Enhancement of the helium resonance lines in the solar atmosphere by suprathermal electron excitation - II. Non-Maxwellian electron distributions

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 1, 2003, Pages 143-163

  Smith, G R ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Line: Formation; Radiative transfer; Sun: Transition region; Sun: UV radiation

Indexed keywords

DISTRIBUTION FUNCTIONS; ELECTRONS; HELIUM; RESONANCE; ULTRAVIOLET SPECTROSCOPY;

COLLISIONAL EXCITATION; ELECTRON DISTRIBUTIONS; LINE FORMATIONS; LINE INTENSITIES; MODEL ATMOSPHERE; RESONANCE LINE; SUN:TRANSITION REGION; SUN:UV RADIATION; TRANSITION REGION LINE; TRANSITION REGIONS;

RADIATIVE TRANSFER;

EID: 0142087568     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06362.x     Document Type: Article

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