Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/7017
DC Field | Value | Language |
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dc.contributor.authorall | Burston, R.; University of Bath, Bath, United Kingdom | en |
dc.contributor.authorall | Astin, I.; University of Bath, Bath, United Kingdom | en |
dc.contributor.authorall | Mitchell, C.; University of Bath, Bath, United Kingdom | en |
dc.contributor.authorall | Alfonsi, Lu.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Pedersen, T.; Space Vehicles Directorate, Air Force Research Laboratory, Hanscom Air Force Base, Massachusetts, USA | en |
dc.contributor.authorall | Skone, S.; Department of Geomatics Engineering, Schulich School of Engineering, University of Calgary, Calgary, Canada | en |
dc.date.accessioned | 2011-06-01T10:37:08Z | en |
dc.date.available | 2011-06-01T10:37:08Z | en |
dc.date.issued | 2010-04-30 | en |
dc.identifier.uri | http://hdl.handle.net/2122/7017 | en |
dc.description.abstract | A model is presented of the growth rate of turbulently generated irregularities in the electron concentration of northern polar cap plasma patches. The turbulence is generated by the short‐term fluctuations in the electric field imposed on the polar cap ionosphere by electric field mapping from the magnetosphere. The model uses an ionospheric imaging algorithm to specify the state of the ionosphere throughout. The growth rates are used to estimate mean amplitudes for the irregularities, and these mean amplitudes are compared with observations of the scintillation indices S4 and s by calculating the linear correlation coefficients between them. The scintillation data are recorded by GPS L1 band receivers stationed at high northern latitudes. A total of 13 days are analyzed, covering four separate magnetic storm periods. These results are compared with those from a similar model of the gradient drift instability (GDI) growth rate. Overall, the results show better correlation between the GDI process and the scintillation indices than for the turbulence process and the scintillation indices. Two storms, however, show approximately equally good correlations for both processes, indicating that there might be times when the turbulence process of irregularity formation on plasma patches may be the controlling one. | en |
dc.language.iso | English | en |
dc.publisher.name | American Geophysical Union | en |
dc.relation.ispartof | Journal of Geophysical Research | en |
dc.relation.ispartofseries | /115(2010) | en |
dc.relation.isversionof | http://hdl.handle.net/2122/5544 | en |
dc.subject | ionospheric irregularities | en |
dc.subject | scintillations | en |
dc.subject | Gradient Drift Instability | en |
dc.title | Turbulent times in the northern polar ionosphere? | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.description.pagenumber | A04310 | en |
dc.subject.INGV | 01. Atmosphere::01.02. Ionosphere::01.02.04. Plasma Physics | en |
dc.subject.INGV | 01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations | en |
dc.subject.INGV | 05. General::05.01. Computational geophysics::05.01.03. Inverse methods | en |
dc.identifier.doi | 10.1029/2009JA014813 | en |
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Res., 100(A12), 23,819–23,827, doi:10.1029/95JA02700. Davies, K. (1990), Ionospheric Radio, Peter Peregrinus, London, U. K. Gondarenko, N. A., and P. N. Guzdar (1999), Gradient drift instability in high latitude plasma patches: Ion inertial effects, Geophys. Res. Lett., 26(22), 3345–3348, doi:10.1029/1999GL003647. Gondarenko, N. A., and P. N. Guzdar (2001), Three‐dimensional structuring characteristics of high‐latitude plasma patches, J. Geophys. Res., 106(A11), 24,611–24,620, doi:10.1029/2000JA000440. Gondarenko, N. A., and P. N. Guzdar (2004a), Plasma patch structuring by the nonlinear evolution of the gradient drift instability in the high‐latitude ionosphere, J. Geophys. Res., 109, A09301, doi:10.1029/2004JA010504. Gondarenko, N. A., and P. N. Guzdar (2004b), Density and electric field fluctuations associated with the gradient drift instability in the high‐latitude ionosphere, Geophys. Res. Lett., 31, L11802, doi:10.1029/2004GL019703. Gondarenko, N. A., and P. N. 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Int., 161(3), 561–565, doi:10.1111/j.1365- 246X.2005.02641.x. Maus, S., et al. (2005c), NGDC/GFZ candidate models for the 10th generation International Geomagnetic Reference Field, Earth Planets Space, 57(12), 1151–1156. Mounir, H., C. J. Cerisier, A. Berthelier, D. Lagoutte, and C. Beghin (1991), The small‐scale turbulent structure of the high latitude ionosphere: ARCAD‐AUREOL‐3 observations, Ann. Geophys., 9, 725–737. Ossakow, S. L., and P. K. Chaturvedi (1979), Current convective instability in the diffuse aurora, Geophys. Res. Lett., 6(4), 332–334, doi:10.1029/ GL006i004p00332. Sojka, J. J., et al. (1998), Gradient drift instability growth rates from globalscale modeling of the polar ionosphere, Radio Sci., 33(6), 1915–1928, doi:10.1029/98RS02490. Spencer, P. S. J., and C. N. Mitchell (2007), Imaging of fast moving electron‐ density structures in the polar cap, Ann. Geophys., 50, 427–434. Zvezdin, V. N., and S. V. Fridman (1992), Regimes of ionospheric turbulence from fractal analysis of satellite radio signal scintillations, J. Atmos. Terr. Phys., 54(7–8), 957–962, doi:10.1016/0021-9169(92)90061-O. | en |
dc.description.obiettivoSpecifico | 1.7. Osservazioni di alta e media atmosfera | en |
dc.description.obiettivoSpecifico | 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | restricted | en |
dc.contributor.author | Burston, R. | en |
dc.contributor.author | Astin, I. | en |
dc.contributor.author | Mitchell, C. | en |
dc.contributor.author | Alfonsi, Lu. | en |
dc.contributor.author | Pedersen, T. | en |
dc.contributor.author | Skone, S. | en |
dc.contributor.department | University of Bath, Bath, United Kingdom | en |
dc.contributor.department | University of Bath, Bath, United Kingdom | en |
dc.contributor.department | University of Bath, Bath, United Kingdom | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Space Vehicles Directorate, Air Force Research Laboratory, Hanscom Air Force Base, Massachusetts, USA | en |
dc.contributor.department | Department of Geomatics Engineering, Schulich School of Engineering, University of Calgary, Calgary, Canada | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | restricted | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | University of Bath, UK | - |
crisitem.author.dept | University of Bath, UK | - |
crisitem.author.dept | 3Department of Electronic and Electrical Engineering, University of Bath | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Space Vehicles Directorate, Air Force Research Laboratory, Hanscom Air Force Base, Massachusetts, USA | - |
crisitem.author.dept | Department of Geomatics Engineering, Schulich School of Engineering, University of Calgary, Calgary, Alberta, Canada | - |
crisitem.author.orcid | 0000-0003-4989-9187 | - |
crisitem.author.orcid | 0000-0002-1806-9327 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.classification.parent | 05. General | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
Appears in Collections: | Article published / in press |
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