![]() 2005 IEEE International Conference on Acoustics, Speech, and Signal Processing March 18-23, 2005 • Pennsylvania Convention Center/Marriott Hotel • Philadelphia, PA, USA |
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ICASSP |
Towards a New Generation of Radio Astronomical Instruments: Signal processing for large distributed arraysOrganizers: Alle-Jan van der Veen, Delft University of Technology; Albert-Jan Boonstra, ASTRONRadio astronomy forms an interesting application area for array signal processing techniques. Technological advances in the last decade have created possibilities for large distributed interferometric radio telescopes with very large receiving areas and a sensitivity which is one to two orders of magnitude better than the current generation. Increased sensitivity implies receiving more interfering signals, and therefore RFI detection and removal is now an important topic in radio astronomy. Fortunately, massive phased array technology will also provide increased flexibility to filter out interference. International efforts for this new generation are coordinated under the framework of the Square Kilometer Array programme (SKA), http://www.skatelescope.org, with a target commissioning date of around 2012. Another example of a distributed phased array radio telescope will be the Low Frequency Array (LOFAR) which is currently under construction in The Netherlands (http://www.lofar.org), and slated for 2006–2008. Prior to this, the international Atacama Large Millimeter/Submillimeter Array, or ALMA, will be constructed in a desert in Chile. The talks in the session cover the following topics:
Overview lecture: Regular lectures:
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