A precise measurement of the solar differential rotation by tracing small bright coronal structures in SOHO-EIT images - Results and comparisons for the period 1998–2006

H. Wöhl; R. Brajša; A. Hanslmeier; S. F. Gissot

doi:10.1051/0004-6361/200913081

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Volume 520 (September-October 2010)

A&A, 520 (2010) A29

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Issue		A&A Volume 520, September-October 2010


Article Number		A29
Number of page(s)		11
Section		The Sun
DOI		https://doi.org/10.1051/0004-6361/200913081
Published online		24 September 2010

Online Material

Table 3: Differential rotation parameters A and B from Eq. (1) and their standard errors M in deg day^-1 obtained applying the automatic method to monthly data sets for the year 1998.

Table 4: Similar to Table 3 for the year 1999, $N_{\rm s/y} = 3014$ .

Table 5: Similar to Table 3 for the year 2000, $N_{\rm s/y} = 7254$ .

Table 6: Similar to Table 3 for the year 2001, $N_{\rm s/y} = 6882$ .

Table 7: Similar to Table 3 for the year 2002, $N_{\rm s/y} = 7123$ .

Table 8: Similar to Table 3 for the year 2003, $N_{\rm s/y} = 9450$ .

Table 9: Similar to Table 3 for the year 2004, $N_{\rm s/y} = 7700$ .

Table 10: Similar to Table 3 for the year 2005, $N_{\rm s/y} = 5162$ .

Table 11: Similar to Table 3 for the year 2006, $N_{\rm s/y} = 3221$ .

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{13081_fig4.eps} \end{figure}$	Figure 4: The low-latitude part of Fig. 3.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{13081_fig5.eps} \end{figure}$	Figure 5: The high-latitude part of Fig. 3.
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