10 July 2014 Ideas for future large single dish radio telescopes
Author Affiliations +
Abstract
The existing large single dish radio telescopes of the 100m class (Effelsberg, Green Bank) were built in the 1970s and 1990s. With some active optics they work now down to 3 millimeter wavelength where the atmospheric quality of the site is also a limiting factor. Other smaller single dish telescopes (50m LMT Mexico, 30m IRAM Spain) are located higher and reach sub-millimeter quality, and the much smaller 12m antennas of the ALMA array reach at a very high site the Terahertz region. They use advanced technologies as carbon fiber structures and flexible body control.

We review natural limits to telescope design and use the examples of a number of telescopes for an overview of the available state-of-the-art in design, engineering and technologies. Without considering the scientific justification we then offer suggestions to realize ultimate performance of huge single dish telescopes (up to 160m). We provide an outlook on design options, technological frontiers and cost estimates.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hans J. Kärcher, Hans J. Kärcher, Jacob W. M. Baars, Jacob W. M. Baars, "Ideas for future large single dish radio telescopes", Proc. SPIE 9145, Ground-based and Airborne Telescopes V, 914503 (10 July 2014); doi: 10.1117/12.2055456; https://doi.org/10.1117/12.2055456
PROCEEDINGS
11 PAGES


SHARE
RELATED CONTENT

The design and analysis of 2m telescope’s K Mirror system
Proceedings of SPIE (September 01 2014)
Review of the refurbishment project for NSRT
Proceedings of SPIE (July 05 2018)
Challenges for QTT structure
Proceedings of SPIE (July 26 2016)
A dynamic thermal model for design and control of an...
Proceedings of SPIE (November 10 2011)
Next generation radio telescope of the 12 to 15...
Proceedings of SPIE (July 30 1998)

Back to Top