Doppler redistribution of anisotropic radiation and resonance polarization in moving scattering media: Predicted results for the coronal Ovi 1032 Å line

Astronomy and Astrophysics

Volumn 445, Issue 2, 2006, Pages 681-692

  Sahal Brechot S ^a   Raouafi, N E ^b,c,d  

^a OBSERVATOIRE DE PARIS   (France)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^c NATIONAL SOLAR OBSERVATORY   (United States)

^d OBSERVATOIRE DE PARIS   (France)

Author keywords

Atomic processes; Line: formation; Line: profile; Polarization; Sun: corona; Sun: solar wind

Indexed keywords

ANISOTROPY; ELECTROMAGNETIC WAVE POLARIZATION; RADIATION EFFECTS; RESONANCE; SOLAR RADIATION; SUN;

ATOMIC PROCESSES; LINE; FORMATION; LINE; PROFILE; SUN: CORONA; SUN: SOLAR WIND;

DOPPLER EFFECT;

EID: 30144442642     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20052822     Document Type: Article

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