The solar cycle as seen by low-ℓ p-mode frequencies: Comparison with global and decomposed activity proxies

Monthly Notices of the Royal Astronomical Society

Volumn 352, Issue 4, 2004, Pages 1102-1108

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

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

Author keywords

Sun: activity; Sun: helioseismology; Sun: magnetic fields

Indexed keywords

DOPPLER VELOCITY; FREQUENCY COMPARISON; P-MODE FREQUENCY; SOLAR CYCLE; SOLAR DISK; SOLAR P-MODE FREQUENCIES; SUN: ACTIVITY; SUN: HELIOSEISMOLOGY; SUN:MAGNETIC FIELDS; SURFACE ACTIVITIES;

SOLAR ENERGY;

EID: 4344705456     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07998.x     Document Type: Article

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