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Observations indicating that ≈ 1 × 107 K solar flare plasmas may be produced in situ from ≈ 1 × 106 K coronal plasma

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http://pubman.mpdl.mpg.de/cone/persons/resource/persons103878

Dammasch,  I. E.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Feldman, U., Dammasch, I. E., Landi, E., & Doschek, G. A. (2004). Observations indicating that ≈ 1 × 107 K solar flare plasmas may be produced in situ from ≈ 1 × 106 K coronal plasma. Astrophysical Journal, 609, 439-451. doi:10.1086/420964.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-F00D-0
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