Title of article
Elliptical magnetic clouds and geomagnetic storms
Author/Authors
Antoniadou، نويسنده , , I. and Geranios، نويسنده , , A. and Vandas، نويسنده , , M. and Panagopoulou، نويسنده , , M. and Zacharopoulou، نويسنده , , O. and Malandraki، نويسنده , , O.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2008
Pages
9
From page
492
To page
500
Abstract
Magnetic clouds are simple phenomena which modulate the interplanetary space and they are a subset of Interplanetary Coronal Mass Ejections. Due to the sustained orientation of their magnetic fields south- and northwards, they can influence the Earthʹs magnetosphere and may give rise to geomagnetic storms. Since such storms are dominant factors of space weather predictions, magnetic clouds are an important factor in this domain. We analyzed six observed magnetic clouds triggered a geomagnetic storm and simulate them in order to identify their characteristics, such as probable shapes, orientation of their axis, duration, etc. geomagnetic storms triggered by these clouds are investigated by their Dst indices.
Keywords
Magnetic clouds , Geomagnetic storms , solar wind , Interplanetary magnetic field
Journal title
PLANETARY AND SPACE SCIENCE
Serial Year
2008
Journal title
PLANETARY AND SPACE SCIENCE
Record number
2309452
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