Source of excitation of low-ℓ solar p modes: Characteristics and solar-cycle variations

Monthly Notices of the Royal Astronomical Society

Volumn 314, Issue 1, 2000, Pages 75-86

  Chaplin, W J ^a,b   Appourchaux, T ^a   Elsworth, Y ^b   Isaak, G R ^b   Miller, B A ^b   New, R ^c  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^c SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

Author keywords

Convection; Methods: data analysis; Sun: activity; Sun: granulation; Sun: oscillations

Indexed keywords

SOLAR ENERGY;

BIRMINGHAM; CONVECTION; METHODS. DATA ANALYSIS; MODE CHARACTERISTICS; SOLAR CYCLE VARIATIONS; SOLAR OSCILLATIONS; SOLAR P MODES; SUN: ACTIVITY; SUN: GRANULATION; SUN: OSCILLATIONS;

ACOUSTIC FIELDS;

EID: 0005678581     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03335.x     Document Type: Article

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