The sensitivity of the C I 538.0 nm Fe I 537.9 nm and Ti II 538.1 nm lines to solar active regions

Astronomy and Astrophysics

Volumn 427, Issue 1, 2004, Pages 345-351

  Penza, V ^a   Caccin, B ^b   Del Moro, D ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b UNIVERSITY OF ROME TOR VERGATA   (Italy)

Author keywords

Radiative transfer; Sun: activity; Sun: atmosphere; Sun: faculae, plages

Indexed keywords

IRON; MAGNETIC FIELD EFFECTS; PERTURBATION TECHNIQUES; SOLAR RADIATION; SUN; TELESCOPES; TITANIUM; ULTRAVIOLET RADIATION;

MAGNETIC CYCLES; PHOTOSPHERE; STELLAR GLOBAL PARAMETERS;

ASTROPHYSICS;

EID: 8644252750     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041151     Document Type: Article

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