The longitudinal polar cusp displacement from geomagnetic measurements in Antarctica

We used ULF geomagnetic field measurements in the Pc5 frequency range (1.7-7 mHz) attwo Antarctic stations to statistically investigate the longitudinal location of the polar cusp.The two stations are located at the same geomagnetic latitude, ~80° S (just poleward of thecusp), and are separated by o...

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Bibliographic Details
Published in:Annals of Geophysics
Main Authors: Marzocchetti, Martina, Lepidi, Stefania, Francia, Patrizia, Cafarella, Lili, Di Mauro, Domenico
Format: Article in Journal/Newspaper
Language:English
Published: Istituto Nazionale di Geofisica e Vulcanologia, INGV 2019
Subjects:
Magnetospheric physics
Structure and dynamics
Geomagnetic field variations and reversals
Solar-terrestrial interaction
Space weather
Antarctic
Antarc*
Antarctica
Online Access:https://www.annalsofgeophysics.eu/index.php/annals/article/view/7779
https://doi.org/10.4401/ag-7779
Description
Summary:We used ULF geomagnetic field measurements in the Pc5 frequency range (1.7-7 mHz) attwo Antarctic stations to statistically investigate the longitudinal location of the polar cusp.The two stations are located at the same geomagnetic latitude, ~80° S (just poleward of thecusp), and are separated by one hour in magnetic local time. Since at each station the Pc5power maximizes when the station approaches the cusp, the comparison between their Pc5power allows to estimate the longitudinal position of the cusp and to examine its movements.We found that there is a displacement of the cusp depending on interplanetary conditions;in particular, the cusp shifts to later hours for negative values of the interplanetary magneticfield and solar wind velocity east-west components (By and Vy), while moves to earlier hoursfor positive values of Vy. Conversely, no dependence of the cusp longitudinal position onpositive By values nor on the interplanetary magnetic field north-south component (Bz) emerges.

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