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\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces \relax \fontsize  {9}{11}\normalfont  \abovedisplayskip 8.5\p@ plus3\p@ minus4\p@ \abovedisplayshortskip \z@ plus2\p@ \belowdisplayshortskip 4\p@ plus2\p@ minus2\p@ \def \leftmargin \leftmargini \parsep 4\p@ plus2\p@ minus\p@ \topsep 8\p@ plus2\p@ minus4\p@ \itemsep 4\p@ plus2\p@ minus\p@ {\leftmargin \leftmargini \topsep 4\p@ plus2\p@ minus2\p@ \parsep 2\p@ plus\p@ minus\p@ \itemsep \parsep }\belowdisplayskip \abovedisplayskip In the top panels, the extended bright areas highlight those parts of the earth that are the source of the earthshine. The satellite-derived cloud cover maps are shown in a secondary gray-scale with brighter areas indicating greater cloud cover. For 31 October 1999, note that the northernmost regions are not sunlit and the southernmost regions do not contribute to earthshine because the moon is fairly far north in the sky. The empty white boxes in the top panels indicate the longitudes of maximal contribution to the earthshine at the Universal Time (UT) shown. The solid boxes in the lower panels show the observed effective albedo as a function of time (note that the time axis is reversed), while the solid line indicates the simulated $A^*$.}}{3}}
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\bibcite{beer91}{beer (1991}
\bibcite{danjon28}{danjon(1928)}
\bibcite{danjon54}{danjon(1954)}
\bibcite{farrar00}{farrar (2000)}
\bibcite{frohlich00}{frohlich (2000)}
\bibcite{goode03}{goode(2003)}
\bibcite{goode01}{goode (2001)}
\bibcite{goode03}{goode (2003)}
\bibcite{ipcc95}{ipcc (1995)}
\bibcite{lean97}{lean (1997)}
\bibcite{palle00}{palle (2000)}
\bibcite{palle03}{palle (2003)}
\bibcite{qiu03}{qiu (2003)}
\bibcite{ram99}{ram99}
\bibcite{ramanathan89}{ramanathan (1989)}
\bibcite{stevens96}{stevens (1996)}
\bibcite{svensmark97}{svensmark97}
\bibcite{willson91}{willson (1991)}
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