7/6/2023 0 Comments Square kilometre array![]() ![]() ![]() Further information on the project can be found at. This Special Issue of Experimental Astronomy provides a snapshot of SKA engineering act- ity around the world, and is based on presentations made at the SKA meeting in Penticton,BC,CanadainJuly2004.Topicscoveredincludeantennaconcepts,so- ware, signal transport and processing, radio frequency interference mitigation, and reports on related technologies in other radio telescopes now under construction. TheSKAProjectcurrentlyinvolves45institutesin17countries,manyofwhich are involved in nationally- or regionally-funded state-of-the-art technical devel- ments being pursued ahead of the 2009 selection of design concept. The Square Kilometre Array Observatory (SKAO) became an intergovernmental organisation in February 2021. The cost is estimated to be about 1000 M. The current schedule for the SKA foresees a decision on the SKA site in 2006, a decisiononthedesignconceptin2009,constructionofthe?rstphase(international path?nder)from2010to2013,andconstructionofthefullarrayfrom2014to2020. The SKA will provide a great leap in sensitivity, resolution and survey speed compared to existing radio telescope, enabling it to revolutionise our understanding of the universe. The SKA will complement major ground- and space-based astronomical facilities under construction or planned in other parts of the electromagnetic spectrum (e.g. The Square Kilometre Array (SKA) is an international endeavour to build the world's largest and most sensitive radio telescope. These capabilities will ensure the SKA will play a leading role in solving the major astrophysical and cosmological questions of the day (see the science case at astronom.htm). The Square Kilometre Array (SKA) observatory is a next-generation radio astronomy facility, which is just started its construction, after successful. The Square Kilometre Array (SKA) Project is a global project to design and c- struct a revolutionary new radio telescope with of order 1 million square meters of collecting area in the wavelength range from3mto1cm.It will have two - ders of magnitude greater sensitivity than current telescopes and an unprecedented large instantaneous ?eld-of-view. ![]()
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