The impact of the proposed Arecibo Observatory upgrade on middle atmosphere research

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dc.contributor.authorWoodman Pollitt, Ronald Francisco
dc.date.accessioned2016-11-07T22:44:03Z
dc.date.accessioned2017-12-21T19:41:42Z
dc.date.available2016-11-07T22:44:03Z
dc.date.available2017-12-21T19:41:42Z
dc.date.issued1986
dc.description.abstractThere are at present three radar frequencies that are being ex­ploited: 50, 430 and 2380 MHz. (In addition, there is a range of HF frequencies in a bi-static mode, using the Heating Facility to illuminate, but which we will not discuss here, since there would be no benefits to be derived from the upgrading.) The proposed upgrading of the Arecibo 300 meter antenna will benefit the research work in the three regions of the atmosphere we have mentioned above through improved performance in the three existing radars, including multifrequency operation.
dc.formatapplication/pdf
dc.identifier.citationWoodman, R. F. (1986). The impact of the proposed Arecibo Observatory upgrade on middle atmosphere research.==$Proceedings of the Arecibo Upgrading Workshop,$==Cornell University, Ithaca, New York, 263-275.
dc.identifier.urihttp://hdl.handle.net/20.500.12816/547
dc.language.isoeng
dc.publisherCornell University
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttps://creativecommons.org/licences/by/4.0/
dc.subjectResearch
dc.subjectHigh atmosphere
dc.subjectRadar
dc.subjectArecibo Ionospheric Observatory
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01
dc.titleThe impact of the proposed Arecibo Observatory upgrade on middle atmosphere research
dc.typeinfo:eu-repo/semantics/conferenceObject

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