Soft X-ray coronal spectra at low activity levels observed by RESIK

Astronomy and Astrophysics

Volumn 514, Issue 12, 2010, Pages

  Sylwester, B ^a   Sylwester, J ^a   Phillips, K J H ^b  

^a Polish Academy of Sciences ^*  (Poland)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Gamma rays; Sun: abundances; Sun: corona; Sun: X rays

Indexed keywords

ACTIVE REGIONS; ACTIVITY LEVELS; BRAGG CRYSTAL SPECTROMETER; CORONAL HEATING; CORONAS-F; DIFFERENTIAL EMISSION MEASURES; ELEMENT ABUNDANCES; EMISSION LINES; HIGH SENSITIVITY; HIGHLY-IONIZED; LINE INTENSITIES; PHYSICAL CONDITIONS; QUIET SUN; SOFT X-RAY; SOLAR ACTIVITY; SPECTRAL BAND; SPECTRAL RANGE; SUN: ABUNDANCES; TEMPERATURE STRUCTURE; WAVELENGTH RANGES; X-RAY EMISSION; X-RAY OBSERVATIONS;

ELECTROMAGNETIC WAVE EMISSION; ION BEAMS; SOLAR ENERGY; SPECTROMETERS; SPECTROMETRY; SUN; X RAY SCATTERING; X RAYS;

GAMMA RAYS;

EID: 77952977573     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912907     Document Type: Article

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