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Solar wind isotopic abundance ratios of Ne, Mg, and Si measured by SOHO/CELIAS/MTOF as diagnostic tool for the inner corona

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons103998

Kallenbach,  R.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons103939

Grünwaldt,  H.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons103964

Hilchenbach,  M.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Kallenbach, R., Ipavich, F. M., Kucharek, H., Bochsler, P., Galvin, A. B., Geiss, J., et al. (1999). Solar wind isotopic abundance ratios of Ne, Mg, and Si measured by SOHO/CELIAS/MTOF as diagnostic tool for the inner corona. Physics and Chemistry of the Earth, 24C(4), 415-419.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-DAE7-0
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