Emission lines of Fe x in active region spectra obtained with the Solar Extreme-ultraviolet Research Telescope and Spectrograph

Monthly Notices of the Royal Astronomical Society

Volumn 389, Issue 2, 2008, Pages 939-948

  Keenan, F P ^a   Jess, D B ^a   Aggarwal, K M ^a   Thomas, R J ^b   Brosius, J W ^b,c   Davila, J M ^b  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c CATHOLIC UNIVERSITY OF AMERICA   (United States)

Author keywords

Atomic data; Sun: activity; Sun: corona

Indexed keywords

CARRIER CONCENTRATION; ELECTROMAGNETIC WAVE EMISSION; ELECTRON DENSITY MEASUREMENT; ELECTRONS; IMPACT IONIZATION; SOLAR ENERGY; SPECTROGRAPHS;

ACTIVE REGIONS; ATOMIC DATA; EMISSION LINES; EXTREME ULTRAVIOLET; FULLY RELATIVISTIC CALCULATIONS; LINE RATIOS; RADIATIVE RATES; SPECTRA'S; SUN : CORONA; SUN: ACTIVITY;

TELESCOPES;

EID: 51149105677     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13615.x     Document Type: Article

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