TY - GEN
T1 - The hardware control system for WEAVE at the William Herschel Telescope
AU - Delgado, Jose Miguel
AU - Menéndez Mendoza, Saúl
AU - Burgal, Jose Alonso
AU - Herreros, Jose Miguel
AU - Picó, Sergio
AU - Abrams, Don Carlos
AU - Martin, Carlos
AU - Cano, Diego
AU - Gribbin, F. J.
AU - Skvarč, Jure
AU - Dee, Kevin
AU - Lhome, Emilie
AU - Dalton, Gavin
AU - Middleton, Kevin
AU - Trager, Scott
AU - L. Aguerri, J. Alfonso
AU - Bonifacio, Piercarlo
AU - Vallenari, Antonella
AU - Carrasco, Esperanza
PY - 2018/7/6
Y1 - 2018/7/6
N2 - When an alt-azimuth telescope is tracking at a specific field, it is
necessary to use a de-rotator system to compensate the Earth's rotation
of the field of view. In order, to keep the telescope tracking the field
of view selected, the instrument will need to a rotation system for
compensating it [1]. The new WEAVE [2] two degrees field of view
requires a new field de-rotator on the top-end of the telescope. The
rotator system has been designed with a direct drive motor which
eliminates the need for mechanical transmission elements such as
gearboxes, speed reducers, and worm gear drives. This design is a huge
advantage for the system performance and lifetime because it eliminates
undesirable characteristics such as long-time drift, elasticity, and
backlash. The hardware control system has been developed with a Rockwell
servo-drive and controller. The rotator has to be controlled by the
high-level software which is also responsible for the telescope control.
This paper summarizes the model developed for simulating and the
software which will be used to accept the rotator system. A performance
study is also carried out to test the CIP (Common Industrial Protocol)
for communications between the high-level software and the rotator
hardware.
AB - When an alt-azimuth telescope is tracking at a specific field, it is
necessary to use a de-rotator system to compensate the Earth's rotation
of the field of view. In order, to keep the telescope tracking the field
of view selected, the instrument will need to a rotation system for
compensating it [1]. The new WEAVE [2] two degrees field of view
requires a new field de-rotator on the top-end of the telescope. The
rotator system has been designed with a direct drive motor which
eliminates the need for mechanical transmission elements such as
gearboxes, speed reducers, and worm gear drives. This design is a huge
advantage for the system performance and lifetime because it eliminates
undesirable characteristics such as long-time drift, elasticity, and
backlash. The hardware control system has been developed with a Rockwell
servo-drive and controller. The rotator has to be controlled by the
high-level software which is also responsible for the telescope control.
This paper summarizes the model developed for simulating and the
software which will be used to accept the rotator system. A performance
study is also carried out to test the CIP (Common Industrial Protocol)
for communications between the high-level software and the rotator
hardware.
U2 - 10.1117/12.2313238
DO - 10.1117/12.2313238
M3 - Conference contribution
T3 - Proceedings of the SPIE
SP - 1070033
BT - Proceedings Volume 10700
PB - SPIE.Digital Library
T2 - SPIE Astronomical Telescopes + Instrumentation, 2018
Y2 - 10 June 2018 through 15 June 2018
ER -