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Line profile characteristics of solar explosive event bursts

MPS-Authors
/persons/resource/persons103979

Innes,  D. E.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104218

Solanki,  S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
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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Citation

Ning, Z., Innes, D. E., & Solanki, S. K. (2004). Line profile characteristics of solar explosive event bursts. Astronomy and Astrophysics, 419, 1141-1148. doi:10.1051/0004-6361:20034499.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-F007-B
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