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The Arecibo Observatory as an MST radarThe radars and other systems at the Arecibo Observatory were designed and built, originally, for incoherent-scatter and radio-astronomy research. More recently, important additions have been made for planetary radar and artificial RF heating of the ionosphere. Although designed and built for a different application, these systems have shown to be very powerful tools for tropospheric, stratospheric and mesospheric research. The Observatory at present has two main radars: one at 430 and the other at 2380 MHz. In addition, 50-MHz MST radar work has been done using portable transmitters brought to the Observatory for this purpose. This capability will become permanent with the recent acquisition of a transmitter at this frequency. Furthermore, control and data processing systems have been developed to use the powerful HF transmitter and antennas of the HF-heating facility as an HF bistatic radar. A brief description of the four radars available at the Observatory is presented.
Document ID
19840019070
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Woodman, R. F.
(Instituto Geofisico del Peru Lima, Peru)
Date Acquired
August 12, 2013
Publication Date
December 1, 1983
Publication Information
Publication: Intern. Council Sci. Unions Middle Atmosphere Program, Vol. 9
Subject Category
Communications And Radar
Accession Number
84N27138
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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