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dc.contributor.author Anghel, Adela
dc.contributor.author Anderson, David
dc.contributor.author Chau Chong Shing, Jorge Luis
dc.contributor.author Yumoto, Kiyohumi
dc.contributor.author Bhattacharyya, Archana
dc.date.accessioned 2018-07-19T14:04:31Z
dc.date.available 2018-07-19T14:04:31Z
dc.date.issued 2013-03-21
dc.identifier.uri http://hdl.handle.net/20.500.12816/1952
dc.description En: Midlatitude Ionospheric Dynamics and Disturbances/ edited by Paul M. Kintner, Jr., Anthea J. Coster, Tim Fuller-Rowell, Antony J. Mannucci, Michael Mendillo, Roderick Heelis, pp. 157-168. es_ES
dc.description.abstract The overall ionospheric variability with periods ranging from long-term, secular changes to days, hours, and even minutes and seconds, is influenced by the solar activity, geomagnetic activity, and processes originating in the lower atmospheric layers. Using a wavelet transform approach, in this paper, we study the short-term (minutes to hours) and day-to-day variability of the ionospheric low-latitude zonal electric fields (LLZEF) at three longitude sectors, Peruvian, Philippine, and Indian, during time intervals of increased geomagnetic activity and relate the LLZEF variability to changes in the dawn-to-dusk component of the interplanetary electric field (IEF). Continuous Morlet wavelet and cross-wavelet amplitude spectra with reduced and increased frequency resolutions were obtained to analyze and compare the oscillation activity in the LLZEF and IEF spectra, in the 10-min to 10-h and 1.25- to 12-d period ranges. For the 1.25- to 12-d period range, periodicities in the LLZEF spectrum were compared with similar periodicities in the IEF spectrum over 9 February to 9 June 2001, with our wavelet results indicating the geomagnetic activity as an important driver of LLZEF variability in this period range. For the 10-min to 10-h period range, four case studies were examined when concurrent observations of Jicamarca incoherent scatter radar zonal electric field and IEF, as calculated from the ACE satellite solar wind velocity and interplanetary magnetic field data, were available. We show that the wavelet transform represents a powerful tool to study the frequency dependence of the two specific mechanisms of ionospheric electric field variability, which are dominant during geomagnetic storms, namely penetration and disturbance dynamo. es_ES
dc.format application/pdf es_ES
dc.language.iso eng es_ES
dc.publisher American Geophysical Union es_ES
dc.relation.ispartof urn:isbn:9780875904467
dc.rights info:eu-repo/semantics/restrictedAccess es_ES
dc.subject Solar activity es_ES
dc.subject Geomagnetism es_ES
dc.subject Ionosphere es_ES
dc.subject Interplanetary magnetic fields es_ES
dc.title Relating the interplanetary-induced electric fields with the low-latitude zonal electric fields under geomagnetically disturbed conditions es_ES
dc.type info:eu-repo/semantics/bookPart es_ES
dc.subject.ocde http://purl.org/pe-repo/ocde/ford#1.05.01 es_ES
dc.description.peer-review Por pares es_ES

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