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Active Adaptive Arrays: The ASTRON Approach to SKA

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Abstract

It has been argued, for a number of reasons, that the next generation radio telescope should be a multi-element interferometer with a collecting area of about 1 km2. The remaining parameters of such an instrument – frequency range, angular resolution, instantaneous bandwidth, etc. – will be science driven. The requirements for propagation studies are briefly discussed, and it is pointed out how variable-source confusion may differ from the normal variety. Finally, the Dutch project to achieve a large collecting area using adaptive arrays of active antennas is described. A systematic approach has been adopted, with the construction of arrays of increasing complexity to test design features at each state. Recently, development of a low frequency array (LOFAR) has become an additional option. It would facilitate tests of some of the larger instrument's features, and provide real data on the influence of the ionosphere and interfering sources.

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References

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Authors and Affiliations

  1. ASTRON, P.O. Box 2, 7990 AA, Dwingeloo, Netherlands

    Richard G. Strom, Bart Smolders & Arnold van Ardenne

  2. Astronomical Institute `Anton Pannekoek', University of Amsterdam, Netherlands

    Richard G. Strom

Authors
  1. Richard G. Strom
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  2. Bart Smolders
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  3. Arnold van Ardenne
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Strom, R.G., Smolders, B. & van Ardenne, A. Active Adaptive Arrays: The ASTRON Approach to SKA. Astrophysics and Space Science 278, 209–212 (2001). https://doi.org/10.1023/A:1013123215943

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  • DOI: https://doi.org/10.1023/A:1013123215943

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