| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1777256 | Journal of Atmospheric and Solar-Terrestrial Physics | 2011 | 5 Pages |
Abstract
Results obtained for the three data sets are used to derive a theoretical (continuous) probability distribution function (PDF) by fitting the histograms representing the percentage of events against the intervals of magnetic index. PDFs allow estimation of the probability of a given level of geomagnetic activity to be reached after the detection, by in situ solar wind observations, of a given interplanetary structure approaching the Earth.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
M.V. Alves, E. Echer, W.D. Gonzalez,