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  5. The Earth's passage of the April 11, 1997 coronal ejecta: geomagnetic field fluctuations at high and low latitude during northward interplanetary magnetic field conditions
 
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The Earth's passage of the April 11, 1997 coronal ejecta: geomagnetic field fluctuations at high and low latitude during northward interplanetary magnetic field conditions

Author(s)
Lepidi, S.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Francia, P.  
Dipartimento di Fisica, Università dell'Aquila, L'Aquila, Italy  
Villante, U.  
Dipartimento di Fisica, Università dell'Aquila, L'Aquila, Italy  
Meloni, A.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Lazarus, A. J.  
Center for Space Research, MIT, Cambridge, USA  
Lepping, R. P.  
Laboratory for Extraterrestrial Physics, NASA/GSFC, Greenbelt, USA  
Language
English
Status
Published
JCR Journal
N/A or not JCR
Peer review journal
Yes
Journal
Annales Geophysicae  
Issue/vol(year)
10 / 17 (1999)
Publisher
EGS - Springer-Verlag
Pages (printed)
1245-1250
Date Issued
1999
URI
https://www.earth-prints.org/handle/2122/3934
Subjects
01. Atmosphere::01.03. Magnetosphere::01.03.99. General or miscellaneous  
01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamics  
Subjects

Magnetospheric physic...

MHD waves and instabi...

Solar wind-magnetosph...

Abstract
An analysis of the low frequency geomagnetic
field fluctuations at an Antarctic (Terra Nova Bay) and a low latitude (L'Aquila, Italy) station during the Earth's passage of a coronal ejecta on April 11, 1997 shows that major solar wind pressure variations were
followed at both stations by a high fluctuation level. During northward interplanetary magnetic field conditions and when Terra Nova Bay is close to the local
geomagnetic noon, coherent fluctuations, at the same frequency (3.6 mHz) and with polarization characteristics indicating an antisunward propagation, were observed simultaneously at the two stations. An analysis of simultaneous measurements from geosynchronous satellites shows evidence for pulsations at approximately the same frequencies also in the magnetospheric field.
The observed waves might then be interpreted as oscillation modes, triggered by an external stimulation, extending to a major portion of the Earth's magnetosphere.
References
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