Physics
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..427d&link_type=abstract
In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:
Physics
Earth Magnetosphere, Solar Wind, Solar-Terrestrial Relations
Scientific paper
The energy release during magnetospheric substorms in response to solar wind changes consists of two main physical processes: the directly-driven and the unloading processes. Recent analysis on the sporadic activity related to the unloading process seems to indicate that the magnetospheric response to solar wind changes might resemble the behaviour of solar wind changes might resemble the behaviour of an out-of-equilibrium system near a marginally stable point (critical point). Here, we present a modified version of the well-known forest-fire cellular automation (FFM) not quasistatically driven for the sporadic activity of the energy release in the geotail regions as revealed by the auroral electrojet index.
Consolini Giuseppe
de Michelis Paola
No associations
LandOfFree
A revised forest fire model non-quasistatically driven for the sporadic activity of the Earth's magnetotail 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 A revised forest fire model non-quasistatically driven for the sporadic activity of the Earth's magnetotail, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A revised forest fire model non-quasistatically driven for the sporadic activity of the Earth's magnetotail will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-780336