Показать сокращенную информацию
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 |