Astronomy and Astrophysics – Astronomy
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...660.1674f&link_type=abstract
The Astrophysical Journal, Volume 660, Issue 2, pp. 1674-1682.
Astronomy and Astrophysics
Astronomy
8
Plasmas, Sun: Corona
Scientific paper
In the present paper we use UV lines emitted by He-like ions as a tool to test the presence of nonthermal high-energy electrons and to quantify their number and energy. The He-like lines we consider are the He-like 1s2s3S-1s2p3P lines observed in the UV, and their use capitalizes on the high excitation energies for the 1s2p3P levels and on the near-unity ion abundances of the He-like ions for large temperature ranges. We investigate the presence of nonthermal high-energy electrons in solar active regions, placing upper limits on the presence of electrons capable of exciting the upper levels of Ne IX, Mg XI, and Si XIII.
Doschek George A.
Feldman Uri
Landi Enrico
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