Geomagnetic consequences of the solar flares during the last Hale solar cycle (II)

Details Geomagnetic consequences of the solar flares during the last Hale solar cycle (II) Geomagnetic consequences of the solar flares during the last Hale solar cycle (II)

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..451m&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Computer Science

Geomagnetic Field, Solar Flares

Scientific paper

The effects of the solar energetic phenomena cover the entire terrestrial environment, from the outer atmospheric layer to the ground. The energy source of all these geomagnetic disturbances is the solar plasma that may originate from solar eruptive phenomena that take their energy from magnetic field of the Sun. This paper is part of a larger study concerning the geomagnetic effects produced by solar phenomena. We analyze the cyclic variability of solar flares (registered in Hα and X-ray) and compare it with the variations of some geomagnetic indices (aa index and the number of sudden storm commencements (SSCs)) for the last Hale cycle. The solar cycles 22 and 23 are different in the level of flare activity and in the slope and the duration of their ascending branch.

Affiliated with

Also associated with

No associations

Rating

Geomagnetic consequences of the solar flares during the last Hale solar cycle (II) 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 Geomagnetic consequences of the solar flares during the last Hale solar cycle (II), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geomagnetic consequences of the solar flares during the last Hale solar cycle (II) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-780346