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

Feldman, U.; Dammasch, I. E.; Landi, E.; Doschek, G. A.

doi:10.1086/420964

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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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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: https://hdl.handle.net/11858/00-001M-0000-0014-F00D-0

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