Aballe Villero, M.A., Garcia De La Rosa, J.I. - GONG - National Solar ...

Canuto, V.M., and Mazzitelli, I.1991, Astrophys. J., 370, 295-311, Stellar turbulent convection: A new
model and applications
Canuto, V.M., et al.,1982, in Advances in Ultraviolet Astronomy: Four Years of IUE Research, eds. Y.
Kondo, J.M. Mead, and R.D. Chapman, NASA Conference Publication #2238, 293, The Relevance of
the IUE Results on Young Stars for the Earth's Paleoatmosphere
Capon, J.1969, Proc. IEEE 57, 1408-1418, reprinted 1978, in Modern Spectrum Analysis, ed. D.G.
Childers, New York: IEEE Press, 119-129, High Resolution Frequency-Wavenumber Spectrum
Analysis
Capon, J.1973, Meth. in Comp. Phys. 13, 1-59, Signal Processing and Frequency-Wavenumber
Spectrum Analysis for a Large Aperture Seismic Array
Capon, J., and Goodman, N.R.1970, Proc. IEEE 58, 1785-1786 erratum 59, 112, reprinted 1978, in
Modern Spectrum Analysis, ed. D.G. Childers, New York: IEEE Press, 162-163, Probability
Distributions for Estimators of the Frequency-Wavenumber Spectrum
Capps, C.D., Henning, R.L., and Hess, G.M.1982, Appl. Opt. 21, 3581-3587, Analytic Inversion of
Remote-Sensing Data
Caputo, F., Marconi, M., and Santolamazza, P.1998, Mon. Not. Roy. astron. Soc. 293, 364, The role of
chemical composition in RR Lyrae pulsationalproperties - I. Periods
Carbone, V., and Bruno, R.1997, Astrophys. J. 488, 482, Sign Singularity of the Magnetic Helicity from
In Situ Solar Wind Observations
Carbonell, M., and Ballester, J.L.1990, Astron. Astrophys. 234, 377
Carbonell, M., and Ballester, J.L.1992, Astron. Astrophys. 255, 350
Carbonell, M., Oliver, R., and Ballester, J.L.1992, Astron. Astrophys., 264, 350-360, Power spectra of
gapped time series: a comparison of several methods
Carbonell, M., Oliver, R., and Ballester, J.L.1994, Astron. Astrophys., 290, 983, A search for chaotic
behaviour in solar activity
Cardon, B.L., Smith, P.L., Scalo, J.M., and Testerman, L.1982, Astrophys. J. 260, 395, Absolute
oscillator strengths for lines of neutral cobalt between 2276 A and 9357 A and a redetermination of the