JPL Technical Report Server

Full-Sky Imaging at Low Frequencies

Show simple item record Jones, D. L. en_US Marsh, K. en_US Mahoney, M. en_US Kuiper, T. en_US Linfield, R. en_US Preston, R. en_US Unwin, S. en_US Shepherd, M. en_US Erickson, W. en_US Weiler, K. en_US 2004-10-04T20:00:41Z 2004-10-04T20:00:41Z 1996-01 en_US
dc.identifier.citation American Astronomical Society en_US
dc.identifier.citation San Antonio, TX en_US
dc.identifier.clearanceno 95-1400
dc.description.abstract Exploring the frequency range from a few tens of MHZ down to a few tens of kHz commonly requires multiple antennas operating as an aperture synthesis interferometer to obtain angular resolution. This design must overcome the corrupting effects of interplanetary scintillation, interfering signals and nearly isotropic antennas that see strong sources such as the Sun and Jupiter at all times. en_US
dc.format.extent 29826 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.title Full-Sky Imaging at Low Frequencies en_US

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