The Large Millimeter Telescope (LMT) is a 50 m diameter radio telescope with an actively controlled segmented surface to be used for astronomy at millimeter wave lengths. The specifications call for a surface accuracy of 70 micrometers RMS and a pointing accuracy of 0.7 arcseconds RMS. This paper evaluates a proposed approach for computing and correcting in real time the surface deformations of the primary reflector and the pointing errors of the telescope due to thermal deformations using a finite element model and temperature measurements throughout the telescope structure
The Sardinia Radio Telescope (SRT), located near Cagliari (Italy), is the world’s second largest ful...
Temperature variations at very long baseline interferometry (VLBI) sites cause thermal deformations ...
Sardinia Radio Telescope (SRT) with its 64 m diameter primary mirror is a modern radio-astronomic fa...
We have developed a computational tool which serves to characterize the performance of large segment...
The techniques used to set and stabilise the surface of the IRAM 30 m radio telescope to a final roo...
Thermal performances of the Thirty Meter Telescope (TMT) structure were evaluated by finite element ...
This paper is a preprint of a paper accepted by IET Microwaves, Antennas and Propagation and is subj...
An engineering validation of a large optical telescope consists of executing major performing tests ...
The 64 m diameter Sardinia Radio Telescope (SRT), located near Cagliari (Italy), is the world’s seco...
The development of metrology instrumentation needed for realization of the active surface and precis...
Large ground-based telescopes are prone to perturbations caused by environmental factors that affect...
Large ground-based telescopes are prone to perturbations caused by environmental factors that affect...
The out-of-plane degrees of freedom (piston, tip, and tilt) of each of the 492 segments in the Thirt...
The Hartebeesthoek Radio Astronomy Observatory (HartRAO) of South Africa is currently developing a L...
Thermal modeling of the Thirty Meter Telescope (TMT) was conducted for evaluations of thermal perfor...
The Sardinia Radio Telescope (SRT), located near Cagliari (Italy), is the world’s second largest ful...
Temperature variations at very long baseline interferometry (VLBI) sites cause thermal deformations ...
Sardinia Radio Telescope (SRT) with its 64 m diameter primary mirror is a modern radio-astronomic fa...
We have developed a computational tool which serves to characterize the performance of large segment...
The techniques used to set and stabilise the surface of the IRAM 30 m radio telescope to a final roo...
Thermal performances of the Thirty Meter Telescope (TMT) structure were evaluated by finite element ...
This paper is a preprint of a paper accepted by IET Microwaves, Antennas and Propagation and is subj...
An engineering validation of a large optical telescope consists of executing major performing tests ...
The 64 m diameter Sardinia Radio Telescope (SRT), located near Cagliari (Italy), is the world’s seco...
The development of metrology instrumentation needed for realization of the active surface and precis...
Large ground-based telescopes are prone to perturbations caused by environmental factors that affect...
Large ground-based telescopes are prone to perturbations caused by environmental factors that affect...
The out-of-plane degrees of freedom (piston, tip, and tilt) of each of the 492 segments in the Thirt...
The Hartebeesthoek Radio Astronomy Observatory (HartRAO) of South Africa is currently developing a L...
Thermal modeling of the Thirty Meter Telescope (TMT) was conducted for evaluations of thermal perfor...
The Sardinia Radio Telescope (SRT), located near Cagliari (Italy), is the world’s second largest ful...
Temperature variations at very long baseline interferometry (VLBI) sites cause thermal deformations ...
Sardinia Radio Telescope (SRT) with its 64 m diameter primary mirror is a modern radio-astronomic fa...