Analysis of power spectra of Doppler shift time series as a diagnostic tool for quiescent coronal loops

Astronomy and Astrophysics

Volumn 462, Issue 1, 2007, Pages 331-340

  Taroyan, Y ^a   Erdelyi R ^a   Doyle, J G ^b   Bradshaw, S J ^c  

^a UNIVERSITY OF SHEFFIELD   (United Kingdom)

^b ARMAGH OBSERVATORY   (United Kingdom)

^c IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Hydrodynamics; Line: profiles; Methods: analytical; Methods: numerical; Sun: corona; Sun: oscillations

Indexed keywords

GALAXIES; HYDRODYNAMICS; NUMERICAL METHODS; OBSERVATORIES; PLASMAS; TEMPERATURE DISTRIBUTION;

LINE: PROFILES; METHODS: ANALYTICAL; SUN: CORONA; SUN: OSCILLATIONS;

DOPPLER EFFECT;

EID: 33846538538     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066069     Document Type: Article

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