A&A 428, 1017 (2004)
DOI: 10.1051/0004-6361:20040200e

Erratum

Dynamics and heating of the magnetic network on the Sun

Efficiency of mode transformation

S. S. Hasan¹ - P. Ulmschneider ²

1 - Indian Institute of Astrophysics, Bangalore-560034, India
2 - Institute für Theoretische Astrophysik, Tiergartenstr. 15, 69121 Heidelberg, Germany

A&A, 422, 1085-1091 (2004), DOI: 10.1051/0004-6361:20040200

Key words: Sun: chromosphere - Sun: magnetic fields - Sun: oscillations - errata, addenda

In Hasan & Ulmschneider (2004), we cited the work of McAteer et al. (2003) in the text, but inadvertently did not include it in the References. The omitted reference is:

McAteer, R. T. J., Gallagher, P. T., Williams, D. R., et al. 2003, ApJ, 587, 806