Vector magnetic fields in prominences - III: HeI D3 Stokes profile analysis for quiescent and eruptive prominences

Solar Physics

Volumn 89, Issue 1, 1983, Pages 3-30

  Athay, R Grant ^a   Querfeld, Charles W ^a   Smartt, Raymond N ^b   Landi Degl'innocenti, Egidio ^c   Bommier, Veronique ^d  

^a National Center for Atmospheric Research   (France)

^b Sacramento Peak Observatory ^*  (France)

^c UNIVERSITY OF FLORENCE   (Italy)

^d OBSERVATOIRE DE PARIS   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0002897173     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/BF00211948     Document Type: Article

References (20)

1. A Model of the Chromosphere from the Helium and Continuum Emissions.
2. Fluid motions the solar chromosphere-corona transition region. II Active region flows in C IV from narrow slit Dopplergrams
3. Fluid motions in the solar chromosphere-corona transition region. III - Active region flows from wide slit Dopplergrams