High-precision density measurements in the solar corona: I. analysis methods and results for Fe XII and Fe XIII

Astronomy and Astrophysics

Volumn 495, Issue 2, 2009, Pages 587-606

  Young, P R ^a,b,c   Watanabe, T ^d   Hara, H ^d   Mariska, J T ^c  

^a RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^b GEORGE MASON UNIVERSITY   (United States)

^c NAVAL RESEARCH LABORATORY   (United States)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Sun: corona; Sun: UV radiation

Indexed keywords

ATOMS; BLENDING; ELECTROCHEMICAL CORROSION; ELECTROCHEMICAL IMPEDANCE SPECTROSCOPY; EXTRATERRESTRIAL ATMOSPHERES; MODELS; ULTRAVIOLET RADIATION;

ACTIVE REGIONS; ANALYSIS METHODS; ATOMIC MODELS; DATA ANALYSIS; DATA-SETS; DENSITY MEASUREMENTS; DOMINANT FACTORS; EIS MEASUREMENTS; ELECTRON NUMBER DENSITIES; EMISSION LINES; FIT PARAMETERS; HIGH PRECISION; HIGH SENSITIVITIES; HIGH-DENSITY LIMITS; IMAGING SPECTROMETERS; LINE FITTINGS; SOLAR CORONAS; SPECIFIC PROBLEMS; SUN: CORONA; SUN: UV RADIATION; TWO ACTIVE REGIONS;

SUN;

EID: 61349134112     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810143     Document Type: Article

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