%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% AGUtmpl.tex: this template file is for articles formatted with LaTeX2e,
% Modified December 2018
%
% This template includes commands and instructions
% given in the order necessary to produce a final output that will
% satisfy AGU requirements.
%
% FOR FIGURES, DO NOT USE \psfrag
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% IMPORTANT NOTE:
%
% SUPPORTING INFORMATION DOCUMENTATION IS NOT COPYEDITED BEFORE PUBLICATION.
%
%
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% Step 1: Set the \documentclass
%
%
% 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}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
%  SUPPORTING INFORMATION TEMPLATE
%
%% ------------------------------------------------------------------------ %%
%
%
%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}
\usepackage{longtable}

\newcommand{\CO}[1]{CO\textsubscript{#1}}
\newcommand{\CH}[1]{CH\textsubscript{#1}}
\newcommand{\N}[1]{N\textsubscript{#1}}

\newcommand{\mainfigclassificationexceedanceprobs}[0]{1}
%
%  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]
%
%
%% ------------------------------------------------------------------------ %%
%
%  ENTER PREAMBLE
%
%% ------------------------------------------------------------------------ %%

% Author names in capital letters:
\authorrunninghead{NICHOLLS ET AL.}

% Shorter version of title entered in capital letters:
\titlerunninghead{CHANGES IN IPCC SCENARIO ASSESSMENT EMULATORS}

%Corresponding author mailing address and e-mail address:
\authoraddr{Corresponding author: Z. Nicholls,
Climate \& Energy College, School of Geography, Earth and Atmospheric Sciences, The University of Melbourne, Parkville, Victoria, Australia
(zebedee.nicholls@climate-energy-college.org)}

\begin{document}

%% ------------------------------------------------------------------------ %%
%
%  TITLE
%
%% ------------------------------------------------------------------------ %%

%\includegraphics{agu_pubart-white_reduced.eps}


\title{Supporting Information for `Changes in IPCC scenario assessment emulators between SR1.5 and AR6 unravelled'}
%
% 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
%
%% ------------------------------------------------------------------------ %%


% 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.}}

\input{authors.tex}


%% ------------------------------------------------------------------------ %%
%
%  BEGIN ARTICLE
%
%% ------------------------------------------------------------------------ %%

% 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 Text S1: Reasons for the higher warming projections in MAGICC6 compared to the projections from AR5-like MAGICCv7.5.3
\item Text S2: Changes in effective radiative forcing by species between MAGICC6 and MAGICCv7.5.3
\item Figure S1: Difference between the emulator output underlying the SR1.5 scenario categorisation and alternate emulator output for exceedance probabilities of 1.5\textdegree C and 2\textdegree C warming for 2100 and peak
\item Figure S2: Projected median and upper 67\% warming projections for SR1.5 scenarios between MAGICC6, MAGICCv7.5.3, FaIRv1.6.2 and FaIR 1.3
\item Figure S3: Difference between the emulator output underlying the SR1.5 scenario categorisation and alternate emulator output for median and 67\textsuperscript{th}-percentile projections for 2100 and peak temperatures
\item Figure S4: Relationship between exceedance probabilities and temperature projections across multiple emulators
\item Figure S5: Difference between the emulator output underlying the SR1.5 scenario categorisation and AR5-like MAGICCv7.5.3 for median and 67\textsuperscript{th}-percentile projections for 2100 and peak temperatures
\item Figure S6: Difference between the emulator output underlying the SR1.5 scenario categorisation and AR5-like MAGICCv7.5.3 for median and 67\textsuperscript{th}-percentile projections for 2100 and peak temperatures shown as histogram rather than scatter plot
\item Figure S7-S8, S12-S15: Comparison of output from the emulator underlying the SR1.5 scenario categorisation (MAGICC6) and MAGICCv7.5.3
\item Figure S9: \CO2 and \CH4 concentration projections from the MAGICCv7.5.3 and FaIRv1.6.2
\item Figure S10: Difference between MAGICCv7.5.3 and FaIRv1.6.2 emulators for median and 67\textsuperscript{th}-percentile projections for 2100 and peak temperatures
\item Figure S11: Difference between MAGICCv7.5.3 and FaIRv1.6.2 emulators for median and 67\textsuperscript{th}-percentile projections for 2100 and peak temperatures shown as a histogram rather than scatter plot
\item Figure S12-S17: Comparison of output from the emulator underlying the SR1.5 scenario categorisation (MAGICC6) and AR5-like MAGICCv7.5.3
\item Figure S18-S21: Comparison of more output from the emulator underlying the SR1.5 scenario categorisation (MAGICC6) and MAGICCv7.5.3
\item Table S1: Emulator model versions, their key characteristics and the main purpose for their use in this study
\end{enumerate}

% \noindent\textbf{Additional Supporting Information (Files uploaded separately)}
% \begin{enumerate}
% \item Captions for Datasets S1 to Sx
% \item Captions for large Tables S1 to Sx (if larger than 1 page, upload as separate excel file)
% \item Captions for Movies S1 to Sx
% \item Captions for Audio S1 to Sx
% \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.}

Here we discuss the reasons for the higher warming projections in MAGICC6 compared to the projections from AR5-like MAGICCv7.5.3 (Supplementary Figure \ref{fig:Surface-Temperature--GSAT-_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}). MAGICC6 generally has lower anthropogenic effective radiative forcing than AR5-like MAGICCv7.5.3 (Supplementary Figure \ref{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}). Therefore, differences in the parameterisations that link emissions and effective radiative forcing are not the reason for MAGICC6's higher warming projections and we hence conclude that differences in model calibration, particularly transient climate response (TCR), explain the difference instead.

We next discuss some of the changes in effective radiative forcing of different species and why these changes are approximately zero. As the AR5-like calibration of MAGICCv7.5.3 reflects literature which is more recent than AR5, this comparison provides an insight into some, but not all, the changes in effective radiative forcing between AR5 and AR6.

\CO2 effective radiative forcing is again relatively unchanged between the two emulators (Supplementary Figure \ref{fig:Effective-Radiative-Forcing-CO2_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}), reflecting the close agreement between the \CO2 ERF estimates used for the RCMIP Phase 2 tuning \cite{RN757} and the AR5 assessment \cite{RN54}. The differences in \CO2 effective radiative forcing are again largely driven by differences in the carbon cycle response (Supplementary Figure \ref{fig:Atmospheric-Concentrations-CO2_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}), with a similar range of differences on either side of the median.

Aerosol effective radiative forcing is more sensitive to changes in aerosol emissions in AR5-like MAGICCv7.5.3 than MAGICC6 (Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Aerosols_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}). These changes arise because the ERF used in RCMIP Phase 2 \cite{RN757} assesses aerosol forcing for 1750-2014 to be -1.01 W m\textsuperscript{-2}, an approximately 10\% increase on AR5's 1750-2011 assessment \cite{RN54} of -0.9 W m\textsuperscript{-2}.

Methane effective radiative forcing increases (Supplementary Figure \ref{fig:Effective-Radiative-Forcing-CH4_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}). The increase follows the upwards revision presented in \cite[without the inclusion of rapid adjustments, which are not included in AR5-like MAGICCv7.5.3]{RN81}.

Taking all the changes together, we see that \CO2 effective radiative forcing is largely unchanged, aerosol effective radiative forcing is initially more negative before being more positive and methane effective radiative forcing is more positive. In sum, the combination of these and other changes leads to an increase of 0.0 - 0.2 W m\textsuperscript{-2} in anthropogenic effective radiative forcing. We note again that these changes are scenario dependent (Supplementary Figure \ref{fig:Atmospheric-Concentrations-CO2-CH4_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_AR6-calibration-SR1-5-processing-FaIRv1-6-2}) and bespoke analysis is required to understand each specific scenario's drivers.

%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{Text S2.}

Here we consider the changes in effective radiative forcing of different species and why these changes cancel out to approximately zero change (with a slight skew towards an increase) in total anthropogenic effective radiative forcing between MAGICC6 and MAGICCv7.5.3.

\CO2 effective radiative forcing has a median change of approximately zero (Supplementary Figure \ref{fig:Effective-Radiative-Forcing-CO2_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}). This almost zero change is the result of a slight increase in the assessment of \CO2 effective radiative forcing (for a given atmospheric \CO2 concentration) and a decrease in projected atmospheric \CO2 concentrations (Supplementary Figure \ref{fig:Atmospheric-Concentrations-CO2_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}). It is also worth noting that, while the median is unchanged, there is a range of differences due to differing climate-carbon feedbacks (particularly those driven by the different temperature projections).

Aerosol effective radiative forcing is more sensitive to changes in aerosol emissions. As a result, the negative aerosol effective radiative forcing is stronger today but reduced in the future as aerosol emissions drop (differences are calculated as MAGICCv7.5.3 minus MAGICC6 output, Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Aerosols_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}). These changes arise because the AR6 assessment of ERF \cite{RN18} assesses aerosol forcing for 2005-2014 relative to 1750 to be -1.3 W m\textsuperscript{-2}, compared to AR5's assessment \cite{RN54} for 2011 relative to 1750 of -0.9 W m\textsuperscript{-2}.

Finally, methane effective radiative forcing increases in the short-term before returning to a median difference of zero with a range of -0.075 W m\textsuperscript{-2} to 0.1 W m\textsuperscript{-2} (Supplementary Figure \ref{fig:Effective-Radiative-Forcing-CH4_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}). The increase follows the upwards revision presented in \citeA{RN81}, tempered by AR6's inclusion of rapid adjustments in the assessment of methane effective radiative forcing in line with \citeA{RN757}. The increased sensitivity to methane emissions (via methane concentrations) also leads to a more pronounced reduction in methane effective radiative forcing after its peak.

In summary, \CO2 effective radiative forcing has a median change of around zero with a slight skew towards a decrease, aerosol effective radiative forcing is initially more negative before being more positive and methane effective radiative forcing is initially more positive before being around zero or slightly more negative. In general, the combination of these and other changes lead to the increase in anthropogenic effective radiative forcing. However, the scenario dependence of these changes should once again be noted as individual scenarios might not match well with the overall trends discussed here (Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}).

% \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}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


%% ------------------------------------------------------------------------ %%
%%  REFERENCE LIST AND TEXT CITATIONS

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% 
%
\bibliography{bibliography} do not specify file extension
%
% no need to specify bibliographystyle
%
% Note that ALL references in this supporting information file must also be referenced in the primary manuscript
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% 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.).
%

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

\clearpage

\begin{center}
\begin{longtable}{ | p{0.17\linewidth} | p{0.14\linewidth} | p{0.23\linewidth} | p{0.35\linewidth} | }
% \settablenum{S1} %%Change number for each table
\caption{Emulators and their calibrations, key characteristics and main purpose in this study.} \\
\hline
\textbf{Model version} & \textbf{Calibration} & \textbf{Key characteristic} & \textbf{Purpose in this study} \\
\hline
\endfirsthead
\multicolumn{3}{c}%
{\tablename\ \thetable\ -- \textit{Continued from previous page}} \\
\hline
\textbf{Model version} & \textbf{Calibration} & \textbf{Key characteristic} & \textbf{Purpose in this study} \\
\hline
\endhead
\hline \multicolumn{3}{r}{\textit{Continued on next page}} \\
\endfoot
\hline
\endlastfoot

\hline
MAGICC6 & SR1.5/AR5 &MAGICC6 with its calibration and input data as used to categorise scenarios in the IPCC SR1.5 report and also used in AR5. & Baseline reference against which we express most emulator variations. \\
\hline
MAGICCv7.5.3 & RCMIP Phase 2 (i.e. `AR5-like') &MAGICCv7.5.3 as used in RCMIP Phase 2, calibrated to match scientific understanding approximately in line with knowledge at the time of SR1.5 (for full details, see \citeA{RN918}). This calibration approximately reflects the science of AR5 and SR1.5, but not the science of AR6. & Provides a MAGICC calibration that approximates the projections might have been made in SR1.5, had MAGICC been re-calibrated at the time. Allows us to disentangle changes from model calibration and changes from model versions. This setup's output provides an indication of what MAGICC6 could have been with updated calibration efforts that better matched the physical science at the time of SR1.5. The key difference to MAGICC6 is a slightly lower TCR - more in line with the AR5 TCR assessment. \\
\hline
MAGICCv7.5.3 & AR6 &MAGICCv7.5.3 calibrated to AR6 (see Cross-chapter Box 7.1 of \citeA{RN18}) & As this setup was used for scenario categorisation in AR6, a comparison with MAGICC6 indicates the full difference in the climate assessment between SR1.5 and AR6. A comparison with `RCMIP Phase 2 MAGICCv7.5.3' approximates the effect of the physical science update and subsequent calibration from AR5 to AR6 (separate from model development). \\
\hline
FaIR1.3 & SR1.5 &The model used for sensitivity exploration (beyond MAGICC6) as part of the IPCC SR1.5 assessment. The differences between SR1.5 MAGICC6 and SR1.5 FaIR 1.3 were largely unexplained at the time. & Demonstrating, for historical context, the relatively large difference that existed between two key emulators at the time of the IPCC SR1.5. \\
\hline
FaIRv1.6.2 & AR6 &FaIRv1.6.2 calibrated to AR6 (see Cross-chapter Box 7.1 of \citeA{RN18}) & The difference between AR6 MAGICCv7.5.3 and AR6 FaIRv1.6.2 highlights the uncertainty that arises due to emulator representation of AR6 science. Both AR6 MAGICCv7.5.3 and AR6 FaIRv1.6.2 were assessed as representing WG1 well, so we cannot say with confidence if one is more correct. The difference is much reduced compared to the difference between MAGICC6 and FaIR1.3 (where, had time allowed, deeper investigation may have revealed which model was more in line with the science available at the time). \\
\hline
\end{longtable}
\end{center}

\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_delta-classification-exceedance-probabilities_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR.pdf}
\caption{
  Difference between the emulator output underlying the SR1.5 scenario categorisation and alternate emulator output for exceedance probabilities of 1.5\textdegree C (top row) and 2\textdegree C warming (bottom row) for 2100 (left column) and peak (i.e. maximum between 2010 and 2100, right column). The data is the same as Figure \mainfigclassificationexceedanceprobs{} but has been plotted as a histogram of differences rather than a scatter plot. Scenarios with exceedance probabilities of close to 100\% cannot have large changes in exceedance probability (because exceedance probability is capped at 100\%), hence the large number of results with no change (zero is marked by the dashed grey line). The difference from MAGICCv7.5.3 emulator is shown in dark blue, from FaIRv1.6.2 is shown in red and from FaIR1.3 is shown in grey.
}
\label{fig:delta-classification-exceedance-probabilities_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=0.9\textwidth]{210_absolute-classification-temperatures_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR.pdf}
\caption{
  Projected median and upper 67\% warming projections for SR1.5 scenarios are very similar between MAGICC6 and MAGICCv7.5.3 (blue dots), slightly higher compared to FaIRv1.6.2 (red dots) or FaIR1.3 (grey dots). Emulator output underlying the SR1.5 scenario categorisation (x-axes) and other emulators (y-axes) for median (top row) and 67\textsuperscript{th}-percentile (bottom row) projections for 2100 (left column) and peak (right column) temperatures. Scenarios on the diagonal (grey dashed line) did not change temperature projections. Scenarios that exhibit lower global-mean temperatures according to the AR6-calibrated emulators are shown below the diagonal. MAGICCv7.5.3 is shown in dark blue, FaIRv1.6.2 is shown in red is and the grey dots indicate FaIR1.3.
}
\label{fig:absolute-classification-temperatures_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_delta-classification-temperatures_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR.pdf}
\caption{
  Difference between the emulator output underlying the SR1.5 scenario categorisation and alternate emulator output for median (top row) and 67\textsuperscript{th}-percentile (bottom row) projections for 2100 (left column) and peak (right column) temperatures. The data is the same as Supplementary Figure \ref{fig:absolute-classification-temperatures_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR} but has been plotted as a histogram rather than a scatter plot. The difference from MAGICCv7.5.3 is shown in dark blue, from FaIRv1.6.2 is shown in red and from FaIR1.3 is shown in grey.
}
\label{fig:delta-classification-temperatures_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_temp-v-exceedance-probs.pdf}
\caption{
  Relationship between exceedance probabilities and temperature projections across multiple emulators. By definition, when the median temperature is 1.5\textdegree C (2.0\textdegree C), the 1.5\textdegree C (2.0\textdegree C) exceedance probability is 50\%. For every 0.01\textdegree C increase in median temperature, 1.5\textdegree C exceedance probability increases by around 1.4\% and 2.0\textdegree C exceedance probability increases by around 0.9\%. The difference in gradient is because the uncertainty increases as the median temperature projection increases i.e. we have wider distributions once we get to around 2.0\textdegree C warming. The relationship is remarkably consistent across the emulators, with some small variations that become more noticeable as we get into the tails of the distributions i.e. as the median temperature moves away from the exceedance threshold of interest.
}
\label{fig:temp-v-exceedance-probs}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_absolute-classification-temperatures_MAGICC6_RCMIP2-MAGICC.pdf}
\caption{
  Emulator output underlying the SR1.5 scenario categorisation (x-axes) and AR5-like MAGICCv7.5.3 (y-axes) for median (top row) and 67\textsuperscript{th}-percentile (bottom row) projections for 2100 (left column) and peak (right column) temperatures. If temperature projections hadn't changed for a scenario, that scenario would be shown on the diagonal (grey dashed line). Scenarios that exhibit lower global-mean temperatures according to AR5-like MAGICCv7.5.3 are shown below the diagonal. The difference between AR5-like MAGICCv7.5.3 and MAGICC6 provides an approximate quantification of the change in projections which results from improved emulator calibrations. The figure is the same as Supplementary Figure \ref{fig:absolute-classification-temperatures_MAGICC6_AR6-MAGICC-AR6-FaIR-SR15-FaIR} but for a different combination of models.
}
\label{fig:absolute-classification-temperatures_MAGICC6_RCMIP2-MAGICC}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_delta-classification-temperatures_MAGICC6_RCMIP2-MAGICC.pdf}
\caption{
  Difference between the emulator output underlying the SR1.5 scenario categorisation and AR5-like MAGICCv7.5.3 for median (top row) and 67\textsuperscript{th}-percentile (bottom row) projections for 2100 (left column) and peak (right column) temperatures. The data is the same as Supplementary Figure \ref{fig:absolute-classification-temperatures_MAGICC6_RCMIP2-MAGICC} but has been plotted as a histogram rather than a scatter plot.
}
\label{fig:delta-classification-temperatures_MAGICC6_RCMIP2-MAGICC}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3.pdf}
\caption{
    Comparison of output from the emulator underlying the SR1.5 scenario categorisation (MAGICC6) and AR5-like MAGICCv7.5.3. a) Timeseries of median anthropogenic effective radiative forcing. b) Difference (MAGICCv7.5.3 - MAGICC6) in median anthropogenic effective radiative forcing.
}
\label{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}
\end{figure}

\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Surface-Temperature--GSAT-_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6.pdf}
\caption{
  Comparison of output from the emulator underlying the SR1.5 scenario categorisation (MAGICC6) and MAGICCv7.5.3. a) Timeseries of median surface air temperature (GSAT). b) Difference (MAGICCv7.5.3 - MAGICC6) in median surface air temperature (GSAT).
}
\label{fig:Surface-Temperature--GSAT-_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6.pdf}
\caption{
  Comparison of output from the emulator underlying the SR1.5 scenario categorisation (MAGICC6) and MAGICCv7.5.3. a) Timeseries of anthropogenic effective radiative forcing. b) Difference (MAGICCv7.5.3 - MAGICC6) in anthropogenic effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=0.8\textwidth]{230_Atmospheric-Concentrations-CO2-CH4_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_AR6-calibration-SR1-5-processing-FaIRv1-6-2.pdf}
\caption{
  \CO2 (top row) and \CH4 (bottom row) concentration projections from MAGICCv7.5.3 and FaIRv1.6.2. In the first column we show absolute projections from each emulator and in the second column we show the difference between the two emulators. MAGICCv7.5.3 projects higher concentrations (in general) than FaIRv1.6.2 which is part of the reason for differences in emissions-driven runs like those performed in WG3.
}
\label{fig:Atmospheric-Concentrations-CO2-CH4_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_AR6-calibration-SR1-5-processing-FaIRv1-6-2}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_absolute-classification-temperatures_AR6-MAGICC7_AR6-FaIR.pdf}
\caption{
  As in Supplementary Figure \ref{fig:absolute-classification-temperatures_MAGICC6_RCMIP2-MAGICC} but for MAGICCv7.5.3 (x-axes) and FaIRv1.6.2.
}
\label{fig:absolute-classification-temperatures_AR6-MAGICC7_AR6-FaIR}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{210_delta-classification-temperatures_AR6-MAGICC7_AR6-FaIR.pdf}
\caption{
  As in Supplementary Figure \ref{fig:delta-classification-temperatures_MAGICC6_RCMIP2-MAGICC} but for MAGICCv7.5.3 (x-axes) and FaIRv1.6.2. The data is the same as Supplementary Figure \ref{fig:absolute-classification-temperatures_AR6-MAGICC7_AR6-FaIR} but has been plotted as a histogram rather than a scatter plot.
}
\label{fig:delta-classification-exceedance-probabilities_AR6-MAGICC7_AR6-FaIR}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Surface-Temperature--GSAT-_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3.pdf}
\caption{
    As in Supplementary Figure \ref{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}, except for median surface air temperature (GSAT).
}
\label{fig:Surface-Temperature--GSAT-_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-CO2_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3.pdf}
\caption{
    As in Supplementary Figure \ref{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}, except for median \CO2 effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-CO2_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Atmospheric-Concentrations-CO2_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3.pdf}
\caption{
    As in Supplementary Figure \ref{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}, except for median \CO2 atmospheric concentrations.
}
\label{fig:Atmospheric-Concentrations-CO2_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-Aerosols_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3.pdf}
\caption{
    As in Supplementary Figure \ref{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}, except for median aerosol effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-Aerosols_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-CH4_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3.pdf}
\caption{
    As in Supplementary Figure \ref{fig:230_Effective-Radiative-Forcing-Basket-Anthropogenic_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}, except for median methane effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-CH4_50_SR1-5-calibration-SR1-5-processing-MAGICC6_RCMIP-Phase-2-calibration-SR1-5-processing-MAGICCv7-5-3}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-CO2_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6.pdf}
\caption{
    As in Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}, except for median \CO2 effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-CO2_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Atmospheric-Concentrations-CO2_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6.pdf}
\caption{
    As in Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}, except for median \CO2 atmospheric concentrations.
}
\label{fig:Atmospheric-Concentrations-CO2_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-Aerosols_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6.pdf}
\caption{
    As in Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}, except for median aerosol effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-Aerosols_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}
\end{figure}


\begin{figure}
% \setfigurenum{S1} %%You can change number for each figure if you want, not required. "S" prepended automatically.
\noindent\includegraphics[width=\textwidth]{230_Effective-Radiative-Forcing-CH4_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6.pdf}
\caption{
    As in Supplementary Figure \ref{fig:Effective-Radiative-Forcing-Basket-Anthropogenic_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}, except for median methane effective radiative forcing.
}
\label{fig:Effective-Radiative-Forcing-CH4_50_AR6-calibration-SR1-5-processing-MAGICCv7-5-3_SR1-5-calibration-SR1-5-processing-MAGICC6}
\end{figure}



% \begin{sidewaystable}
% \settablenum{S1 (cont.)}
% \caption{
%     \SONECAP{}
% }
% % \label{tab:assessed_ranges_relative_differences}
% % \small
% \input{summary-table-absolute-1.tex}
% \end{sidewaystable}

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

% enter figures and tables below here: %%%%%%%
%
%
%
%
% 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}

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

% 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
% a section 2, or a section 2.3.1 without a section 2.3.2.
% Please make sure your section numbers are balanced.
% ---------------
% Level 1 head
%
% Use the \section{} command to identify level 1 heads;
% type the appropriate head wording between the curly
% brackets, as shown below.
%
%An example:
%\section{Level 1 Head: Introduction}
%
% ---------------
% Level 2 head
%
% Use the \subsection{} command to identify level 2 heads.
%An example:
%\subsection{Level 2 Head}
%
% ---------------
% Level 3 head
%
% Use the \subsubsection{} command to identify level 3 heads
%An example:
%\subsubsection{Level 3 Head}
%
%---------------
% Level 4 head
%
% Use the \subsubsubsection{} command to identify level 3 heads
% An example:
%\subsubsubsection{Level 4 Head} An example.
%
%% ------------------------------------------------------------------------ %%
%
%  IN-TEXT LISTS
%
%% ------------------------------------------------------------------------ %%
%
% Do not use bulleted lists; enumerated lists are okay.
% \begin{enumerate}
% \item
% \item
% \item
% \end{enumerate}
%
%% ------------------------------------------------------------------------ %%
%
%  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
%  be automatically numbered, e.g.,:
%  \begin{equation}
%  x^2=y^2 + z^2
%  \end{equation}

% IF YOU HAVE MULTI-LINE EQUATIONS, PLEASE
% BREAK THE EQUATIONS INTO TWO OR MORE LINES
% OF SINGLE COLUMN WIDTH (20 pc, 8.3 cm)
% using double backslashes (\\).

% To create multiline equations, use the
% \begin{eqnarray} and \end{eqnarray} environment
% 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
% (+, -, etc.) if possible, with the sign of operation
% on the new line.

% Indent second and subsequent lines to align with
% the first character following the equal sign on the
% first line.

% Use an \hspace{} command to insert horizontal space
% into your equation if necessary. Place an appropriate
% unit of measure between the curly braces, e.g.
% \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
% an equation.

% To explicitly number an equation, type \eqnum{}
% (with the desired number between the brackets)
% after the \begin{equation} or \begin{eqnarray}
% command.  The \eqnum{} command will affect only
% the equation it appears with; LaTeX will number
% any equations appearing later in the manuscript
% 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}
%
%
