Century-scale persistence in longitude distribution in the Sun and in silico

Astronomy and Astrophysics

Volumn 429, Issue 3, 2005, Pages 1093-1096

  Pelt, J ^a,b   Tuominen, I ^b   Brooke, J ^c  

^a TARTU OBSERVATORY   (Estonia)

^b UNIVERSITY OF OULU   (Finland)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

Author keywords

Methods: statistical; Sun: activity; Sun: magnetic fields; Sun: sunspots

Indexed keywords

COMPUTER SIMULATION; DATA PROCESSING; MAGNETIC FIELD EFFECTS; PARAMETER ESTIMATION; RANDOM PROCESSES; STATISTICAL METHODS;

METHODS: STATISTICAL; SUN: ACTIVITY; SUN: MAGNETIC FIELDS; SUN: SUNSPOTS;

ASTROPHYSICS;

EID: 11844306020     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041357     Document Type: Article

References (5)

1. Bai, T. 2003, ApJ, 585, 1114
2. Berdyugina, S. V., & Usoskin, I. G. 2003, A&A, 1121
3. Jetsu, L., Pelt, J., & Tuominen, I. 1993, A&A, 278, 449
4. Tuominen, I., Berdyugina, S. V., & Korpi, M. J. 2002, AN, 323, 367
5. Usoskin, I. G. 2003, private communication