The chaotic solar cycle - II. Analysis of cosmogenic 10Be data
暂无分享,去创建一个
I. Skokić | A. Hanslmeier | F. Steinhilber | R. Braǰsa | I. Skokić | A. Hanslmeier | C. MacLeod | B. Vršnak | J. Čalogović | F. Steinhilber | B. Vršnak | R. Brajša | C. L. MacLeod | J. Čalogović | D. Ruždjak | Ž. Ivezić | D. Ruždjak | Ž. Ivezić
[1] P. R. Wilson. Solar and stellar activity cycles , 1994 .
[2] Brandon C. Kelly,et al. Are the Variations in Quasar Optical Flux Driven by Thermal Fluctuations , 2009 .
[3] J. Zirker. The Magnetic Universe , 2009 .
[4] N. Sheeley,et al. The rotation of photospheric magnetic fields: A random walk transport model , 1994 .
[5] Press,et al. Class of fast methods for processing irregularly sampled or otherwise inhomogeneous one-dimensional data. , 1995, Physical review letters.
[6] Christophe Letellier,et al. The Symmetry of Chaos , 2007 .
[7] T. Schreiber. Interdisciplinary application of nonlinear time series methods , 1998, chao-dyn/9807001.
[8] E. Spiegel. Chaos and Intermittency in the Solar Cycle , 2009 .
[9] R. Braǰsa,et al. On the 24-day period observed in solar flare occurrence , 2004 .
[10] R. Leighton. Transport of Magnetic Fields on the Sun. , 1964 .
[11] Usa,et al. QUANTIFYING QUASAR VARIABILITY AS PART OF A GENERAL APPROACH TO CLASSIFYING CONTINUOUSLY VARYING SOURCES , 2009, 0909.1326.
[12] C. Fröhlich,et al. Total solar irradiance during the Holocene , 2009 .
[13] A. Wolfendale,et al. Secular solar and geomagnetic variations in the last 10,000 years. Proceedings at the NATO Advanced Research Workshop, held at Durham, England, 6 - 10 April 1987. , 1988 .
[14] M. Ossendrijver,et al. The solar dynamo , 2003 .
[15] W. Press,et al. Interpolation, realization, and reconstruction of noisy, irregularly sampled data , 1992 .
[16] J. Beer,et al. Large variations in Holocene solar activity: Constraints from 10Be in the Greenland Ice Core Project ice core , 2006 .
[17] P. Hoyng. Mean Field Dynamo Theory , 1992 .
[18] Oded Regev,et al. Chaos and complexity in astrophysics , 2007, 0705.2251.
[19] L. Ma. Thousand-Year Cycle Signals in Solar Activity , 2007 .
[20] M. Schüssler,et al. Theoretical Models of Solar Magnetic Variability , 2004 .
[21] S. Solanki,et al. Unusual activity of the Sun during recent decades compared to the previous 11,000 years , 2004, Nature.
[22] Manfred Morari,et al. False-nearest-neighbors algorithm and noise-corrupted time series , 1997 .
[23] C. Torrence,et al. A Practical Guide to Wavelet Analysis. , 1998 .
[24] T. Deeming. Fourier analysis with unequally-spaced data , 1975 .
[25] A. Kosovichev,et al. Application of Data Assimilation Method for Predicting Solar Cycles , 2008 .
[26] S. Solanki,et al. On the common solar signal in different cosmogenic isotope data sets , 2009 .
[27] Stefano Sello,et al. Solar cycle forecasting: A nonlinear dynamics approach , 2001 .
[28] D. Sokoloff,et al. Solar Grand Minima and Random Fluctuations in Dynamo Parameters , 2008, 0806.3331.
[29] A. Ruzmaikin,et al. Radiocarbon evidence of the global stochasticity of solar activity , 1990 .
[30] H. Abarbanel,et al. Determining embedding dimension for phase-space reconstruction using a geometrical construction. , 1992, Physical review. A, Atomic, molecular, and optical physics.
[31] K. Mccracken. Geomagnetic and atmospheric effects upon the cosmogenic 10Be observed in polar ice , 2004 .
[32] William H. Press,et al. The Time Delay of Gravitational Lens 0957+561. I. Methodology and Analysis of Optical Photometric Data , 1992 .
[33] J. Beer,et al. Interplanetary magnetic field during the past 9300 years inferred from cosmogenic radionuclides , 2010 .
[34] L. Mestel. Stellar magnetism , 1999 .
[35] C. Schrijver,et al. Dispersal of Magnetic Flux in the Quiet Solar Photosphere , 1999 .
[36] L. A. Aguirre,et al. Forecasting the Time Series of Sunspot Numbers , 2008 .
[37] J. Beer. Long-term indirect indices of solar variability , 2000 .
[38] N. Sheeley,et al. The origin of rigidly rotating magnetic field patterns on the sun , 1987 .
[39] L. D. Meeker,et al. Major features and forcing of high‐latitude northern hemisphere atmospheric circulation using a 110,000‐year‐long glaciochemical series , 1997 .
[40] E. Bullock,et al. MODELING THE TIME VARIABILITY OF SDSS STRIPE 82 QUASARS AS A DAMPED RANDOM WALK , 2010, 1004.0276.
[41] J. Schmelz,et al. The sun : a laboratory for astrophysics , 1992 .
[42] H. Kantz,et al. Nonlinear time series analysis , 1997 .