Publication:
Transmitter-induced modulation of subionospheric VLF signals: Ionospheric heating rather than electron precipitation

dc.contributor.coauthorGraf, K. L.
dc.contributor.coauthorSpasojevic, M.
dc.contributor.departmentDepartment of Electrical and Electronics Engineering
dc.contributor.kuauthorİnan, Umran Savaş
dc.contributor.schoolcollegeinstituteCollege of Engineering
dc.date.accessioned2024-11-09T13:25:49Z
dc.date.issued2011
dc.description.abstractThe controlled keying of ground-based VLF transmitters with periodic on/off sequences allows the detection of weak but measurable cross-modulation effects on other subionospheric VLF probe signals used for VLF remote sensing. In this paper, we reexamine previously published and additional cases of such events and determine that the initial interpretations of such cross modulation as being due to electron precipitation is likely incorrect. Rather, such events appear to be fully consistent with ionospheric heating caused by the keyed signal, even when the probe VLF signal path lies thousands of kilometers from the heating VLF transmitter. The 21.4 kHz transmitter NPM located in Lualualei, Hawaii, is keyed on/off in periodic sequences, and that same periodicity is observed on the subionospherically propagating probe signal generated by the 24.8 kHz transmitter NLK of Jim Creek, Washington. Previous initial conclusions published for these experiments do not hold under detailed review due to the lack of discernible onset delay and lag time in the observed perturbations, which eliminates transmitter-induced precipitation of electron radiation as a possible cause. Detailed testing of the receiver shows instrumental cross-modulation to not be a concern in these observations. It is thus concluded that the observed perturbations, despite occurring on a probe signal pathway that is 1750 km away from NPM at its point of closest approach, are due to direct ionospheric heating by the keyed VLF transmitter NPM. Results indicate that the VLF transmitter may affect the overlying ionosphere over much larger lateral regions than previously believed.
dc.description.fulltextYES
dc.description.indexedbyWOS
dc.description.indexedbyScopus
dc.description.issueA12
dc.description.openaccessYES
dc.description.publisherscopeInternational
dc.description.sponsoredbyTubitakEuN/A
dc.description.sponsorshipDefense Advanced Research Projects Agency under Office of Naval Research
dc.description.sponsorshipDepartment of Air Force
dc.description.sponsorshipNational Science Foundation
dc.description.versionPublisher version
dc.description.volume116
dc.identifier.doi10.1029/2011JA016996
dc.identifier.eissn2169-9402
dc.identifier.embargoNO
dc.identifier.filenameinventorynoIR00617
dc.identifier.issn2169-9380
dc.identifier.quartileN/A
dc.identifier.scopus2-s2.0-83455163642
dc.identifier.urihttps://hdl.handle.net/20.500.14288/3462
dc.identifier.wos297978700005
dc.keywordsLow-frequency transmitters
dc.keywordsRadiation belt electrons
dc.keywordsNighttime d-region
dc.keywordsRadio-waves
dc.language.isoeng
dc.publisherAmerican Geophysical Union (AGU)
dc.relation.grantnoN00014-06-1-1036, N00014-03-1-0630, N00014-05-1-0854
dc.relation.grantnoFA9453-11-C-0011
dc.relation.grantnoANT-1043442, ANT-0538627
dc.relation.ispartofJournal of Geophysical Research: Space Physics
dc.relation.urihttp://cdm21054.contentdm.oclc.org/cdm/ref/collection/IR/id/682
dc.subjectAstronomy and astrophysics
dc.titleTransmitter-induced modulation of subionospheric VLF signals: Ionospheric heating rather than electron precipitation
dc.typeJournal Article
dspace.entity.typePublication
local.contributor.kuauthorİnan, Umran Savaş
local.publication.orgunit1College of Engineering
local.publication.orgunit2Department of Electrical and Electronics Engineering
relation.isOrgUnitOfPublication21598063-a7c5-420d-91ba-0cc9b2db0ea0
relation.isOrgUnitOfPublication.latestForDiscovery21598063-a7c5-420d-91ba-0cc9b2db0ea0
relation.isParentOrgUnitOfPublication8e756b23-2d4a-4ce8-b1b3-62c794a8c164
relation.isParentOrgUnitOfPublication.latestForDiscovery8e756b23-2d4a-4ce8-b1b3-62c794a8c164

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