Geoefficiency of solar eruptive events

Details Geoefficiency of solar eruptive events Geoefficiency of solar eruptive events

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49.1113b&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 8, pp.1113-1114

Physics

Scientific paper

The sources of geomagnetic disturbances during 1999-2003 are discussed. The relation between geomagnetic activity and the rate of coronal mass ejections (CMEs), their parameters, and the dynamics of solar photospheric magnetic fields is considered. It is shown that during the reorganization of unipolar regions of the photospheric magnetic field, the number of CMEs increases and their parameters change. The geomagnetic disturbance level also increases in these periods.

Affiliated with

Also associated with

No associations

Rating

Geoefficiency of solar eruptive events does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Geoefficiency of solar eruptive events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geoefficiency of solar eruptive events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1887457