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

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.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-F00D-0 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-F00E-E

Genre: Journal Article

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Feldman, U., Author
Dammasch, I. E.¹, Author
Landi, E., Author
Doschek, G. A., Author

Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291

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MPIS_GROUPS: Sun and Heliosphere

MPIS_PROJECTS: SOHO: SUMER

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Dates: Date issued: 2004

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1086/420964
BibTex Citekey: Feldman:2004-070

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Title: Astrophysical Journal

Source Genre: Journal

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Pages: - Volume / Issue: 609 Sequence Number: - Start / End Page: 439 - 451 Identifier: -