Показать сокращенную информацию
dc.contributor.author | Karpov S. | |
dc.contributor.author | Beskin G. | |
dc.contributor.author | Bondar S. | |
dc.contributor.author | Perkov A. | |
dc.contributor.author | Ivanov E. | |
dc.contributor.author | Guarnieri A. | |
dc.contributor.author | Bartolini C. | |
dc.contributor.author | Greco G. | |
dc.contributor.author | Shearer A. | |
dc.contributor.author | Sasyuk V. | |
dc.date.accessioned | 2018-09-18T20:24:09Z | |
dc.date.available | 2018-09-18T20:24:09Z | |
dc.date.issued | 2013 | |
dc.identifier.issn | 1633-4760 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/139509 | |
dc.description.abstract | Here we briefly summarize our long period experience of constructing and operating wide-field monitoring cameras with sub-second temporal resolution to look for optical components of GRBs, fast-moving satellites and meteors. General requirements for hardware for such systems are discussed along with algorithms of real-time detection and classification of various kinds of short optical transients. We also give a status report on the next generation, multi-objective and transforming monitoring system, the MegaTORTORA, whose 6-channel (Mini-MegaTORTORA-Spain) and 9-channel prototypes (Mini-MegaTORTORA-Kazan) we are building now at SAO RAS. This system combines a wide field of view with subsecond temporal resolution in monitoring regime, and is able to reconfigure itself, in a fractions of second, to follow-up mode which has better sensitivity and provides us with multi-color and polarimetric information on detected transients simultaneously. © EAS, EDP Sciences 2013. | |
dc.relation.ispartofseries | EAS Publications Series | |
dc.title | Status and perspectives of Mini-MegaTORTORA wide-field monitoring system with high temporal resolution | |
dc.type | Conference Paper | |
dc.relation.ispartofseries-volume | 61 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 465 | |
dc.source.id | SCOPUS16334760-2013-61-SID84887096573 |