Even moderate geomagnetic pulsations can cause fluctuations of <i>fo</i>F2 frequency of the auroral ionosphere
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Published:2021-06-16
Issue:3
Volume:39
Page:549-562
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ISSN:1432-0576
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Container-title:Annales Geophysicae
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language:en
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Short-container-title:Ann. Geophys.
Author:
Yagova Nadezda, Kozlovsky AlexanderORCID, Fedorov EvgenyORCID, Kozyreva OlgaORCID
Abstract
Abstract. The ionosonde at the Sodankylä Geophysical Observatory (SOD; 67∘ N,
27∘ E; Finland) routinely performs vertical sounding once per
minute which enables the study of fast ionospheric variations at a
frequency of the long-period geomagnetic pulsations Pc5–6/Pi3
(1–5 mHz). Using the ionosonde data from April 2014–December
2015 and colocated geomagnetic measurements, we have investigated
a correspondence between the magnetic field pulsations and
variations of the critical frequency of radio waves reflected from
the ionospheric F2 layer (foF2). For this study, we have developed
a technique for automated retrieval of the critical frequency of
the F2 layer from ionograms. As a rule, the Pc5–6/Pi3 frequency
band fluctuations in foF2 were observed at daytime during quiet or
moderately disturbed space weather conditions. In most cases
(about 80 %), the coherence between the foF2 variations and
geomagnetic pulsations was low. However in some cases (specified
as “coherent”) the coherence was as large as γ2≥0.5.
The following conditions are favorable for the occurrence of
coherent cases: enhanced auroral activity (6 h maximal auroral electrojet (AE)
≥800 nT), high solar wind speed (V>600 km/s), fluctuating
solar wind pressure and northward interplanetary magnetic field.
In the cases when the coherence was higher at shorter periods of
oscillations, the magnetic pulsations demonstrated features
typical for the Alfvén field line resonance.
Publisher
Copernicus GmbH
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geology,Astronomy and Astrophysics
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