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dc.contributor.author Woodman Pollitt, Ronald Francisco
dc.date.accessioned 2018-07-04T16:49:10Z
dc.date.available 2018-07-04T16:49:10Z
dc.date.issued 1983-01
dc.identifier.issn 0252-9769
dc.identifier.uri http://repositorio.igp.gob.pe/handle/IGP/1695
dc.description En: Revista Geofísica, n. 18/19, p. 31-38. es_ES
dc.description.abstract "We shall limit ourselves here to a brief discussion of the work done at the Jicamarca Observatory connected either with: a) the geometry of the Magnetic Field or, b) with backscatter from en­hanced fluctuations (non-thermal) produced either by turbulence or by plasma instabilities. Although equally important, work related to the usual ionospheric parameters obtained with in­coherent scatter techniques, like electron densi­ties, temperature, ion composition etc., is not treated here; since our main intention is to under­line what is unique to the Jicamarca Observatory..." 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/restrictedAccess es_ES
dc.rights.uri info:eu-repo/semantics/restrictedAccess es_ES
dc.source Repositorio institucional - IGP es_ES
dc.subject Campos magnéticos es_ES
dc.subject Inestabilidades del plasma es_ES
dc.subject Turbulencia es_ES
dc.subject Radar es_ES
dc.subject Ionósfera--Investigación--Perú es_ES
dc.subject Radar--Perú--Mediciones es_ES
dc.subject Radar de dispersión incoherente es_ES
dc.title Scientific contributions of the Jicamarca Observatory peculiar to its equatorial latitude of operating frequency es_ES
dc.type info:eu-repo/semantics/article es_ES
dc.subject.ocde Radar es_ES
dc.subject.ocde Investigación científica es_ES
dc.subject.ocde Perú es_ES
dc.subject.ocde Atmósfera es_ES
dc.identifier.journal Revista Geofísica es_ES

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