Issue |
A&A
Volume 428, Number 3, December IV 2004
|
|
---|---|---|
Page(s) | 1017 - 1017 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20040200e | |
Published online | 07 December 2004 |
Dynamics and heating of the magnetic network on the Sun
Efficiency of mode transformation
1
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
This article has no abstract.
Key words: Sun: chromosphere / Sun: magnetic fields / Sun: oscillations / errata, addenda
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.