A&A 428, 1017-1017 (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 and P. Ulmschneider21 Indian Institute of Astrophysics, Bangalore-560034, India
e-mail: hasan@iiap.res.in
2 Institute für Theoretische Astrophysik, Tiergartenstr. 15, 69121 Heidelberg, Germany
e-mail: ulm@ita.uni-heidelberg.de
Erratum of A&A 422 p. 1085
Abstract
A&A, 422, 1085-1091 (2004), DOI: 10.1051/0004-6361:20040200
Key words: Sun: chromosphere -- Sun: magnetic fields -- Sun: oscillations -- errata, addenda
© ESO 2004
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