The hot prominence periphery in EUV lines

Details The hot prominence periphery in EUV lines The hot prominence periphery in EUV lines

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...334..280d&link_type=abstract

Astronomy and Astrophysics, v.334, p.280-288 (1998)

Astronomy and Astrophysics

Astrophysics

23

Sun: Prominences, Sun: Uv Radiation

Scientific paper

Two sets of He I and metallic lines were observed with the EUV spectrograph SUMER in a quiescent prominence. H, He, and Ca II lines were observed simultaneously with both German telescopes on Tenerife. The visible lines from elements with different atomic weights yield thermal and non-thermal broadening parameters of 7500 <= Tkin <= 8000 K and 2.5

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