\documentclass[10pt]{article}

\usepackage{fullpage}
\usepackage{setspace}
\usepackage{parskip}
\usepackage{titlesec}
\usepackage[section]{placeins}
\usepackage{xcolor}
\usepackage{breakcites}
\usepackage{lineno}
\usepackage{hyphenat}





\PassOptionsToPackage{hyphens}{url}
\usepackage[colorlinks = true,
            linkcolor = blue,
            urlcolor  = blue,
            citecolor = blue,
            anchorcolor = blue]{hyperref}
\usepackage{etoolbox}
\makeatletter
\patchcmd\@combinedblfloats{\box\@outputbox}{\unvbox\@outputbox}{}{%
  \errmessage{\noexpand\@combinedblfloats could not be patched}%
}%
\makeatother


\usepackage{natbib}




\renewenvironment{abstract}
  {{\bfseries\noindent{\abstractname}\par\nobreak}\footnotesize}
  {\bigskip}

\titlespacing{\section}{0pt}{*3}{*1}
\titlespacing{\subsection}{0pt}{*2}{*0.5}
\titlespacing{\subsubsection}{0pt}{*1.5}{0pt}


\usepackage{authblk}


\usepackage{graphicx}
\usepackage[space]{grffile}
\usepackage{latexsym}
\usepackage{textcomp}
\usepackage{longtable}
\usepackage{tabulary}
\usepackage{booktabs,array,multirow}
\usepackage{amsfonts,amsmath,amssymb}
\providecommand\citet{\cite}
\providecommand\citep{\cite}
\providecommand\citealt{\cite}
% You can conditionalize code for latexml or normal latex using this.
\newif\iflatexml\latexmlfalse
\providecommand{\tightlist}{\setlength{\itemsep}{0pt}\setlength{\parskip}{0pt}}%

\AtBeginDocument{\DeclareGraphicsExtensions{.pdf,.PDF,.eps,.EPS,.png,.PNG,.tif,.TIF,.jpg,.JPG,.jpeg,.JPEG}}

\usepackage[utf8]{inputenc}
\usepackage[ngerman,english]{babel}



\usepackage{float}








\begin{document}

\title{Seasonal Variations of Soil Thermal Conductivity at the InSight Landing
Site}



\author[1]{Matthias Grott}%
\author[2]{Sylvain Piqueux}%
\author[3]{Tilman Spohn}%
\author[1]{Joerg Knollenberg}%
\author[4]{Christian Krause}%
\author[2]{Eloise Marteau}%
\author[2]{Troy L. Hudson}%
\author[5]{Francois Forget}%
\author[6]{Lucas Lange}%
\author[7]{N. Müller}%
\author[2]{Matthew P. Golombek}%
\author[8]{Seiichi Nagihara}%
\author[9]{Paul Morgan}%
\author[10]{J.P. Murphy}%
\author[11]{Matthew Adam Siegler}%
\author[12]{Scott D. King}%
\author[13]{Donald Banfield}%
\author[2]{Suzanne E Smrekar}%
\author[2]{William Bruce Banerdt}%
\affil[1]{DLR Institute for Planetary Research}%
\affil[2]{Jet Propulsion Laboratory}%
\affil[3]{Institute of  Planetary Research}%
\affil[4]{DLR Institute of Space Systems}%
\affil[5]{Laboratoire de Meteorologie Dynamique}%
\affil[6]{Laboratoire de Météorologie Dynamique,Institut Pierre-Simon Laplace (LMD/IPSL), Sorbonne Université, Centre National de la Recherche Scientifique (CNRS), École Polytechnique, École Normale Supérieure (ENS), Paris, France}%
\affil[7]{German Aerospace Center (DLR), Institute of Planetary Research}%
\affil[8]{Texas Tech University}%
\affil[9]{Colorado School of Mines}%
\affil[10]{Virginia Polytechnic Institute and State University}%
\affil[11]{Planetary Sciences Institute}%
\affil[12]{Virginia Tech}%
\affil[13]{Cornell}%


\vspace{-1em}



  
  \date{May 18, 2024}


\begingroup
\let\center\flushleft
\let\endcenter\endflushleft
\maketitle
\endgroup





\selectlanguage{english}
\begin{abstract}
The heat flow and physical properties package measured soil thermal
conductivity at the landing site in the 0.03 to 0.37 m depth range. Six
measurements spanning solar longitudes from
8.0\$\^{}\textbackslash{}circ\$ to 210.0\$\^{}\textbackslash{}circ\$
were made and atmospheric pressure at the site was simultaneously
measured using InSight's Pressure Sensor. We find that soil thermal
conductivity strongly correlates with atmospheric pressure. This trend
is compatible with predictions of the pressure dependence of thermal
conductivity for unconsolidated soils under martian atmospheric
conditions, indicating that heat transport through the pore filling gas
is a major contributor to the total heat transport. This implies that
any cementation or induration of the soil sampled by the experiments
must be minimal and that the soil surrounding the mole at depths below
the duricrust is unconsolidated. Thermal conductivity data presented
here are the first direct evidence that the atmosphere interacts with
the top most meter of material on Mars.%
\end{abstract}%



\sloppy


\selectlanguage{english}
\begin{figure}[H]
\begin{center}
\includegraphics[width=0.70\columnwidth]{figures/954581-0-figure-10639762-rdtyw9/954581-0-figure-10639762-rdtyw9}

\end{center}
\end{figure}\selectlanguage{english}
\begin{figure}[H]
\begin{center}
\includegraphics[width=0.70\columnwidth]{figures/954581-0-supp-10639763-rxtyw9/954581-0-supp-10639763-rxtyw9}

\end{center}
\end{figure}\selectlanguage{english}
\begin{figure}[H]
\begin{center}
\includegraphics[width=0.70\columnwidth]{figures/954581-0-figure-10639764-r5tyw9/954581-0-figure-10639764-r5tyw9}

\end{center}
\end{figure}\selectlanguage{english}
\begin{figure}[H]
\begin{center}
\includegraphics[width=0.70\columnwidth]{figures/954581-0-figure-10639765-rptyw9/954581-0-figure-10639765-rptyw9}

\end{center}
\end{figure}

\selectlanguage{english}
\FloatBarrier
\end{document}

