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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Bibliographic Details
Main Authors: Meggs, R. W., Mitchell, C. N., Howells, V. S. C.
Other Authors: Department of Electronic and Electrical Engineering, STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2005
Subjects:
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Eia
EISCAT
Online Access:https://hal.science/hal-00317604
https://hal.science/hal-00317604/document
https://hal.science/hal-00317604/file/angeo-23-753-2005.pdf
Description
Summary: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.

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