Publication Date:
2017-04-04
Description:
Arrays of GPS Ionospheric Scintillation and TEC Monitors (GISTMs) are used in a comparative scintillation study focusing on quasi-conjugate pairs of GPS receivers in
the Arctic and Antarctic. Intense GPS phase scintillation and rapid variations in ionospheric total electron content (TEC)
that can result in cycle slips were observed at high latitudes with dual-frequency GPS receivers during the first significant
geomagnetic storm of solar cycle 24 on 5–7 April 2010.
The impact of a bipolar magnetic cloud of north-south (NS) type embedded in high speed solar wind from a coronal hole caused a geomagnetic storm with maximum 3-hourly Kp = 8- and hourly ring current Dst =−73 nT. The interhemispheric comparison of phase scintillation reveals similarities but also
asymmetries of the ionospheric response in the northern and southern auroral zones, cusps and polar caps. In the nightside
auroral oval and in the cusp/cleft sectors the phase scintillation was observed in both hemispheres at about the same times and was correlated with geomagnetic activity. The
scintillation level was very similar in approximately conjugate locations in Qiqiktarjuaq (75.4° N; 23.4° E CGM lat.
and lon.) and South Pole (74.1° S; 18.9° E), in Longyearbyen (75.3° N; 111.2° E) and Zhongshan (74.7° S; 96.7° E), while it was significantly higher in Cambridge Bay (77.0° N; 310.1° E) than at Mario Zucchelli (80.0° S; 307.7° E). In the polar cap, when the interplanetary magnetic field (IMF) was
strongly northward, the ionization due to energetic particle precipitation was a likely cause of scintillation that was
stronger at Concordia (88.8° S; 54.4° E) in the dark ionosphere than in the sunlit ionosphere over Eureka (88.1° N; 333.4° E), due to a difference in ionospheric conductivity.
When the IMF tilted southward, weak or no significant scintillation was detected in the northern polar cap, while in the southern polar cap rapidly varying TEC and strong phase scintillation persisted for many hours. This interhemispheric asymmetry is explained by the difference in the location of solar terminator relative to the cusps in the Northern and Southern Hemisphere. Solar terminator was in the immediate proximity of the cusp in the Southern Hemisphere where sunlit ionospheric plasma was readily convected into the central
polar cap and a long series of patches was observed. In contrast, solar terminator was far poleward of the northern cusp thus reducing the entry of sunlit plasma and formation of dense patches. This is consistent with the observed and modeled seasonal variation in occurrence of polar cap
patches. The GPS scintillation and TEC data analysis is supported by data from ground-based networks of magnetometers, riometers, ionosondes, HF radars and all-sky imagers,
as well as particle flux measurements by DMSP satellites.
Description:
Published
Description:
2287-2304
Description:
1.7. Osservazioni di alta e media atmosfera
Description:
3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale
Description:
JCR Journal
Description:
open
Keywords:
Ionosphere (Ionospheric irregularities)
;
Magnetospheric physics (Storms and substorms)
;
Radio science (Space and satellite communication)
;
01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques
;
01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations
;
05. General::05.04. Instrumentation and techniques of general interest::05.04.99. General or miscellaneous
;
05. General::05.08. Risk::05.08.01. Environmental risk
Repository Name:
Istituto Nazionale di Geofisica e Vulcanologia (INGV)
Type:
article
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