Please use this identifier to cite or link to this item:
AuthorsCafarella, L.* 
Di Mauro, D.* 
Lepidi, S.* 
Meloni, A.* 
TitleGeomagnetic Observatories in Antarctica; State of the Art and a Perspective View in the Global and Regional Frameworks
Other TitlesAn Overview in the IPY Perspective
Issue DateNov-2008
KeywordsGeomagnetic observatories
Secular variation
Subject Classification01. Atmosphere::01.03. Magnetosphere::01.03.99. General or miscellaneous 
04. Solid Earth::04.05. Geomagnetism::04.05.02. Geomagnetic field variations and reversals 
04. Solid Earth::04.05. Geomagnetism::04.05.08. Instruments and techniques 
AbstractThe Earth is immersed in a planetary magnetic field. The field is generated in the Earth’s core and can be measured at its surface. It shows mainly a typical dipolar profile with the dipole axis roughly parallel to the Earth’s rotation axis (tilting about 12°). At low latitudes the field reaches its minimum, while its maximum intensity is observable in polar regions, reaching there almost three times its equatorial value. The region around the Earth where the geomagnetic field extends is known as the Earth’s magnetosphere. This region contains a very low density gas of electrically charged particles and is the space around the Earth where many electric and magnetic phenomena happen.
Appears in Collections:Book chapters

Files in This Item:
File Description SizeFormat 
Cafarella_book_Capra.pdfmain article4.12 MBAdobe PDFView/Open
Show full item record

Page view(s)

Last Week
Last month
checked on Jul 24, 2017


checked on Jul 24, 2017

Google ScholarTM