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Lacasa Saiz de Arce, Lucas (2011). Comment on the existence of a long range correlation in the geomagnetic disturbance storm time (Dst) index. "Astrophysics And Space Science", v. 337 (n. 1); pp. 21-22. ISSN 0004-640X. https://doi.org/10.1007/s10509-011-0926-0.
Title: | Comment on the existence of a long range correlation in the geomagnetic disturbance storm time (Dst) index |
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Author/s: |
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Item Type: | Article |
Título de Revista/Publicación: | Astrophysics And Space Science |
Date: | January 2011 |
ISSN: | 0004-640X |
Volume: | 337 |
Subjects: | |
Freetext Keywords: | Solar-terrestrial relations, Solar wind |
Faculty: | E.T.S.I. Aeronáuticos (UPM) |
Department: | Matemática Aplicada y Estadística [hasta 2014] |
Creative Commons Licenses: | Recognition - No derivative works - Non commercial |
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Very recently (Banerjee et al. in Astrophys. Space, doi: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.
Item ID: | 16704 |
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DC Identifier: | https://oa.upm.es/16704/ |
OAI Identifier: | oai:oa.upm.es:16704 |
DOI: | 10.1007/s10509-011-0926-0 |
Official URL: | http://link.springer.com/article/10.1007%2Fs10509-... |
Deposited by: | Memoria Investigacion |
Deposited on: | 14 Nov 2014 17:57 |
Last Modified: | 14 Nov 2014 17:57 |