Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/76063
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dc.contributorDepartment of Building Services Engineeringen_US
dc.contributorDepartment of Land Surveying and Geo-Informaticsen_US
dc.creatorKumar, Sen_US
dc.creatorChen, Wen_US
dc.creatorChen, MLen_US
dc.creatorLiu, ZZen_US
dc.creatorSingh, RPen_US
dc.date.accessioned2018-05-10T02:55:16Z-
dc.date.available2018-05-10T02:55:16Z-
dc.identifier.issn2169-9380en_US
dc.identifier.urihttp://hdl.handle.net/10397/76063-
dc.language.isoenen_US
dc.publisherWiley-Blackwellen_US
dc.rights©2017. American Geophysical Union. All Rights Reserved.en_US
dc.subjectLightningen_US
dc.subjectIonosphereen_US
dc.subjectGravity wavesen_US
dc.subjectIonospheric irregularitiesen_US
dc.titleThunderstorm-/lightning-induced ionospheric perturbation : an observation from equatorial and low-latitude stations around Hong Kongen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage9032en_US
dc.identifier.epage9044en_US
dc.identifier.volume122en_US
dc.identifier.issue8en_US
dc.identifier.doi10.1002/2017JA023914en_US
dcterms.abstractTotal electron content (TEC) computed from the network of Global Positioning System over Hong Kong area known as Hong Kong Sat-Ref-network has been used to study perturbation in the ionosphere from thunder storm activity. Data for geomagnetic quiet day (Kp<4, on 1 April 2014) have been analyzed. The lightning activity was measured from Total Lightning sensor LS8000 over/around the Hong Kong region. Deviation in vertical TEC (DTEC) and the rate of change of TEC index (ROTI) have been derived and compared for lightning day of 1 April 2014 and nonlightning day of 7 April 2014. An analysis showed reduction in TEC during evening hour (up to 1245 UT), whereas an enhancement during nighttime hour on the lightning day is observed. The variations in DTEC during nonlightning day are found to be insignificant in comparison to that during the lightning day. The ionospheric perturbation in TEC has been noticed up to a distance around similar to 500km and more from the lightning center. ROTI is found to vary from 3 to 60total electron content unit (TECU)/min (1TECU=10(16)elm(-2)) on the day of thunderstorm activity, whereas ROTI is insignificant on nonlightning days. Signature of density bubbles in slant TEC data and periodicities (10-100min) in DTEC data are observed. For the same pseudorandom numbers (1, 10, 13, 23, and 28) strong amplitude scintillations are also observed at a close by station. Amplitude scintillations are proposed to be caused by plasma bubbles. The results are tentatively explained by thunderstorm-induced electric fields and gravity waves.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationJournal of geophysical research : space physics, Aug. 2017, v. 122, no. 8, p. 9032-9044en_US
dcterms.isPartOfJournal of geophysical research : space physicsen_US
dcterms.issued2017-08-
dc.identifier.isiWOS:000411788800079-
dc.identifier.eissn2169-9402en_US
dc.identifier.rosgroupid2017005180-
dc.description.ros2017-2018 > Academic research: refereed > Publication in refereed journalen_US
dc.description.validate201805 bcrcen_US
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberLSGI-0363-
dc.description.fundingSourceRGCen_US
dc.description.fundingSourceOthersen_US
dc.description.fundingTextERB/DST, New Delhien_US
dc.description.pubStatusPublisheden_US
dc.identifier.OPUS6778687-
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