Options
The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude
Author(s)
Type
Conference paper
Language
English
Obiettivo Specifico
1A. Geomagnetismo e Paleomagnetismo
Status
Published
Conference Name
Issued date
June 27, 2005
Conference Location
Monte Porzio Catone
Publisher
Società Astronomica Italiana
Keywords
Abstract
We study ULF geomagnetic field fluctuations detected on October 29-31, 2003,
when the Earth’s arrival of solar wind CMEs produced major geomagnetic storms; these
solar wind structures are characterized by extremely high plasma speed and long-duration
intervals with northward interplanetary magnetic field. The analyzed geomagnetic field data
are from four high latitude stations (three in Antarctica), located deep in the polar cap. The
analysis is extended also to low latitude European stations, in order to discriminate between local and global magnetospheric phenomena.
when the Earth’s arrival of solar wind CMEs produced major geomagnetic storms; these
solar wind structures are characterized by extremely high plasma speed and long-duration
intervals with northward interplanetary magnetic field. The analyzed geomagnetic field data
are from four high latitude stations (three in Antarctica), located deep in the polar cap. The
analysis is extended also to low latitude European stations, in order to discriminate between local and global magnetospheric phenomena.
File(s)
Loading...
Name
mem_salt_lepidi.pdf
Description
main article
Size
546.78 KB
Format
Adobe PDF
Checksum (MD5)
7a3cc9dc161898f06b08ce3fbd32afc4