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Home All issues Volume 504 / No 1 (September II 2009) A&A, 504 1 (2009) L1-L4 Full HTML
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Table 1:

Frequency shifts at each l per unit of change in solar proxy and correlations from the analysis of independent 91.25-day GOLF spectra.
  April 1996-June 2007 June 2007-May 2009
l Gradienta $r_{\rm p}$ $r_{\rm s}$ $P_{\rm s}$ Gradienta $r_{\rm p}$ $r_{\rm s}$ $P_{\rm s}$
  10.7- cm radio flux
0 1.3 $\pm$ 0.2 0.82 0.77 $1.15 \times 10^{-9}$ -16.6 $\pm$ 12.1 -0.66 -0.71 0.07
1 1.7 $\pm$ 0.2 0.82 0.82 $1.93 \times 10^{-11}$ 6.2 $\pm$ 11.5 0.52 0.43 0.34
2 2.1 $\pm$ 0.2 0.86 0.85 $5.55 \times 10^{-13}$ -26.7 $\pm$ 13.1 -0.48 -0.32 0.48
  Mount Wilson MPSI
0 57.4 $\pm$ 7.3 0.81 0.78 $9.74 \times 10^{-10}$ -498.3 $\pm$ 440.6 -0.58 -0.39 0.38
1 78.9 $\pm$ 7.0 0.83 0.85 $7.37 \times 10^{-13}$ 239.6 $\pm$ 419.1 0.56 0.46 0.29
2 96.0 $\pm$ 7.8 0.85 0.84 $2.63 \times 10^{-12}$ -827.3 $\pm$ 457.1 -0.44 -0.07 0.88
a Gradient against the radio flux in units of nHz RF-1 (with 1 RF = 10-22 J s-1 m-2 Hz-1);
against the MPSI in units of nHz G-1.

Source LaTeX | All tables | In the text

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