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...
| Autores: | , , , , , , , |
|---|---|
| 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 |
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openAccess |
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application/pdf |
| dc.publisher.none.fl_str_mv |
American Geophysical Union |
| publisher.none.fl_str_mv |
American Geophysical Union |
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IGP |
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IGP-Institucional |
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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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 |
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La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).