:
- The LIGO interferometers are extremely sensitive to optical scattering or absorption losses induced by both particulate and hydrocarbon contamination. In order to minimize the likelihood of contamination of optical surfaces, numerous operational practices have been implemented at the LIGO Observatories. The purpose of this document is to describe the operational practices that have been implemented so that it can serve as a reference for observatory staff and visitors.
- Files in Document:
-
- E0900047-v1.pdf (file is not accessible)
- Other Files:
- E0900047_v1.doc (file is not accessible)
- Topics:
- Authors:
- Keywords:
- contamination particulates hydrocarbon