Comment on the existence of a long range correlation in the geomagnetic disturbance storm time (Dst) index

Details Comment on the existence of a long range correlation in the geomagnetic disturbance storm time (Dst) index Comment on the existence of a long range correlation in the geomagnetic disturbance storm time (Dst) index

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.337...21l&link_type=abstract

Astrophysics and Space Science, Volume 337, Issue 1, pp.21-22

Astronomy and Astrophysics

Astrophysics

Solar-Terrestrial Relations, Solar Wind

Scientific paper

Very recently (Banerjee et al. in Astrophys. Space, doi:10.1007/s10509-011-0836-1, 2011) the statistics of geomagnetic Disturbance storm (Dst) index have been addressed, and the conclusion from this analysis suggests that the underlying dynamical process can be modeled as a fractional Brownian motion with persistent long-range correlations. In this comment we expose several misconceptions and flaws in the statistical analysis of that work. On the basis of these arguments, the former conclusion should be revisited.

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