Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/89911
PIRA download icon_1.1View/Download Full Text
DC FieldValueLanguage
dc.contributorDepartment of Building Services Engineeringen_US
dc.creatorGao, Yen_US
dc.creatorChen, Men_US
dc.creatorQin, Zen_US
dc.creatorQiu, Zen_US
dc.creatorYang, Yen_US
dc.creatorDu, YPen_US
dc.creatorWang, Sen_US
dc.creatorZhang, Gen_US
dc.date.accessioned2021-05-13T08:32:38Z-
dc.date.available2021-05-13T08:32:38Z-
dc.identifier.issn2169-897Xen_US
dc.identifier.urihttp://hdl.handle.net/10397/89911-
dc.language.isoenen_US
dc.publisherWiley-Blackwellen_US
dc.rights©2020. American Geophysical Union. All Rights Reserved.en_US
dc.subjectLeader channel evolutionen_US
dc.subjectTall toweren_US
dc.subjectUpward flashen_US
dc.subjectUpward positive stepped leaderen_US
dc.titleThe spatial evolution of upward positive stepped leaders initiated from a 356-m-tall tower in Southern Chinaen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage1en_US
dc.identifier.epage18en_US
dc.identifier.volume125en_US
dc.identifier.issue2en_US
dc.identifier.doi10.1029/2019JD031508en_US
dcterms.abstractTwo initial upward positive leaders (UPLs) in upward negative flashes initiated from a 356-m-tall tower were observed with a high-speed camera, an electric field sensor, and a magnetic field sensor. Although the waveforms of electric fields measured were saturated, both camera images and magnetic fields showed that the two UPLs had obvious stepwise characteristics in their upward moving stage. The magnetic fields associated with the UPLs were characterized by a series of fast-changing bipolar impulses superimposed on a slowly increasing continuous component as the leaders moved upward, which were well corresponding to the light intensity changes of their high-speed camera images. The 2-D step length and step extension speed of the two leaders were estimated in the range of 0.5–3 m and 1.1–9.4 × 105 m/s, respectively. The radius of the leader luminous channel as a function of time and height was also estimated. The channel radius showed first a stable increasing trend in the leader upward moving stage and then 4–5 times of shrinking and expanding processes after the leader connected the cloud. The channel expanding and shrinking speeds were in the range of 2–9 × 104 m/s. Particularly, the channel radius showed an obvious increasing trend with the increase of the height all the time, which was in the range of 2.8–3.5 m when around the tower tip and of 5.6–8.4 m when at 24 m high above the tower tip. Such a feature of the channel radius is in good agreement with the concept of leader corona sheath in literature.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationJournal of geophysical research. Atmospheres, 27 Jan. 2020, v. 125, no. 2, e2019JD031508, p. 1-18en_US
dcterms.isPartOfJournal of geophysical research. Atmospheresen_US
dcterms.issued2020-01-27-
dc.identifier.scopus2-s2.0-85079403480-
dc.identifier.eissn2169-8996en_US
dc.identifier.artne2019JD031508en_US
dc.description.validate202105 bcvcen_US
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumbera0806-n03-
dc.identifier.SubFormID1898-
dc.description.fundingSourceRGCen_US
dc.description.fundingTextPolyU 152652/16E; PolyU 152147/19Een_US
dc.description.pubStatusPublisheden_US
dc.description.oaCategoryVoR alloweden_US
Appears in Collections:Journal/Magazine Article
Files in This Item:
File Description SizeFormat 
1898_2019JD031508.pdf4.67 MBAdobe PDFView/Open
Open Access Information
Status open access
File Version Version of Record
Access
View full-text via PolyU eLinks SFX Query
Show simple item record

Page views

139
Last Week
41
Last month
Citations as of Nov 10, 2025

Downloads

112
Citations as of Nov 10, 2025

SCOPUSTM   
Citations

20
Citations as of Dec 19, 2025

WEB OF SCIENCETM
Citations

13
Citations as of Dec 18, 2025

Google ScholarTM

Check

Altmetric


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.