Mostrar el registro sencillo del ítem Balsley, B.B. Blamont, J. Forbes, J.M. Geller, M.A. Hirota, I. Vincent, R.A. Woodman Pollitt, Ronald Francisco 2016-11-08T05:15:14Z 2017-12-21T19:41:40Z 2016-11-08T05:15:14Z 2017-12-21T19:41:40Z 1983
dc.description p. 9-[13] es_ES
dc.description.abstract MSG-6 has been set up to study this on the basis that there is need to have observatories very close to the equator so that we may understand equatorial dynamics much more precisely than we do now. Such observatories, which are equipped with MST radars, lidar and other facilities, should be constructed and operated th rough international cooperation. Specific require­ments for the observation of equatorial middle atmosphere dynamics were discussed at the Workshop held 10-12 May 1982 at Estes Park, CO, USA, as will be shown in Section 2. MSG-6 has further worked on the problem, obtaining the opinions of each member as to the following questio ns: (1 ) locations of IEOs; (2) specification of the faciliti es at IEOs; and (3) finanical support on the construction and the maintenance of IEOs.The proposed locations for IEOs are, in alphabetical arder, Christmas Island, Galapagos Island, Kourous, Nauru and Tumbes (or Iquitos). es_ES
dc.format application/pdf es_ES
dc.language.iso eng es_ES
dc.publisher Instituto Geofísico del Perú es_ES
dc.rights info:eu-repo/semantics/openAccess es_ES
dc.rights.uri es_ES
dc.subject Observatories es_ES
dc.subject Dynamics es_ES
dc.subject Radar es_ES
dc.subject Upper atmosphere es_ES
dc.title Report of MSG-6 on the scientific aspects of an international equatorial observatory (IEO) es_ES
dc.type info:eu-repo/semantics/contributionToPeriodical es_ES
dc.subject.ocde es_ES




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