Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude

In this paper, we present further observational evidence for the transpolar propagation of large-scale traveling ionospheric disturbances (LSTIDs) from their nightside source region to the dayside reported by Cai et al. (2011). Slant total electron content (STEC) observed by longitudinally aligned G...

Full description

Bibliographic Details
Published in:Annales Geophysicae
Main Authors: Cai, H. T., Yin, F., Ma, S. Y., Xu, J. S., Liu, Y. W.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-30-1709-2012
https://angeo.copernicus.org/articles/30/1709/2012/
id ftcopernicus:oai:publications.copernicus.org:angeo15884
record_format openpolar
spelling ftcopernicus:oai:publications.copernicus.org:angeo15884 2023-05-15T16:04:31+02:00 Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude Cai, H. T. Yin, F. Ma, S. Y. Xu, J. S. Liu, Y. W. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-30-1709-2012 https://angeo.copernicus.org/articles/30/1709/2012/ eng eng doi:10.5194/angeo-30-1709-2012 https://angeo.copernicus.org/articles/30/1709/2012/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-30-1709-2012 2020-07-20T16:25:37Z In this paper, we present further observational evidence for the transpolar propagation of large-scale traveling ionospheric disturbances (LSTIDs) from their nightside source region to the dayside reported by Cai et al. (2011). Slant total electron content (STEC) observed by longitudinally aligned GPS receiver chains in North American and European sectors was analyzed to demonstrate presences of LSTIDs at both nightside and dayside mid-latitude. Signatures of TID were inferred from phase difference in time series of STEC perturbations (TECP) derived from measurements of ground-based GPS receivers, which are separated by hundreds of kilometers longitudinally. Periods of the daytime and nighttime ionospheric disturbances were estimated to be around 128 min, being in good agreement with that of the transpolar AGW (atmospheric gravity wave) recorded by EISCAT (European Incoherent Scatter Scientific Association)/ESR (EISCAT Svalbard Radar) radars. On the dayside, the LSTID moved equatorward with an average phase speed of ~440 m s −1 . In North American sector, however, southward speed of the nighttime LSTID was much slower, being around 160 m s −1 . We suggest that the observed daytime and nighttime mid-latitude LSTIDs are likely to have the same source region, being located somewhere at nighttime auroral latitude. Having been launched on the nightside, the waves propagate simultaneously equatorward and poleward. The equatorward-moving waves are recorded by GPS receiver chain in North American sector. The poleward-moving waves, however, cross the polar cap from nightside to dayside and then are detected consecutively at high and mid-latitudes by EISCAT/ESR radars and GPS receiver chains, respectively. Text EISCAT Svalbard Copernicus Publications: E-Journals Svalbard Annales Geophysicae 30 12 1709 1717
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description In this paper, we present further observational evidence for the transpolar propagation of large-scale traveling ionospheric disturbances (LSTIDs) from their nightside source region to the dayside reported by Cai et al. (2011). Slant total electron content (STEC) observed by longitudinally aligned GPS receiver chains in North American and European sectors was analyzed to demonstrate presences of LSTIDs at both nightside and dayside mid-latitude. Signatures of TID were inferred from phase difference in time series of STEC perturbations (TECP) derived from measurements of ground-based GPS receivers, which are separated by hundreds of kilometers longitudinally. Periods of the daytime and nighttime ionospheric disturbances were estimated to be around 128 min, being in good agreement with that of the transpolar AGW (atmospheric gravity wave) recorded by EISCAT (European Incoherent Scatter Scientific Association)/ESR (EISCAT Svalbard Radar) radars. On the dayside, the LSTID moved equatorward with an average phase speed of ~440 m s −1 . In North American sector, however, southward speed of the nighttime LSTID was much slower, being around 160 m s −1 . We suggest that the observed daytime and nighttime mid-latitude LSTIDs are likely to have the same source region, being located somewhere at nighttime auroral latitude. Having been launched on the nightside, the waves propagate simultaneously equatorward and poleward. The equatorward-moving waves are recorded by GPS receiver chain in North American sector. The poleward-moving waves, however, cross the polar cap from nightside to dayside and then are detected consecutively at high and mid-latitudes by EISCAT/ESR radars and GPS receiver chains, respectively.
format Text
author Cai, H. T.
Yin, F.
Ma, S. Y.
Xu, J. S.
Liu, Y. W.
spellingShingle Cai, H. T.
Yin, F.
Ma, S. Y.
Xu, J. S.
Liu, Y. W.
Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
author_facet Cai, H. T.
Yin, F.
Ma, S. Y.
Xu, J. S.
Liu, Y. W.
author_sort Cai, H. T.
title Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
title_short Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
title_full Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
title_fullStr Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
title_full_unstemmed Simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
title_sort simultaneous observations of large-scale traveling ionospheric disturbances on the nightside and dayside middle latitude
publishDate 2018
url https://doi.org/10.5194/angeo-30-1709-2012
https://angeo.copernicus.org/articles/30/1709/2012/
geographic Svalbard
geographic_facet Svalbard
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-30-1709-2012
https://angeo.copernicus.org/articles/30/1709/2012/
op_doi https://doi.org/10.5194/angeo-30-1709-2012
container_title Annales Geophysicae
container_volume 30
container_issue 12
container_start_page 1709
op_container_end_page 1717
_version_ 1766400094550097920