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The Astronomical Low-Frequency ArrayAn array of satellites is proposed to make astronomic observations in the low frequency range of a few tens of MHz down to roughly 100 kHz, a range that cannot be observed through the ionosphere. The array would be in a solar orbit to avoid radio interference from Earth and to simplify trajectory tracking and control.
Document ID
20060037479
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Jones, D. L.
Allen, R. J.
Blume, W. H.
Desch, M. M.
Erickson, W. C.
Kaiser, M. L.
Kassim, N. E.
Kuiper, T. B. H.
Mahoney, M. J.
Marsh, K. A.
Michalski, R.
Oberto, R. E.
Perley, R. A.
Preston, R. A.
Stone, R. G.
Weiler, K. W.
Date Acquired
August 23, 2013
Publication Date
January 1, 1996
Distribution Limits
Public
Copyright
Other
Keywords
low-frequency array radio astronomy microsats

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