Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons

Descripción del Articulo

Data from a network of high-frequency (HF) beacons deployed in Peru are used to estimate the regional ionospheric electron density in a volume. Pseudorange, accumulated carrier phase, and signal power measurements for each of the 36 ray paths provided by the network at a 1 min cadence are incorporat...

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Detalles Bibliográficos
Autores: Hysell, D. L., Rojas, E., Goldberg, H., Milla, Marco, Kuyeng, K., Valdez, A., Morton, Y. T., Bourne, H.
Formato: artículo
Fecha de Publicación:2021
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/5123
Enlace del recurso:http://hdl.handle.net/20.500.12816/5123
https://doi.org/10.1029/2021JA029229
Nivel de acceso:acceso abierto
Materia:Beacon
Electron density
Equatorial ionosphere
HF
Inverse methods
https://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
title Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
spellingShingle Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
Hysell, D. L.
Beacon
Electron density
Equatorial ionosphere
HF
Inverse methods
https://purl.org/pe-repo/ocde/ford#1.05.01
title_short Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
title_full Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
title_fullStr Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
title_full_unstemmed Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
title_sort Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons
author Hysell, D. L.
author_facet Hysell, D. L.
Rojas, E.
Goldberg, H.
Milla, Marco
Kuyeng, K.
Valdez, A.
Morton, Y. T.
Bourne, H.
author_role author
author2 Rojas, E.
Goldberg, H.
Milla, Marco
Kuyeng, K.
Valdez, A.
Morton, Y. T.
Bourne, H.
author2_role author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Hysell, D. L.
Rojas, E.
Goldberg, H.
Milla, Marco
Kuyeng, K.
Valdez, A.
Morton, Y. T.
Bourne, H.
dc.subject.none.fl_str_mv Beacon
Electron density
Equatorial ionosphere
HF
Inverse methods
topic Beacon
Electron density
Equatorial ionosphere
HF
Inverse methods
https://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.none.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.05.01
description Data from a network of high-frequency (HF) beacons deployed in Peru are used to estimate the regional ionospheric electron density in a volume. Pseudorange, accumulated carrier phase, and signal power measurements for each of the 36 ray paths provided by the network at a 1 min cadence are incorporated in the estimates. Additional data from the Jicamarca incoherent scatter radar, the Jicamarca sounder, and GPS receivers can also be incorporated. The electron density model is estimated as the solution to a global optimization problem that uses ray tracing in the forward model. The electron density is parametrized in terms of B-splines in the horizontal direction and generalized Chapman functions or related functions in the vertical. Variational sensitivity analysis has been added to the method to allow for the utilization of the signal power observable which gives additional information about the morphology of the bottomside F region as well as absorption including absorption in the D and E regions. The goal of the effort is to provide contextual information for improving numerical forecasts of plasma interchange instabilities in the postsunset F region ionosphere associated with equatorial spread F (ESF). Data from two ESF campaigns are presented. In one experiment, the HF data revealed the presence of a large-scale bottomside deformation that seems to have led to instability under otherwise inauspicious conditions. In another experiment, gradual variations in HF signal power were found to be related to the varying shape of the bottomside F layer.
publishDate 2021
dc.date.accessioned.none.fl_str_mv 2022-02-25T11:26:43Z
dc.date.available.none.fl_str_mv 2022-02-25T11:26:43Z
dc.date.issued.fl_str_mv 2021-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Hysell, D. L., Rojas, E., Goldberg, H., Milla, M. A., Kuyeng, K., Valdez, A., … Bourne, H. (2021). Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons.==$Journal of Geophysical Research: Space Physics, 126$==(7), e2021JA029229. https://doi.org/10.1029/2021JA029229
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/5123
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1029/2021JA029229
identifier_str_mv Hysell, D. L., Rojas, E., Goldberg, H., Milla, M. A., Kuyeng, K., Valdez, A., … Bourne, H. (2021). Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons.==$Journal of Geophysical Research: Space Physics, 126$==(7), e2021JA029229. https://doi.org/10.1029/2021JA029229
index-oti2018
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/5123
https://doi.org/10.1029/2021JA029229
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:2169-9402
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
dc.source.none.fl_str_mv reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
institution IGP
reponame_str IGP-Institucional
collection IGP-Institucional
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spelling Hysell, D. L.Rojas, E.Goldberg, H.Milla, MarcoKuyeng, K.Valdez, A.Morton, Y. T.Bourne, H.2022-02-25T11:26:43Z2022-02-25T11:26:43Z2021-07Hysell, D. L., Rojas, E., Goldberg, H., Milla, M. A., Kuyeng, K., Valdez, A., … Bourne, H. (2021). Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beacons.==$Journal of Geophysical Research: Space Physics, 126$==(7), e2021JA029229. https://doi.org/10.1029/2021JA029229index-oti2018http://hdl.handle.net/20.500.12816/5123Journal of Geophysical Research: Space Physicshttps://doi.org/10.1029/2021JA029229Data from a network of high-frequency (HF) beacons deployed in Peru are used to estimate the regional ionospheric electron density in a volume. Pseudorange, accumulated carrier phase, and signal power measurements for each of the 36 ray paths provided by the network at a 1 min cadence are incorporated in the estimates. Additional data from the Jicamarca incoherent scatter radar, the Jicamarca sounder, and GPS receivers can also be incorporated. The electron density model is estimated as the solution to a global optimization problem that uses ray tracing in the forward model. The electron density is parametrized in terms of B-splines in the horizontal direction and generalized Chapman functions or related functions in the vertical. Variational sensitivity analysis has been added to the method to allow for the utilization of the signal power observable which gives additional information about the morphology of the bottomside F region as well as absorption including absorption in the D and E regions. The goal of the effort is to provide contextual information for improving numerical forecasts of plasma interchange instabilities in the postsunset F region ionosphere associated with equatorial spread F (ESF). Data from two ESF campaigns are presented. In one experiment, the HF data revealed the presence of a large-scale bottomside deformation that seems to have led to instability under otherwise inauspicious conditions. In another experiment, gradual variations in HF signal power were found to be related to the varying shape of the bottomside F layer.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9402info:eu-repo/semantics/openAccessBeaconElectron densityEquatorial ionosphereHFInverse methodshttps://purl.org/pe-repo/ocde/ford#1.05.01Mapping irregularities in the postsunset equatorial ionosphere with an expanded network of HF beaconsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALHysell_el_al_2021_JGR_Space_Physics.pdfapplication/pdf5244692https://repositorio.igp.gob.pe/bitstreams/be8a80a2-8845-4121-9533-4bb379f5f98d/downloaddc205462b667770e9f753b53c3f269f5MD55LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/d0dd8aed-b23c-4f49-a952-4113e383b649/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTHysell_el_al_2021_JGR_Space_Physics.pdf.txtHysell_el_al_2021_JGR_Space_Physics.pdf.txtExtracted texttext/plain1961https://repositorio.igp.gob.pe/bitstreams/264f4013-2ef1-4c6a-a918-ed740d90ca61/downloadff1f15d5778f3c4913fabe4b2a497c96MD53THUMBNAILHysell_el_al_2021_JGR_Space_Physics.pdf.jpgHysell_el_al_2021_JGR_Space_Physics.pdf.jpgIM Thumbnailimage/jpeg65737https://repositorio.igp.gob.pe/bitstreams/faf09bd1-2e89-4be1-97b4-f671f71fcc17/download0f69dfeb33a7824cf88fd3652f8c47e9MD5420.500.12816/5123oai:repositorio.igp.gob.pe:20.500.12816/51232025-08-19 10:40:41.489open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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