A first comparison of irregularity and ion drift velocity measurements in the E-region
E-region irregularity velocity measurements at large flow angles with the STARE Finland coherent VHF radar are considered in context of the ion and electron velocity data provided by the EISCAT tristatic radar system, CUTLASS Finland coherent HF radar, and IMAGE fluxgate magnetometers. The data have...
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ftcopernicus:oai:publications.copernicus.org:angeo35986 2023-05-15T16:04:28+02:00 A first comparison of irregularity and ion drift velocity measurements in the E-region Makarevich, R. A. Honary, F. Howells, V. S. C. Koustov, A. V. Milan, S. E. Davies, J. A. Senior, A. McCrea, I. W. Dyson, P. L. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-24-2375-2006 https://angeo.copernicus.org/articles/24/2375/2006/ eng eng doi:10.5194/angeo-24-2375-2006 https://angeo.copernicus.org/articles/24/2375/2006/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-24-2375-2006 2020-07-20T16:27:12Z E-region irregularity velocity measurements at large flow angles with the STARE Finland coherent VHF radar are considered in context of the ion and electron velocity data provided by the EISCAT tristatic radar system, CUTLASS Finland coherent HF radar, and IMAGE fluxgate magnetometers. The data have been collected during a special experiment on 27 March 2004 during which EISCAT was scanning between several E- and one F-region altitudes along the magnetic field line. Within the E-region, the EISCAT measurements at two altitudes of 110 and 115 km are considered while the electron velocity is inferred from the EISCAT ion velocity measurements at 278 km. The line-of-sight (l-o-s) VHF velocity measured by STARE VHF los is compared to the ion and electron velocity components ( V i0 comp and V e0 comp ) along the STARE l-o-s direction. The comparison with V e0 comp for the entire event shows that the measurements exhibit large scatter and small positive correlation. The correlation with V e0 comp was substantial in the first half of the interval under study when V e0 comp was larger in magnitude. The comparison with V i0 comp at 110 and 115 km shows a considerable positive correlation, with VHF velocity being typically larger (smaller) in magnitude than V i0 comp at 110 km (115 km) so that V VHF los appears to be bounded by the ion velocity components at two altitudes. It is also demonstrated that the difference between V VHF los and V i0 comp at 110 km can be treated, in the first approximation, as a linear function of the effective backscatter height h eff also counted from 110 km; h eff varies in the range 108–114 km due to the altitude integration effects in the scattering cross-section. Our results are consistent with the notion that VHF velocity at large flow angles is directly related to the ion drift velocity component at an altitude h eff . Text EISCAT Copernicus Publications: E-Journals Annales Geophysicae 24 9 2375 2389 |
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Open Polar |
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Copernicus Publications: E-Journals |
op_collection_id |
ftcopernicus |
language |
English |
description |
E-region irregularity velocity measurements at large flow angles with the STARE Finland coherent VHF radar are considered in context of the ion and electron velocity data provided by the EISCAT tristatic radar system, CUTLASS Finland coherent HF radar, and IMAGE fluxgate magnetometers. The data have been collected during a special experiment on 27 March 2004 during which EISCAT was scanning between several E- and one F-region altitudes along the magnetic field line. Within the E-region, the EISCAT measurements at two altitudes of 110 and 115 km are considered while the electron velocity is inferred from the EISCAT ion velocity measurements at 278 km. The line-of-sight (l-o-s) VHF velocity measured by STARE VHF los is compared to the ion and electron velocity components ( V i0 comp and V e0 comp ) along the STARE l-o-s direction. The comparison with V e0 comp for the entire event shows that the measurements exhibit large scatter and small positive correlation. The correlation with V e0 comp was substantial in the first half of the interval under study when V e0 comp was larger in magnitude. The comparison with V i0 comp at 110 and 115 km shows a considerable positive correlation, with VHF velocity being typically larger (smaller) in magnitude than V i0 comp at 110 km (115 km) so that V VHF los appears to be bounded by the ion velocity components at two altitudes. It is also demonstrated that the difference between V VHF los and V i0 comp at 110 km can be treated, in the first approximation, as a linear function of the effective backscatter height h eff also counted from 110 km; h eff varies in the range 108–114 km due to the altitude integration effects in the scattering cross-section. Our results are consistent with the notion that VHF velocity at large flow angles is directly related to the ion drift velocity component at an altitude h eff . |
format |
Text |
author |
Makarevich, R. A. Honary, F. Howells, V. S. C. Koustov, A. V. Milan, S. E. Davies, J. A. Senior, A. McCrea, I. W. Dyson, P. L. |
spellingShingle |
Makarevich, R. A. Honary, F. Howells, V. S. C. Koustov, A. V. Milan, S. E. Davies, J. A. Senior, A. McCrea, I. W. Dyson, P. L. A first comparison of irregularity and ion drift velocity measurements in the E-region |
author_facet |
Makarevich, R. A. Honary, F. Howells, V. S. C. Koustov, A. V. Milan, S. E. Davies, J. A. Senior, A. McCrea, I. W. Dyson, P. L. |
author_sort |
Makarevich, R. A. |
title |
A first comparison of irregularity and ion drift velocity measurements in the E-region |
title_short |
A first comparison of irregularity and ion drift velocity measurements in the E-region |
title_full |
A first comparison of irregularity and ion drift velocity measurements in the E-region |
title_fullStr |
A first comparison of irregularity and ion drift velocity measurements in the E-region |
title_full_unstemmed |
A first comparison of irregularity and ion drift velocity measurements in the E-region |
title_sort |
first comparison of irregularity and ion drift velocity measurements in the e-region |
publishDate |
2018 |
url |
https://doi.org/10.5194/angeo-24-2375-2006 https://angeo.copernicus.org/articles/24/2375/2006/ |
genre |
EISCAT |
genre_facet |
EISCAT |
op_source |
eISSN: 1432-0576 |
op_relation |
doi:10.5194/angeo-24-2375-2006 https://angeo.copernicus.org/articles/24/2375/2006/ |
op_doi |
https://doi.org/10.5194/angeo-24-2375-2006 |
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Annales Geophysicae |
container_volume |
24 |
container_issue |
9 |
container_start_page |
2375 |
op_container_end_page |
2389 |
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1766400060510175232 |