Sunspot group tilt angles and the strength of the solar cycle (Corrigendum)

M. Dasi-Espuig; S. K. Solanki; N. A. Krivova; R. Cameron; T. Peñuela

doi:10.1051/0004-6361/201014301e

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Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 556, August 2013


Article Number		C3
Number of page(s)		1
Section		The Sun
DOI		https://doi.org/10.1051/0004-6361/201014301e
Published online		05 August 2013

A&A 556, C3 (2013)

Sunspot group tilt angles and the strength of the solar cycle (Corrigendum)

M. Dasi-Espuig¹, S. K. Solanki¹^,2, N. A. Krivova¹, R. Cameron¹ and T. Peñuela¹^,3

¹ Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
e-mail: dasi@mps.mpg.de
² School of Space Research, Kyung Hee University, Yongin, 446-701 Gyeonggi, Korea
³ Astronomical Institute, St. Petersburg State University, Russia

This article has no abstract.

Key words: sunspots / Sun: dynamo / magnetic fields / Sun: activity / errata, addenda

Erratum to: A&A 518, A7 (2010), DOI: 10.1051/0004-6361/201014301

© ESO, 2013

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