The onset of solar cycle 24: What global acoustic modes are telling us

Astronomy and Astrophysics

Volumn 504, Issue 1, 2009, Pages

  Salabert, D ^a,b   Garcia R A ^c   Palle P L ^a,b   Jimenez Reyes S J ^a,b  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD DE LA LAGUNA   (Spain)

^c UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

Methods: Data analysis; Sun: Activity; Sun: Helioseismology

Indexed keywords

ACOUSTIC MODE; FITTING METHOD; FREQUENCY SHIFT; HELIOSEISMIC; METHODS: DATA ANALYSIS; MULTI-STEP; P-MODE FREQUENCY; SIGNIFICANT SURFACES; SOLAR ACTIVITY CYCLES; SOLAR CYCLE; SOLAR MAGNETIC FIELDS; SOLAR P-MODE FREQUENCIES; SOLAR SURFACES; SPACE-BASED; SPATIAL DISTRIBUTION; SUN: ACTIVITY; SUN: HELIOSEISMOLOGY; TEMPORAL VARIATION;

FREQUENCY SHIFT KEYING; MAGNETIC FIELDS; SIZE DISTRIBUTION; SOLAR ENERGY; SUN; UPPER ATMOSPHERE;

MAXIMUM LIKELIHOOD ESTIMATION;

EID: 70149107854     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912736     Document Type: Article

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