Simultaneous observations of the main trough using GPS imaging and the EISCAT radar
International audience We use a digisonde at Jicamarca and a chain of GPS receivers on the west side of South America to investigate the effects of the pre-reversal enhancement (PRE) in E x B drift, the asymmetry ( I a ) of equatorial ionization anomaly (EIA), and the magnetic activity ( K p ) on th...
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ftccsdartic:oai:HAL:hal-00317604v1 2023-11-12T04:16:38+01:00 Simultaneous observations of the main trough using GPS imaging and the EISCAT radar Meggs, R. W. Mitchell, C. N. Howells, V. S. C. Department of Electronic and Electrical Engineering STFC Rutherford Appleton Laboratory (RAL) Science and Technology Facilities Council (STFC) 2005-03-30 https://hal.science/hal-00317604 https://hal.science/hal-00317604/document https://hal.science/hal-00317604/file/angeo-23-753-2005.pdf en eng HAL CCSD European Geosciences Union hal-00317604 https://hal.science/hal-00317604 https://hal.science/hal-00317604/document https://hal.science/hal-00317604/file/angeo-23-753-2005.pdf info:eu-repo/semantics/OpenAccess ISSN: 0992-7689 EISSN: 1432-0576 Annales Geophysicae https://hal.science/hal-00317604 Annales Geophysicae, 2005, 23 (3), pp.753-757 [SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/article Journal articles 2005 ftccsdartic 2023-10-21T23:07:19Z International audience We use a digisonde at Jicamarca and a chain of GPS receivers on the west side of South America to investigate the effects of the pre-reversal enhancement (PRE) in E x B drift, the asymmetry ( I a ) of equatorial ionization anomaly (EIA), and the magnetic activity ( K p ) on the generation of equatorial spread F (ESF). Results show that the ESF appears frequently in summer (November, December, January, and February) and equinoctial (March, April, September, and October) months, but rarely in winter (May, June, July, and August) months. The seasonal variation in the ESF is associated with those in the PRE E x B drift and I a . The larger E x B drift (>20m/s) and smaller | I a | (<0.3) in summer and equinoctial months provide a preferable condition to development the ESF. Conversely, the smaller E x B drift and larger | I a | are responsible for the lower ESF occurrence in winter months. Regarding the effects of magnetic activity, the ESF occurrence decreases with increasing K p in the equinoctial and winter months, but not in the summer months. Furthermore, the larger and smaller E x B drifts are presented under the quiet ( K p <3) and disturbed ( K p ?3) conditions, respectively. These results indicate that the suppression in ESF and the decrease in E x B drifts are mainly caused by the decrease in the eastward electric field. Article in Journal/Newspaper EISCAT Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Eia ENVELOPE(7.755,7.755,63.024,63.024) |
institution |
Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
English |
topic |
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.STU]Sciences of the Universe [physics]/Earth Sciences |
spellingShingle |
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.STU]Sciences of the Universe [physics]/Earth Sciences Meggs, R. W. Mitchell, C. N. Howells, V. S. C. Simultaneous observations of the main trough using GPS imaging and the EISCAT radar |
topic_facet |
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.STU]Sciences of the Universe [physics]/Earth Sciences |
description |
International audience We use a digisonde at Jicamarca and a chain of GPS receivers on the west side of South America to investigate the effects of the pre-reversal enhancement (PRE) in E x B drift, the asymmetry ( I a ) of equatorial ionization anomaly (EIA), and the magnetic activity ( K p ) on the generation of equatorial spread F (ESF). Results show that the ESF appears frequently in summer (November, December, January, and February) and equinoctial (March, April, September, and October) months, but rarely in winter (May, June, July, and August) months. The seasonal variation in the ESF is associated with those in the PRE E x B drift and I a . The larger E x B drift (>20m/s) and smaller | I a | (<0.3) in summer and equinoctial months provide a preferable condition to development the ESF. Conversely, the smaller E x B drift and larger | I a | are responsible for the lower ESF occurrence in winter months. Regarding the effects of magnetic activity, the ESF occurrence decreases with increasing K p in the equinoctial and winter months, but not in the summer months. Furthermore, the larger and smaller E x B drifts are presented under the quiet ( K p <3) and disturbed ( K p ?3) conditions, respectively. These results indicate that the suppression in ESF and the decrease in E x B drifts are mainly caused by the decrease in the eastward electric field. |
author2 |
Department of Electronic and Electrical Engineering STFC Rutherford Appleton Laboratory (RAL) Science and Technology Facilities Council (STFC) |
format |
Article in Journal/Newspaper |
author |
Meggs, R. W. Mitchell, C. N. Howells, V. S. C. |
author_facet |
Meggs, R. W. Mitchell, C. N. Howells, V. S. C. |
author_sort |
Meggs, R. W. |
title |
Simultaneous observations of the main trough using GPS imaging and the EISCAT radar |
title_short |
Simultaneous observations of the main trough using GPS imaging and the EISCAT radar |
title_full |
Simultaneous observations of the main trough using GPS imaging and the EISCAT radar |
title_fullStr |
Simultaneous observations of the main trough using GPS imaging and the EISCAT radar |
title_full_unstemmed |
Simultaneous observations of the main trough using GPS imaging and the EISCAT radar |
title_sort |
simultaneous observations of the main trough using gps imaging and the eiscat radar |
publisher |
HAL CCSD |
publishDate |
2005 |
url |
https://hal.science/hal-00317604 https://hal.science/hal-00317604/document https://hal.science/hal-00317604/file/angeo-23-753-2005.pdf |
long_lat |
ENVELOPE(7.755,7.755,63.024,63.024) |
geographic |
Eia |
geographic_facet |
Eia |
genre |
EISCAT |
genre_facet |
EISCAT |
op_source |
ISSN: 0992-7689 EISSN: 1432-0576 Annales Geophysicae https://hal.science/hal-00317604 Annales Geophysicae, 2005, 23 (3), pp.753-757 |
op_relation |
hal-00317604 https://hal.science/hal-00317604 https://hal.science/hal-00317604/document https://hal.science/hal-00317604/file/angeo-23-753-2005.pdf |
op_rights |
info:eu-repo/semantics/OpenAccess |
_version_ |
1782333707707744256 |