The SCORPIO-2 Focal Reducer Control System
Transactions of IAA RAS, issue 53, 44–53 (2020)
DOI: 10.32876/ApplAstron.53.44-53
Keywords: instrumentation, observational tools, control systems
About the paper Full textAbstract
There is often need to quickly change the telescope instrumentation during astrophysical observations, for instance it is a switchover from photometry to spectroscopy. Multimode devices with a changeable optical scheme allow switching between different observational methods with a minimal time loss. A properly constructed and automated control system plays an important role here. In this paper, we review the control system of SCORPIO-2 multimode focal reducer operating in the primary focus of the 6-m SAO RAS telescope. The typical architecture of the system allowing remote observations is presented. We summarize the principles of the focal reducer hardware level operation, the detailed design of a unit with phase-rotating elements for high-precision polarimetric measurements is considered. Some design features of the focal reducer and its individual units control scheme implemented on microprocessors are presented. The observational complex included 'SCORPIO-2 + calibration and guiding adapter + detector + telescope' is controlled by a compact computer built into the focal reducer body. The software package written on IDL to make remote control of the observational complex is briefly described. We show one of the possibilities to create a distributed system allowing remote observations from a single point using different instruments: multimode focal reducer, calibration and off-axis guiding unit, image acquisition system, observational data archiving system and telescope. The focal reducer control system allows collecting all the device elements into a single block, minimizing internal and external connections. Quick switching between different methods provides flexibility of observational programs choice for the current state of the atmosphere, thereby saving observation time.
Citation
A. E. Perepelitsyn, V. R. Amirkhanyan, A. V. Moiseev. The SCORPIO-2 Focal Reducer Control System // Transactions of IAA RAS. — 2020. — Issue 53. — P. 44–53.
@article{perepelitsyn2020,
abstract = {There is often need to quickly change the telescope instrumentation during astrophysical observations, for instance it is a switchover from photometry to spectroscopy. Multimode devices with a changeable optical scheme allow switching between different observational methods with a minimal time loss. A properly constructed and automated control system plays an important role here. In this paper, we review the control system of SCORPIO-2 multimode focal reducer operating in the primary focus of the 6-m SAO RAS telescope.
The typical architecture of the system allowing remote observations is presented. We summarize the principles of the focal reducer hardware level operation, the detailed design of a unit with phase-rotating elements for high-precision polarimetric measurements is considered. Some design features of the focal reducer and its individual units control scheme implemented on microprocessors are presented. The observational complex included 'SCORPIO-2 + calibration and guiding adapter + detector + telescope' is controlled by a compact computer built into the focal reducer body. The software package written on IDL to make remote control of the observational complex is briefly described.
We show one of the possibilities to create a distributed system allowing remote observations from a single point using different instruments: multimode focal reducer, calibration and off-axis guiding unit, image acquisition system, observational data archiving system and telescope. The focal reducer control system allows collecting all the device elements into a single block, minimizing internal and external connections. Quick switching between different methods provides flexibility of observational programs choice for the current state of the atmosphere, thereby saving observation time.},
author = {A.~E. Perepelitsyn and V.~R. Amirkhanyan and A.~V. Moiseev},
doi = {10.32876/ApplAstron.53.44-53},
issue = {53},
journal = {Transactions of IAA RAS},
keyword = {instrumentation, observational tools, control systems},
pages = {44--53},
title = {The SCORPIO-2 Focal Reducer Control System},
url = {http://iaaras.ru/en/library/paper/2049/},
year = {2020}
}
TY - JOUR
TI - The SCORPIO-2 Focal Reducer Control System
AU - Perepelitsyn, A. E.
AU - Amirkhanyan, V. R.
AU - Moiseev, A. V.
PY - 2020
T2 - Transactions of IAA RAS
IS - 53
SP - 44
AB - There is often need to quickly change the telescope instrumentation
during astrophysical observations, for instance it is a switchover
from photometry to spectroscopy. Multimode devices with a changeable
optical scheme allow switching between different observational
methods with a minimal time loss. A properly constructed and
automated control system plays an important role here. In this paper,
we review the control system of SCORPIO-2 multimode focal reducer
operating in the primary focus of the 6-m SAO RAS telescope. The
typical architecture of the system allowing remote observations is
presented. We summarize the principles of the focal reducer hardware
level operation, the detailed design of a unit with phase-rotating
elements for high-precision polarimetric measurements is considered.
Some design features of the focal reducer and its individual units
control scheme implemented on microprocessors are presented. The
observational complex included 'SCORPIO-2 + calibration and guiding
adapter + detector + telescope' is controlled by a compact computer
built into the focal reducer body. The software package written on
IDL to make remote control of the observational complex is briefly
described. We show one of the possibilities to create a distributed
system allowing remote observations from a single point using
different instruments: multimode focal reducer, calibration and off-
axis guiding unit, image acquisition system, observational data
archiving system and telescope. The focal reducer control system
allows collecting all the device elements into a single block,
minimizing internal and external connections. Quick switching between
different methods provides flexibility of observational programs
choice for the current state of the atmosphere, thereby saving
observation time.
DO - 10.32876/ApplAstron.53.44-53
UR - http://iaaras.ru/en/library/paper/2049/
ER -