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% AGUtmpl.tex: this template file is for articles formatted with LaTeX2e,
% Modified December 2018
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% This template includes commands and instructions
% given in the order necessary to produce a final output that will
% satisfy AGU requirements.
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% FOR FIGURES, DO NOT USE \psfrag
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% IMPORTANT NOTE:
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% SUPPORTING INFORMATION DOCUMENTATION IS NOT COPYEDITED BEFORE PUBLICATION.
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% Step 1: Set the \documentclass
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%
% PLEASE USE THE DRAFT OPTION TO SUBMIT YOUR PAPERS.
% The draft option produces double spaced output.
%
% Choose the journal abbreviation for the journal you are
% submitting to:

% jgrga JOURNAL OF GEOPHYSICAL RESEARCH (use for all of them)
% gbc   GLOBAL BIOCHEMICAL CYCLES
% grl   GEOPHYSICAL RESEARCH LETTERS
% pal   PALEOCEANOGRAPHY
% ras   RADIO SCIENCE
% rog   REVIEWS OF GEOPHYSICS
% tec   TECTONICS
% wrr   WATER RESOURCES RESEARCH
% gc    GEOCHEMISTRY, GEOPHYSICS, GEOSYSTEMS
% sw    SPACE WEATHER
% ms    JAMES
% ef    EARTH'S FUTURE
%
%
%
% (If you are submitting to a journal other than jgrga,
% substitute the initials of the journal for "jgrga" below.)

\documentclass[draft,grl]{agutexSI2019}

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%  SUPPORTING INFORMATION TEMPLATE
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%% ------------------------------------------------------------------------ %%
%
%
%Please use this template when formatting and submitting your Supporting Information.

%This template serves as both a “table of contents” for the supporting information for your article and as a summary of files.
%
%
%OVERVIEW
%
%Please note that all supporting information will be peer reviewed with your manuscript. It will not be copyedited if the paper is accepted.
%In general, the purpose of the supporting information is to enable authors to provide and archive auxiliary information such as data tables, method information, figures, video, or computer software, in digital formats so that other scientists can use it.
%The key criteria are that the data:
% 1. supplement the main scientific conclusions of the paper but are not essential to the conclusions (with the exception of
%    including %data so the experiment can be reproducible);
% 2. are likely to be usable or used by other scientists working in the field;
% 3. are described with sufficient precision that other scientists can understand them, and
% 4. are not exe files.
%
%USING THIS TEMPLATE
%
%***All references should be included in the reference list of the main paper so that they can be indexed, linked, and counted as citations.  The reference section does not count toward length limits.
%
%All Supporting text and figures should be included in this document. Insert supporting information content into each appropriate section of the template. To add additional captions, simply copy and paste each sample as needed.

%Tables may be included, but can also be uploaded separately, especially if they are larger than 1 page, or if necessary for retaining table formatting. Data sets, large tables, movie files, and audio files should be uploaded separately. Include their captions in this document and list the file name with the caption. You will be prompted to upload these files on the Upload Files tab during the submission process, using file type “Supporting Information (SI)”

%IMPORTANT NOTE ON FIGURES AND TABLES
% Placeholders for figures and tables appear after the \end{article} command, after references.
% DO NOT USE \psfrag or \subfigure commands.
%
 \usepackage{graphicx}
%
%  Uncomment the following command to allow illustrations to print
%   when using Draft:
 \setkeys{Gin}{draft=false}
%
% You may need to use one of these options for graphicx depending on the driver program you are using. 
%
% [xdvi], [dvipdf], [dvipsone], [dviwindo], [emtex], [dviwin],
% [pctexps],  [pctexwin],  [pctexhp],  [pctex32], [truetex], [tcidvi],
% [oztex], [textures]
%
%
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%  ENTER PREAMBLE
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% Author names in capital letters:
%\authorrunninghead{BALES ET AL.}

% Shorter version of title entered in capital letters:
%\titlerunninghead{SHORT TITLE}

%Corresponding author mailing address and e-mail address:
%\authoraddr{Corresponding author: A. B. Smith,
%Department of Hydrology and Water Resources, University of
%Arizona, Harshbarger Building 11, Tucson, AZ 85721, USA.
%(a.b.smith@hwr.arizona.edu)}

\begin{document}

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%  TITLE
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%\includegraphics{agu_pubart-white_reduced.eps}


\title{Supporting Information for "Broad consistency between observed and simulated trends in sea surface temperature patterns"}
%
% e.g., \title{Supporting Information for "Terrestrial ring current:
% Origin, formation, and decay $\alpha\beta\Gamma\Delta$"}
%
%DOI: 10.1002/%insert paper number here%

%% ------------------------------------------------------------------------ %%
%
%  AUTHORS AND AFFILIATIONS
%
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% List authors by first name or initial followed by last name and
% separated by commas. Use \affil{} to number affiliations, and
% \thanks{} for author notes.
% Additional author notes should be indicated with \thanks{} (for
% example, for current addresses).

% Example: \authors{A. B. Author\affil{1}\thanks{Current address, Antartica}, B. C. Author\affil{2,3}, and D. E.
% Author\affil{3,4}\thanks{Also funded by Monsanto.}}

\authors{Dirk Olonscheck\affil{1}, Maria Rugenstein\affil{1}, Jochem Marotzke\affil{1}}
\affiliation{1}{Max Planck Institute for Meteorology, Bundesstrasse 53, 20146 Hamburg, Germany}

%\correspondingauthor{Dirk Olonscheck}{dirk.olonscheck@mpimet.mpg.de}





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%
%  BEGIN ARTICLE
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% The body of the article must start with a \begin{article} command
%
% \end{article} must follow the references section, before the figures
%  and tables.

\begin{article}

%% ------------------------------------------------------------------------ %%
%
%  TEXT
%
%% ------------------------------------------------------------------------ %%



\noindent\textbf{Contents of this file}
%%%Remove or add items as needed%%%
\begin{enumerate}
\item Tables S1 to S2
\item Figures S1 to S8

%if Tables are larger than 1 page, upload as separate excel file
\end{enumerate}

%\noindent\textbf{Introduction}
%Type or paste your text here. The introduction gives a brief overview of the supporting information. You should include information %about as many of the following as possible (when appropriate):
% 1. a general overview of the kind of data files;
% 2. information about when and how the data were collected or created;
% 3. a general description of processing steps used;
% 4. any known imperfections or anomalies in the data.

%\clearpage

%Delete all unused file types below. Copy/paste for multiples of each file type as needed.
%\noindent\textbf{Text S1.}
%Type or paste text here. This should be additional explanatory text, such as: extended descriptions of results, full details of models, extended lists of acknowledgements etc.  It should not be additional discussion, analysis, interpretation or critique. It should not be an additional scientific experiment or paper.
%
%Repeat for any additional Supporting Text

%%Enter Data Set, Movie, and Audio captions here
%%EXAMPLE CAPTIONS

%\noindent\textbf{Data Set S1.} %Type or paste caption here.
%upload your dataset(s) to AGU's journal submission site and select "Supporting Information (SI)" as the file type. Following naming %convention: ds01.

%Repeat for any additional Supporting data sets

%\noindent\textbf{Movie S1.} %Type or paste caption here.
%upload your movie(s) to AGU's journal submission site and select, "Supporting Information %(SI)" as the file type. Following naming convention: ms01.

%Repeat any additional Supporting movies

%\noindent\textbf{Audio S1.} %Type or paste caption here.
%upload your audio file(s) to AGU's journal submission site and select "Supporting Information %(SI)" as the file type. Following naming convention: auds01.


%Repeat for any additional Supporting audio files

%%% End of body of article:
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% Optional Notation section goes here
%
% Notation -- End each entry with a period.
% \begin{notation}
% Term & definition.\\
% Second term & second definition.\\
% \end{notation}
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%%  REFERENCE LIST AND TEXT CITATIONS

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% 
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% \bibliography{<name of your .bib file>} do not specify file extension
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% no need to specify bibliographystyle
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% Note that ALL references in this supporting information file must also be referenced in the primary manuscript
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% if you get an error about newblock being undefined, uncomment this line:
%\newcommand{\newblock}{}

% \bibliography{ uncomment this line and enter the name of your bibtex file here } 




%Reference citation instructions and examples:
%
% Please use ONLY \cite and \citeA for reference citations.
% \cite for parenthetical references
% ...as shown in recent studies (Simpson et al., 2019)
% \citeA for in-text citations
% ...Simpson et al (2019) have shown...
% DO NOT use other cite commands (e.g., \citet, \citep, \citeyear, \nocite, \citealp, etc.).
%
%
%...as shown by \citeA{jskilby}.
%...as shown by \citeA{lewin76}, \citeA{carson86}, \citeA{bartoldy02}, and \citeA{rinaldi03}.
%...has been shown \cite<e.g.,>{jskilbye}.
%...has been shown \cite{lewin76,carson86,bartoldy02,rinaldi03}.
%...has been shown \cite{lewin76,carson86,bartoldy02,rinaldi03}.
%
% apacite uses < > for prenotes, not [ ]
% DO NOT use other cite commands (e.g., \citet, \citep, \citeyear, \nocite, \citealp, etc.).
%

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%
%  END ARTICLE
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%% ------------------------------------------------------------------------ %%
\end{article}
\clearpage

% Copy/paste for multiples of each file type as needed.

% enter figures and tables below here: %%%%%%%
%
\begin{table}
	\makeatletter
	\renewcommand{\thetable}{S\@arabic\c@table}
	\begin{center}
	\caption{Minimum, average, and maximum Pearson correlation coefficient, r, of the annual global mean SST evolution between the realizations of each model ensemble and the averages across observational estimates. A small spread and a high value of r indicate that the ensemble members resemble the observed SST evolution, while a high spread and a low value of r indicate less agreement. Compare with Figure 1.}\label{tab:dailyCMIP5}
	\vspace{1cm}
		\fontsize{13}{13}\selectfont
		\renewcommand{\arraystretch}{1}
		\begin{tabular}{l c c c} % centered columns
			%\hline
			Model ensemble & r$_{min}$ & r$_{avg}$ & r$_{max}$ \\[0.2ex] % heading
			\hline \\[0.1ex]%\hline
			CMIP5 & 0.38 & 0.72 & 0.84 \\ 
			CMIP6 & 0.48 & 0.76 & 0.88\\
			CanESM2 & 0.77 & 0.83 & 0.88\\
			CESM-LE & 0.58 & 0.69 & 0.81 \\
			CSIRO-Mk3-6-0 & 0.37 & 0.54 & 0.64 \\
			GFDL-ESM2M & 0.66 & 0.78 & 0.86 \\
			IPSL-CM6A-LR & 0.70 & 0.78 & 0.86\\
			MIROC6 & 0.54 & 0.65 & 0.73 \\
			MPI-GE & 0.68 & 0.74 & 0.82 \\[1ex]
			\hline
		\end{tabular}\\[1ex]
	\end{center}
\end{table}
\clearpage

\begin{table}
	\makeatletter
	\renewcommand{\thetable}{S\@arabic\c@table}
	%\setcounter{table}{0} 
	\begin{center}
	\caption{Percent of ensemble members of each model with a globally averaged SST trend larger than the observed COBE-SST2 trend for the four trend periods. In the early warming period, no single realization captures the observed warming, whereas in the recent warming period, the representation of the observed warming strongly differs between the models. For the recent hiatus, all models warm more than observed.}\label{tab:pctTrends}
	\vspace{1cm}
		\fontsize{13}{13}\selectfont
		\renewcommand{\arraystretch}{1}
		\begin{tabular}{l c c c c} % centered columns
			%\hline
			Model ensemble & 1915-1944 & 1945-1974 & 1975-2004 & 1995-2014 \\[0.2ex] % heading
			\hline \\[0.1ex]%\hline
			CMIP5 & 0 & 90 & 0 & - \\ 
			CMIP6 & 0 & 41 & 39 & 96 \\
			CanESM2 & - & - & 94 & 100 \\
			CESM-LE & - & 39 & 2 & - \\
			CSIRO-Mk3-6-0 & 0 & 3 & 13 & 96\\
			GFDL-ESM2M & - & - & 26 & 93 \\
			IPSL-CM6A-LR & 0 & 67 & 54 & 96 \\
			MIROC6 & 0 & 34 & 2 & 90 \\
			MPI-GE & 0 & 79 & 24 & - \\[1ex]
			\hline
		\end{tabular}\\[1ex]
	\end{center}
\end{table}
\clearpage 

\renewcommand\thefigure{S\arabic{figure}}    
\setcounter{figure}{0}  
\begin{figure}
\includegraphics[width=1.\textwidth]{FigS1_revised.pdf}
\caption{Same as Figure 1, but with respect to the reference period 1850-1900. Note that only the single-model large ensembles are shown with simulations that start in 1850.}
\label{figintro_ref}
\end{figure}

\begin{figure}
\includegraphics[width=1.\textwidth]{FigS2_revised.pdf}
\caption{Trend in SST patterns in the three observational data sets COBE-SST2, ERSSTv5, and HadISST2 for the four characteristic trend periods. Stippling marks statistically significant trends at the 95\% level. Note that the observational uncertainty is much greater than the difference between the data sets (Kennedy, 2014).
}
\label{obs}
\end{figure}

\begin{figure}
\begin{center}
%\includegraphics[width=0.8\textwidth]{sst_trends_bestPatCor.pdf}
\includegraphics[width=0.55\textwidth]{FigS3_revised.pdf}
\caption{COBE-SST2 trend pattern and model simulations with the highest pattern correlation with COBE-SST2 for the period 1975-2004 (left column) and the period 1995-2014 (right column). The numbers on top of each panel specify the number of the ensemble member, and the value of r, respectively.}
\label{bestpat}
\end{center}
\end{figure}

\begin{figure}
\includegraphics[width=1.\textwidth]{FigS4_revised.pdf}
\caption{Same as Fig. 2, but using the observational data set ERSSTv5.}
\label{bigfig_ersst}
\end{figure}

\begin{figure}
\includegraphics[width=1.\textwidth]{FigS5_revised.pdf}
\caption{Same as Fig. 2, but using the observational data set HadISST2.}
\label{bigfig_hadisst}
\end{figure}

\begin{figure}
\includegraphics[width=1.\textwidth]{FigS6_revised.pdf}
\caption{Same as Fig. 2 for CMIP5 and CMIP6, but for all simulations in CMIP5 and CMIP6, including all ensemble members for each model instead of just the first ensemble member of each model as shown in Fig.\,2 in the main text.}
\label{bigfig_cmip}
\end{figure}

\begin{figure}
\begin{center}
\includegraphics[width=0.95\textwidth]{FigS7_revised.pdf}
\caption{Terms of Equation 1 for all model ensembles. The observed COBE-SST2 trend (top row), and the ensemble mean trend of each model ensemble (other rows) for the four characteristic historical periods. The ensemble standard deviation $\sigma$ of all model ensembles is shown in Figure S8.} 
\label{terms_eq1_1}
\end{center}
\end{figure} 

%\renewcommand\thefigure{S\arabic{figure}}    
%\setcounter{figure}{6}  
\begin{figure}
\begin{center}
\includegraphics[width=0.95\textwidth]{FigS8_revised.pdf}
\caption{\textbf{(As Figure S7, continued)} The ensemble standard deviation $\sigma$ of all model ensembles for the four characteristic historical periods. Note that the larger ensemble standard deviation in the last column is caused by the computation over only a 20-year period.}
\label{terms_eq1_2}
\end{center}
\end{figure}


%
%
% EXAMPLE FIGURES
% ---------------
% If you get an error about an unknown bounding box, try specifying the width and height of the figure with the natwidth and natheight options.
% \begin{figure}
%\setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
% \noindent\includegraphics[natwidth=800px,natheight=600px]{samplefigure.eps}
%\caption{caption}
%\label{epsfiguresample}
%\end{figure}
%
%
% Giving latex a width will help it to scale the figure properly. A simple trick is to use \textwidth. Try this if large figures run off the side of the page.
% \begin{figure}
% \noindent\includegraphics[width=\textwidth]{anothersample.png}
%\caption{caption}
%\label{pngfiguresample}
%\end{figure}
%
%
%\begin{figure}
%\noindent\includegraphics[width=\textwidth]{athirdsample.pdf}
%\caption{A pdf test figure}
%\label{pdffiguresample}
%\end{figure}
%
% PDFLatex does not seem to be able to process EPS figures. You may want to try the epstopdf package.
%
%
% ---------------
% EXAMPLE TABLE
%
%\begin{table}
%\settablenum{S1} %%Change number for each table
%\caption{Time of the Transition Between Phase 1 and Phase 2\tablenotemark{a}}
%\centering
%\begin{tabular}{l c}
%\hline
% Run  & Time (min)  \\
%\hline
%  $l1$  & 260   \\
%  $l2$  & 300   \\
%  $l3$  & 340   \\
%  $h1$  & 270   \\
%  $h2$  & 250   \\
%  $h3$  & 380   \\
%  $r1$  & 370   \\
%  $r2$  & 390   \\
%\hline
%\end{tabular}
%\tablenotetext{a}{Footnote text here.}
%\end{table}
% ---------------
%
% EXAMPLE LARGE TABLE (UPLOADED SEPARATELY)
%\begin{table}
%\settablenum{S1} %%Change number for each table
%\caption{Time of the Transition Between Phase 1 and Phase 2\tablenotemark{a}}
%\end{table}

\end{document}

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More Information and Advice:

%% ------------------------------------------------------------------------ %%
%
%  SECTION HEADS
%
%% ------------------------------------------------------------------------ %%

% Capitalize the first letter of each word (except for
% prepositions, conjunctions, and articles that are
% three or fewer letters).

% AGU follows standard outline style; therefore, there cannot be a section 1 without
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% ---------------
% Level 1 head
%
% Use the \section{} command to identify level 1 heads;
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%An example:
%\section{Level 1 Head: Introduction}
%
% ---------------
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% Use the \subsubsection{} command to identify level 3 heads
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%
%---------------
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% Use the \subsubsubsection{} command to identify level 3 heads
% An example:
%\subsubsubsection{Level 4 Head} An example.
%
%% ------------------------------------------------------------------------ %%
%
%  IN-TEXT LISTS
%
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%
% Do not use bulleted lists; enumerated lists are okay.
% \begin{enumerate}
% \item
% \item
% \item
% \end{enumerate}
%
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%
%  EQUATIONS
%
%% ------------------------------------------------------------------------ %%

% Single-line equations are centered.
% Equation arrays will appear left-aligned.

Math coded inside display math mode \[ ...\]
 will not be numbered, e.g.,:
 \[ x^2=y^2 + z^2\]

 Math coded inside \begin{equation} and \end{equation} will
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 \begin{equation}
 x^2=y^2 + z^2
 \end{equation}

% IF YOU HAVE MULTI-LINE EQUATIONS, PLEASE
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% using double backslashes (\\).

% To create multiline equations, use the
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% as demonstrated below.
\begin{eqnarray}
  x_{1} & = & (x - x_{0}) \cos \Theta \nonumber \\
        && + (y - y_{0}) \sin \Theta  \nonumber \\
  y_{1} & = & -(x - x_{0}) \sin \Theta \nonumber \\
        && + (y - y_{0}) \cos \Theta.
\end{eqnarray}

%If you don't want an equation number, use the star form:
%\begin{eqnarray*}...\end{eqnarray*}

% Break each line at a sign of operation
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% \hspace{1in}; you may have to experiment to achieve
% the correct amount of space.


%% ------------------------------------------------------------------------ %%
%
%  EQUATION NUMBERING: COUNTER
%
%% ------------------------------------------------------------------------ %%

% You may change equation numbering by resetting
% the equation counter or by explicitly numbering
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% To explicitly number an equation, type \eqnum{}
% (with the desired number between the brackets)
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% command.  The \eqnum{} command will affect only
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% according to the equation counter.
%

% If you have a multiline equation that needs only
% one equation number, use a \nonumber command in
% front of the double backslashes (\\) as shown in
% the multiline equation above.

%% ------------------------------------------------------------------------ %%
%
%  SIDEWAYS FIGURE AND TABLE EXAMPLES
%
%% ------------------------------------------------------------------------ %%
%
% For tables and figures, add \usepackage{rotating} to the paper and add the rotating.sty file to the folder.
% AGU prefers the use of {sidewaystable} over {landscapetable} as it causes fewer problems.
%
% \begin{sidewaysfigure}
% \includegraphics[width=20pc]{samplefigure.eps}
% \caption{caption here}
% \label{label_here}
% \end{sidewaysfigure}
%
%
%
% \begin{sidewaystable}
% \caption{}
% \begin{tabular}
% Table layout here.
% \end{tabular}
% \end{sidewaystable}
%
%

