Nonlinear deconvolution with deblending: A new analyzing technique for spectroscopy

Astronomy and Astrophysics

Volumn 507, Issue 3, 2009, Pages 1711-1718

  Sennhauser, C ^a   Berdyugina, S V ^a,b   Fluri, D M ^a  

^a ETH ZURICH   (Switzerland)

^b KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

Author keywords

Line: formation; Stars: magnetic fields

Indexed keywords

ABSORPTION LINES; ATOMIC TRANSITION; CALCULATION TIME; DOPPLER IMAGING; INDIVIDUAL COMPONENTS; LEAST SQUARE; LINE BROADENING; LINE PATTERN; LINE PROFILES; LINE: FORMATION; MEAN LINE; MOLECULAR BAND; NON-LINEARITY; PRINCIPLE COMPONENT ANALYSIS; SPECTRAL LINE; SPECTROPOLARIMETRY; SPECTROSCOPY DATA;

BLENDING; CONVOLUTION; MAGNETIC FIELDS; NONLINEAR ANALYSIS; SIGNAL TO NOISE RATIO; STARS;

ATOMIC SPECTROSCOPY;

EID: 70849129785     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912467     Document Type: Article

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