Principal Component Analysis of the Solar Magnetic Field I: The Axisymmetric Field at the Photosphere
- 1 November 2004
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 225 (1) , 1-19
- https://doi.org/10.1007/s11207-004-3257-2
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Impulses of activity and the Solar cycleSolar Physics, 2003
- Turbulence, Coherent Structures, Dynamical Systems and SymmetryPublished by Cambridge University Press (CUP) ,1996
- Singular Spectrum AnalysisPublished by Springer Nature ,1996
- Double magnetic cycle of solar activitySolar Physics, 1995
- Unique determination of model coronal magnetic fields using photospheric observationsSolar Physics, 1993
- A Use's Guide to Principal ComponentsPublished by Wiley ,1991
- PIPs and POPs: The reduction of complex dynamical systems using principal interaction and oscillation patternsJournal of Geophysical Research: Atmospheres, 1988
- Time Evolution of the Large-Scale Solar Magnetic FieldSymposium - International Astronomical Union, 1971