Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/100772
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dc.contributorDepartment of Land Surveying and Geo-Informatics-
dc.creatorKumar, Sen_US
dc.creatorChen, Wen_US
dc.date.accessioned2023-08-11T03:13:21Z-
dc.date.available2023-08-11T03:13:21Z-
dc.identifier.isbn978-1-5090-1757-7 (Electronic)en_US
dc.identifier.isbn978-1-5090-1938-0 (Print on Demand(PoD))en_US
dc.identifier.urihttp://hdl.handle.net/10397/100772-
dc.description2016 International Conference on Localization and GNSS (ICL-GNSS), 28-30 June 2016, Barcelona, Spain.en_US
dc.language.isoenen_US
dc.publisherIEEEen_US
dc.rights© 2016 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.en_US
dc.rightsThe following publication S. Kumar and W. Chen, "Remote sensing of ionospheric plasma bubbles using GPS/GNSS," 2016 International Conference on Localization and GNSS (ICL-GNSS), Barcelona, Spain, 2016, pp. 1-5 is available at https://doi.org/10.1109/ICL-GNSS.2016.7533858.en_US
dc.subjectEquatorial ionosphereen_US
dc.subjectPlasma bubblesen_US
dc.subjectSolar deep minimumen_US
dc.titleRemote sensing of ionospheric plasma bubbles using GPS/GNSSen_US
dc.typeConference Paperen_US
dc.identifier.spage1en_US
dc.identifier.epage5en_US
dc.identifier.doi10.1109/ICL-GNSS.2016.7533858en_US
dcterms.abstractThe equatorial plasma bubble (EPB) is plasma depleted region of the ionosphere which affects the trans-ionospheric communication/ navigation to great extent. In this paper occurrence and characteristic of plasma bubbles over the Hong Kong during deep solar minimum 2007-2009, has been studied using the GPS data from continuously operating reference stations (CORS) network. Generally, plasma bubble occurrence is expected to be maximum during the equinox season but for the deep solar minimum period from 2007 to 2009 unusual seasonal occurrence in plasma bubbles has been observed and found to be a maximum during the June solstice instead of equinox. The diurnal characteristics of plasma bubbles have been studied and their occurrences are found to be more prominent during the nighttime hours. Moreover, the daytime EPBs observations are also noticed but their occurrences are found to be occasional. The observed daytime plasma bubbles are expected to be generated in the post-midnight hour at higher altitude and can survive until the daytime. The latitudinal dimensions of observed plasma bubbles during 2007-2009 are found to be dominant in 200-400 km range.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitation2016 International Conference on Localization and GNSS (ICL-GNSS), Barcelona, Spain, 28-30 June 2016, p. 1-5en_US
dcterms.issued2016-
dc.identifier.scopus2-s2.0-84986237833-
dc.relation.conferenceInternational Conference on Localization and GNSS [ICL-GNSS]-
dc.description.validate202305 bckw-
dc.description.oaAccepted Manuscripten_US
dc.identifier.FolderNumberLSGI-0434-
dc.description.fundingSourceRGCen_US
dc.description.fundingSourceOthersen_US
dc.description.fundingTextNational Natural Science Foundation of Chinaen_US
dc.description.pubStatusPublisheden_US
dc.identifier.OPUS9580129-
dc.description.oaCategoryGreen (AAM)en_US
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