IMPLEMENTATION OF THE $\alpha$ UMI MONITORING SYSTEM AT SAO RAS
Section: ASTRONOMICAL INSTRUMENTS AND METHODS
Authors:
1.
Special Astrophysical Observatory of the Russian Academy of Sciences
2.
Special Astrophysical Observatory of the Russian Academy of Sciences
3.
Special Astrophysical Observatory of the Russian Academy of Sciences
4.
Special Astrophysical Observatory of the Russian Academy of Sciences
Type:
Сonference article
Published:
27.12.2024
Subject area:
UDC 52
UDC 53
UDC 520
UDC 521
UDC 523
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAK SCI004000 Astronomy
BISAK SCI005000 Physics / Astrophysics
UDC 53
UDC 520
UDC 521
UDC 523
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAK SCI004000 Astronomy
BISAK SCI005000 Physics / Astrophysics
Language:
English
Keywords:
methods: observational; techniques: image processing
Abstract (English):
A new $\alpha$ UMi monitoring system based on an IP camera with a CMOS photodetector has been developed and installed at the Upper Scientific Site of the Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS). The main aim of the development is to measure the astronomical seeing and monitor its variation. Here we briefly describe the method of differential image motion monitoring (DIMM) used as the device operational principle and give some details on the characteristics and operation of the monitoring system developed.
A new $\alpha$ UMi monitoring system based on an IP camera with a CMOS photodetector has been developed and installed at the Upper Scientific Site of the Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS). The main aim of the development is to measure the astronomical seeing and monitor its variation. Here we briefly describe the method of differential image motion monitoring (DIMM) used as the device operational principle and give some details on the characteristics and operation of the monitoring system developed.
Keywords:
methods: observational; techniques: image processing
methods: observational; techniques: image processing
1. Sarazin M. and Roddier F., 1990, Astronomy and Astrophysics, 227, p. 294
2. Shaldyrvan I.V., Komarov V.V., Fokin M.Y., 2023, Izvestiya Krymskoj Astrofizicheskoj Observatorii, 119, p. 12
3. Tokovinin A., 2002, Publications of the Astronomical Society of the Pacific, 114, p. 1156
