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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2479
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dc.contributor.authorJones, D.L.-
dc.contributor.authorDwarakanath, K.S.-
dc.date.accessioned2007-05-25T11:21:08Z-
dc.date.available2007-05-25T11:21:08Z-
dc.date.issued2000-
dc.identifier.citationGeophysical Monograph Series, 2000, Vol.119, p339-349en
dc.identifier.urihttp://hdl.handle.net/2289/2479-
dc.descriptionRestricted Access. Radio Astronomy at Long Wavelengths, Geophysical Monograph Series, Vol. 119, Eds. R. G. Stone, K. W. Weiler, M. L. Goldstein, and J.-L. Bougeret (American Geophysical Union, Washington, DC), 2000.en
dc.description.abstractA radio interferometer array in space providing high dynamic range images with unprecedented angular resolution over the broad frequency range from 0.03 - 30 MHz will open new vistas in solar, terrestrial, galactic, and extragalactic astrophysics. The ALFA interferometer will image and track transient disturbances in the solar corona and interplanetary medium - a new capability which is crucial for understanding many aspects of solar-terrestrial interaction and space weather. ALFA will also produce the first sensitive, high-angular-resolution radio surveys of the entire sky at low frequencies. The radio sky will look entirely different below about 30 MHz. As a result, ALFA will provide a fundamentally new view of the universe and an extraordinarily large and varied science return.en
dc.format.extent738124 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Geophysical Unionen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2000ralw.conf..339Jen
dc.rights2000 American Geophysical Unionen
dc.subjectRADIO ASTRONOMYen
dc.subjectLONG WAVELENGTHen
dc.subjectLOW FREQENCYen
dc.titleThe astronomical low frequency array: A proposed explorer mission for radio astronomyen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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