JPL Technical Report Server

Full-Sky Imaging at Low Frequencies

Show simple item record

dc.contributor.author Jones, D. L. en_US
dc.contributor.author Marsh, K. en_US
dc.contributor.author Mahoney, M. en_US
dc.contributor.author Kuiper, T. en_US
dc.contributor.author Linfield, R. en_US
dc.contributor.author Preston, R. en_US
dc.contributor.author Unwin, S. en_US
dc.contributor.author Shepherd, M. en_US
dc.contributor.author Erickson, W. en_US
dc.contributor.author Weiler, K. en_US
dc.date.accessioned 2004-10-04T20:00:41Z
dc.date.available 2004-10-04T20:00:41Z
dc.date.issued 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.identifier.uri http://hdl.handle.net/2014/31951
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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account