Low frequency geomagnetic field variations at Dome C (Antarctica)
Abstract. We conduct an analysis of the geomagnetic field variations recorded at the new Antarctic station Dome C, lo-cated very close to the geomagnetic pole, which has been op-erating for approximately one month during the 1999â2000 campaign. We also perform a comparison with simultane-ous measure...
| Main Authors: | , , , , , |
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| Other Authors: | |
| Format: | Text |
| Language: | English |
| Published: |
2002
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| Subjects: | |
| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.592.4997 http://hal.archives-ouvertes.fr/docs/00/32/92/47/PDF/angeo-21-923-2003.pdf |
| Summary: | Abstract. We conduct an analysis of the geomagnetic field variations recorded at the new Antarctic station Dome C, lo-cated very close to the geomagnetic pole, which has been op-erating for approximately one month during the 1999â2000 campaign. We also perform a comparison with simultane-ous measurements at the Italian Antarctic station Terra Nova Bay, in order to investigate the spatial extension of the phe-nomena observed at very high latitude. Our results show that between the two stations the daily variation is similar and the fluctuations with fâź1 mHz are coherent, provided that in both cases the comparison is made between geographically oriented components, suggesting that ionospheric currents related to the geographic position, more than field-aligned currents, are responsible for the lowest frequency variations; conversely, higher frequency (Pc5) fluctuations are substan-tially decoupled between the two stations. We also found that at Dome C the fluctuation power in the 0.55â6.7 mHz frequency band is well related with the solar wind speed dur-ing the whole day and that at Terra Nova Bay the correlation is also high, except around local geomagnetic noon, when the station approaches the polar cusp. These results indicate that the solar wind speed control of the geomagnetic field fluctu-ation power is very strict in the polar cap and less important close to the polar cusp. Key words. Magnetospheric physics (MHD waves and in-stabilities; Polar cap phenomena; Solar wind-magnetosphere interactions) 1 |
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