By Topic

The solar and interplanetary causes of space storms in solar cycle 23

Sign In

Cookies must be enabled to login.After enabling cookies , please use refresh or reload or ctrl+f5 on the browser for the login options.

Formats Non-Member Member
$31 $13
Learn how you can qualify for the best price for this item!
Become an IEEE Member or Subscribe to
IEEE Xplore for exclusive pricing!
close button

puzzle piece

IEEE membership options for an individual and IEEE Xplore subscriptions for an organization offer the most affordable access to essential journal articles, conference papers, standards, eBooks, and eLearning courses.

Learn more about:

IEEE membership

IEEE Xplore subscriptions

2 Author(s)
Bothmer, V. ; Max-Planck-Inst. fur Aeronomie, Katlenburg-Lindau, Germany ; EU-INTAS-ESA Team

This paper presents a brief overview on the results of a joint EU-INTAS-ESA project, which is focused on the investigation of the interplanetary and solar causes of geomagnetic storms in solar cycle 23. Based on the in situ data of the solar wind plasma and magnetic field parameters measured by the Wind and ACE (Advanced Composition Explorer) spacecraft, in joint analysis with the unprecedented set of remote sensing observations provided by the SOHO (Solar and Heliospheric Observatory) satellite since its launch in December 1995, the main statistical results from the detailed investigation of geomagnetic disturbed days with Ap>20 are presented here.

Published in:

Plasma Science, IEEE Transactions on  (Volume:32 ,  Issue: 4 )