\documentclass[a4paper,11pt] {article}

\usepackage{graphicx}
\usepackage{amsmath}
\usepackage{amsfonts}
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\usepackage{pifont}
\usepackage{enumerate}
\usepackage{mathrsfs}


\title{SUPPLEMENTARY MATERIAL}



\begin{document}

\renewcommand{\figurename}{Supplementary Fig}

\begin {figure}
\begin{center}
\begin{tabular}{ccc}
   \includegraphics[width=4cm]{./inca_0.jpg} &
   \includegraphics[width=4cm]{./inca_2.jpg} &
   \includegraphics[width=4cm]{./inca_3.jpg} \\
        Ls 189.0 & Ls 217.3 & Ls 219.8 \\
   
   
   \includegraphics[width=4cm]{./inca_4.jpg} &
   \includegraphics[width=4cm]{./inca_6.jpg} &
   \includegraphics[width=4cm]{./inca_7.jpg} \\
     Ls 233.3 & Ls 246.9 & Ls 249.6 \\
     \\

\end{tabular}
\includegraphics[width=5cm]{./scale.jpg} \\
\vspace{1cm}
   \includegraphics[width=14cm]{./inca189.jpg} \\
   \textbf{Ls 189.0}  \\
    


\end{center}
\caption{Top: surface temperature as seen by THEMIS in the Inca City region (-81N,295E) during MY28 southern spring. Ls of the acquisition is in bold letters when images in the visible are available. Bottom: THEMIS visible image over the same area of Inca City at Ls 207.6. CRISM images spatial extent (Sup. Fig \ref{incacrism}) is identified by red line. The warm spots on temperatures maps correspond to the concentration of dark spots between the dunes.}
\label{incathemis}
\end{figure} 


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%



\begin {figure}
\begin{center}
\includegraphics[width=15cm]{./inca_crism.jpg}

%\begin{tabular}{cccc}
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_CO2_0b.png} &
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_CO2_1b.png} &
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_CO2_2b.png} &
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_CO2_3b.png} \\
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_REFF_0b.png} &
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_REFF_1b.png} &
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_REFF_2b.png} &
%   \includegraphics[width=3.5cm]{./figures/crism/inca_crism_REFF_3b.png} \\
%    Ls 196.2 & Ls 206.6 & Ls 241.1 & Ls 254.8 \\
%\end{tabular}
\begin{tabular}{cc}
\includegraphics[width=5cm]{./barre_co2.jpg} &
\includegraphics[width=5cm]{./barre_reff.jpg} \\
\end{tabular}
\end{center}
\caption{Top: CO$_2$ ice spectral signature derived from CRISM data over Inca City. Bottom: reflectance factor at 1.33 $\mu$m. Their spatial extent is identified by red line in Sup. Fig \ref{incathemis}. No clear opaque cover of the CO$_2$ ice can be observed at the pixel scale in the available data (except in a few spots at Ls 196.2).}
\label{incacrism}
\end{figure} 

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


\begin {figure}
\begin{center}
   \includegraphics[width=4cm]{./dolo_vis_cad.jpg} \\
   \textbf{Ls 202.4} \\
\end{center}
\caption{THEMIS visible image over Dolomedes at Ls 202.4. CRISM images spatial extent (Sup. Fig \ref{dolocrism}) is identified by red line. Dark spots distribution follows the stratification and are present on different oriented slopes.}
\label{dolothemisvis}
\end{figure}


\begin {figure}
\begin{center}
\begin{tabular}{c}
   
\includegraphics[width=15cm]{./themis_dolo.jpg} \\


\end{tabular}
\includegraphics[width=5cm]{./scale.jpg} \\

\end{center}
\caption{Surface temperature as seen by THEMIS in the Dolomedes region (-87N,174E) during MY28 southern spring. Spatial extent is the same as in Sup. Fig 3. Structures in the temperature maps begin to emerge at Ls 211.8.}
\label{dolothemis}
\end{figure}

\begin {figure}
\begin{center}

\includegraphics[width=15cm]{./dolomedes_crism.jpg}
%
%\begin{tabular}{cccccc}
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_CO2_0b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_CO2_1b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_CO2_2b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_CO2_3b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_CO2_4b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_CO2_5b.png} \\
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_REFF_0b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_REFF_1b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_REFF_2b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_REFF_3b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_REFF_4b.png} &
%   \includegraphics[width=2cm]{./figures/crism/dolomedes_crism_REFF_5b.png} \\
%    Ls 205.7 & Ls 207.6 & Ls 214.5 & Ls 243.4 & Ls 245.4 & Ls 258.4 \\
%\end{tabular}

\begin{tabular}{cc}
\includegraphics[width=5cm]{./barre_co2.jpg} &
\includegraphics[width=5cm]{./barre_reff.jpg} \\
\end{tabular}
\end{center}
\caption{Top: CO$_2$ ice spectral signature derived from CRISM data over Dolomedes. Bottom: reflectance factor at 1.33 $\mu$m. Their spatial extent is identified by red line in Sup. Fig \ref{dolothemisvis}.}
\label{dolocrism}
\end{figure} 

\end{document}
