Application of Non-linear Analysis to Intensity Oscillations of the Chromospheric Bright Points

[1]  Holger Kantz,et al.  Nonlinear Time Series Analysis , 2005 .

[2]  Timmer,et al.  What can Be inferred from surrogate data testing? , 2000, Physical review letters.

[3]  Milan Paluš,et al.  Sunspot Cycle: A Driven Nonlinear Oscillator? , 1999 .

[4]  Jürgen Kurths,et al.  Detection of n:m Phase Locking from Noisy Data: Application to Magnetoencephalography , 1998 .

[5]  M. Carlsson,et al.  Formation of Solar Calcium H and K Bright Grains , 1997 .

[6]  R. Kariyappa.  Solar oscillations in strong and weak fraunhofer lines over a quiet region , 1996 .

[7]  Kurths,et al.  Phase synchronization of chaotic oscillators. , 1996, Physical review letters.

[8]  R. Kariyappa.  Intensity oscillations in chromospheric bright points and network elements , 1994 .

[9]  S M Pincus,et al.  Greater signal regularity may indicate increased system isolation. , 1994, Mathematical biosciences.

[10]  Theiler,et al.  Generating surrogate data for time series with several simultaneously measured variables. , 1994, Physical review letters.

[11]  R. Kariyappa,et al.  Heating of the quiet solar chromosphere , 1994 .

[12]  William H. Press,et al.  The Art of Scientific Computing Second Edition , 1998 .

[13]  L. Tsimring,et al.  The analysis of observed chaotic data in physical systems , 1993 .

[14]  H. Uitenbroek,et al.  Ca ii H2v and K2v cell grains , 1991 .

[15]  Carroll,et al.  Synchronization in chaotic systems. , 1990, Physical review letters.

[16]  R. Athay,et al.  Model solar chromosphere with prescribed heating , 1989 .

[17]  D. Ruelle,et al.  Ergodic theory of chaos and strange attractors , 1985 .

[18]  P. Grassberger,et al.  Estimation of the Kolmogorov entropy from a chaotic signal , 1983 .

[19]  L. Cram,et al.  High spatial and temporal resolution observations of the solar CA II H line , 1983 .

[20]  P. Grassberger,et al.  Characterization of Strange Attractors , 1983 .

[21]  O. White,et al.  The vertical propagation of waves in the solar atmosphere. II Phase delays in the quiet chromosphere and cell-network distinctions , 1982 .

[22]  James P. Crutchfield,et al.  Geometry from a Time Series , 1980 .

[23]  Julius S. Bendat,et al.  Engineering Applications of Correlation and Spectral Analysis , 1980 .

[24]  M. Hénon,et al.  A two-dimensional mapping with a strange attractor , 1976 .

[25]  Sou-Yang Liu.  Direct Observational Evidence for the Propagation and Dissipation of Energy in the Chromosphere , 1974 .

[26]  J. Beckers,et al.  High resolution spectroscopy of the disk chromosphere , 1972 .

[27]  R. L. Stratonovich,et al.  Topics in the theory of random noise , 1967 .

[28]  F. Orrall,et al.  Observational Study of Macroscopic Inhomogeneities in the Solar Atmosphere.IV. Velocity and Intensity Fluctuations Observed in the K Line. , 1963 .

[29]  L. Trefethen,et al.  Numerical linear algebra , 1997 .

[30]  E. Priest,et al.  Implications of rapid footpoint motions of photospheric flux tubes for coronal heating , 1993 .

[31]  Loren Enochson,et al.  Digital Time Series Analysis. , 1972 .