Observational evidences for heating of the solar corona by nanoflares in the 
network derived from the transition region spectral lines

Rybak, J.; Kucera, A.; Curdt, W.; Wöhl, H.

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Observational evidences for heating of the solar corona by nanoflares in the network derived from the transition region spectral lines

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Curdt, W.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Rybak, J., Kucera, A., Curdt, W., & Wöhl, H. (2004). Observational evidences for heating of the solar corona by nanoflares in the network derived from the transition region spectral lines. In R. W. Walsh, J. Ireland, D. Danesy, & B. Fleck (Eds.), Proc. SOHO 15 - Coronal heating (pp. 529-534). Noordwijk: ESA Publ. Div.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-F1C3-C

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