Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2671
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dc.contributor.authorJones, D.L.-
dc.contributor.authorDwarakanath, K.S.-
dc.contributor.author+28 Co-authors-
dc.date.accessioned2007-06-11T06:37:54Z-
dc.date.available2007-06-11T06:37:54Z-
dc.date.issued2000-04-
dc.identifier.citationAstrophysical Phenomena Revealed by Space VLBI, Proceedings of the VSOP Symposium, held at the Institute of Space and astronautical Science, Sagamihara, Kanagawa, Japan, January 19 - 21, 2000, Eds.: H. Hirabayashi, P.G. Edwards, and D.W. Murphy, Published by the Institute of Space and Astronautical Science, 2000, p265-268en
dc.identifier.urihttp://hdl.handle.net/2289/2671-
dc.descriptionRestricted Access.en
dc.description.abstractAt sufficiently low frequencies, no ground-based radio array will be able to produce high resolution images while looking through the ionosphere. A space-based array will be needed to explore the objects and processes which dominate the sky at the lowest radio frequencies. An imaging radio interferometer based on a large number of small, inexpensive satellites would be able to track solar radio bursts associated with coronal mass ejections out to the distance of Earth, determine the frequency and duration of early epochs of nonthermal activity in galaxies, and provide unique information about the interstellar medium. This would be a ``space-space" VLBI mission, as only baselines between satellites would be used. Angular resolution would be limited only by interstellar and interplanetary scattering.en
dc.format.extent167604 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherInstitute of Space and Astronautical Scienceen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2000aprs.conf..265Jen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0003120en
dc.rights2000 Institute of Space and Astronautical Scienceen
dc.titleSpace VLBI at low frequenciesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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