EDP Sciences Journals List
Advanced Search
Free access article

Issue A&A
Volume 476, Number 2, December III 2007
Page(s) 951 - 957
Section The Sun
DOI http://dx.doi.org/10.1051/0004-6361:20078004



A&A 476, 951-957 (2007)
DOI: 10.1051/0004-6361:20078004

The statistical significance of the North-South asymmetry of solar activity revisited

M. Carbonell1, J. Terradas2, R. Oliver2, and J. L. Ballester2

1  Departament de Matemàtiques i Informàtica, Universitat de les Illes Balears, 07122 Palma de Mallorca, Spain
    e-mail: marc.carbonell@uib.es
2  Departament de Física, Universitat de les Illes Balears, 07122 Palma de Mallorca, Spain
    e-mail: [jaume.terradas;ramon.oliver;joseluis.ballester]@uib.es

(Received 4 June 2007 / Accepted 26 July 2007 )

Abstract
Aims.Many studies of the North-South asymmetry of solar activity and its features have been performed. However, most of these studies do not consider whether or not the asymmetry of the time series under consideration is statistically significant. If the asymmetry is statistically insignificant, any study about its behavior is meaningless. Here, we discuss the difficulties found when trying to assess the statistical significance of the North-South asymmetry (hereafter SSNSA) of the most usually considered time series of solar activity.
Methods.We distinguish between solar activity time series composed of integer or non-integer and dimensionless data, or composed of non-integer and dimensional data. For each of these cases, we discuss the most suitable statistical tests which can be applied and highlight the difficulties in obtaining valid information about the statistical significance of solar activity time series.
Results.Our results suggest that, apart from the need to apply suitable statistical tests, other effects such as data binning, the considered units and the need, in some tests, to consider groups of data, substantially affect the determination of the statistical significance of the asymmetry.
Conclusions.The assessment of the statistical significance of the N-S asymmetry of solar activity is difficult and an absolute answer cannot be given, since many different effects influence the results given by the statistical tests. The quantitative results about the statistical significance of the N-S asymmetry of solar activity provided by different authors, as well as studies of its behaviour, must be considered with care because they depend on the chosen values of different parameters or on the considered units.


Key words: Sun: activity -- methods: data analysis -- methods: statistical



© ESO 2007


What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.