dc.contributor.author |
Agachev A. |
|
dc.contributor.author |
Balakin A. |
|
dc.contributor.author |
Buǐnov G. |
|
dc.contributor.author |
Buchinskaya S. |
|
dc.contributor.author |
Daishev R. |
|
dc.contributor.author |
Kisun'Ko G. |
|
dc.contributor.author |
Komissaruk V. |
|
dc.contributor.author |
Mavrin S. |
|
dc.contributor.author |
Murzakhanov Z. |
|
dc.contributor.author |
Rafikov R. |
|
dc.contributor.author |
Skochilov A. |
|
dc.contributor.author |
Cheredilin V. |
|
dc.contributor.author |
Chugunov Y. |
|
dc.date.accessioned |
2018-09-17T21:14:29Z |
|
dc.date.available |
2018-09-17T21:14:29Z |
|
dc.date.issued |
1998 |
|
dc.identifier.issn |
1063-7842 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/134719 |
|
dc.description.abstract |
Results of work on the assembly and adjustment of an original pentagonal, two-loop interferometer are reported; the interferometer is a passive version of a compact laser gravitational wave detector. It is shown that the correlative automatic noise-compensation system developed for the project is capable of lowering the phase noise level in the resultant signal channel of the detector by two orders of magnitude. © 1998 American Institute of Physics. |
|
dc.relation.ispartofseries |
Technical Physics |
|
dc.title |
Pentagonal two-loop ring interferometer |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
5 |
|
dc.relation.ispartofseries-volume |
43 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
591 |
|
dc.source.id |
SCOPUS10637842-1998-43-5-SID0040246466 |
|