Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-22T07:37:08.093Z Has data issue: false hasContentIssue false

Low-cost dichroic mirrors for future Deep Space ground stations

Published online by Cambridge University Press:  06 October 2011

Marco Pasian*
Affiliation:
Department of Electronics, University of Pavia, Via Ferrata 1, 27100 Pavia, Italy. Phone: +39 0328 985223.
Maurizio Bozzi
Affiliation:
Department of Electronics, University of Pavia, Via Ferrata 1, 27100 Pavia, Italy. Phone: +39 0328 985223.
Luca Perregrini
Affiliation:
Department of Electronics, University of Pavia, Via Ferrata 1, 27100 Pavia, Italy. Phone: +39 0328 985223.
*
Corresponding author: M. Pasian Email: [email protected]

Abstract

Future Deep Space (DS) ground stations envisioned by running projects funded by major space agencies are based on arrays of reflector antennas operating in different frequency bands. Therefore, a multi-band feeding system is required for each antenna, and a possible solution foresees the use of dichroic mirrors to separate/combine different beams. This paper presents a low-cost and fast manufacturing process for the fabrication of dichroic mirrors, usually referred to as punching technique or metal stamping. In particular, the specific advantages and limits of this fabrication technique are outlined and discussed, showing both electrical performance and manufacturing accuracy measurements from a test prototype. In addition, a typical scenario for future DS ground stations is described, showing the impact of these low-cost dichroic mirrors on the final ground station performance and cost, compared to the standard approach for dichroic mirror manufacturing based on more expensive and time-consuming technologies (e.g. milling machining).

Type
Industrial and Engineering Papers
Copyright
Copyright © Cambridge University Press and the European Microwave Association 2011

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

[1]Vassallo, E. et al. : The European space agency's deep-space antennas. Proc. IEEE, 95 (11) (2007), 21112131.CrossRefGoogle Scholar
[2]Imbriale, W.A.: Large Antennas of the Deep Space Network, John Wiley & Sons, Inc., Hoboken, NJ, USA, 2003.Google Scholar
[3]Rawson, S. et al. : Future architectures for ESA deep space ground stations, in 5th ESA Int. Workshop on TT&C for Space Application, ESA/ESTEC, The Netherlands, September 2010.Google Scholar
[5]Allen Telescope Array official website: http://www.seti.org/ataGoogle Scholar
[6]Munk, B.A.: Frequency Selective Surfaces: Theory and Design, John Wiley & Sons, Inc., USA, 2000.CrossRefGoogle Scholar
[7]Besso, P.; Bozzi, M.; Perregrini, L.; Drioli, L.S.; Nickerson, W.: Deep space antenna for rosetta mission: design and testing of the S/X-band dichroic mirror. IEEE Trans. Antennas Propag., 51 (3) (2003), 388394.CrossRefGoogle Scholar
[8]Besso, P.; Bozzi, M.; Formaggi, M.; Pasian, M.; Perregrini, L.: Design of K-band inductive dichroic mirrors for upgrading ESA deep-space antenna DSA2, in 37th European Microwave Conf. 2007, Munich, Germany, October 8–12, 2007.Google Scholar
[9]Bozzi, M.; Perregrini, L.; Weinzierl, J.; Winnewisser, C.: Efficient analysis of quasi-optical filters by a hybrid MoM/BI-RME method. IEEE Trans. Antennas Propag., 49 (7) (2001), 10541064.CrossRefGoogle Scholar
[10]Kitsuregawa, T.: Advanced Technology in Satellite Communication Antennas: Electrical & Mechanical Design, Artech House, Inc., Boston, MA, U.S.A., 1990.Google Scholar
[11]Ticra GRASP9, official website: www.ticra.comGoogle Scholar