<div dir="ltr">
<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">Dear </span><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">Colleagues</span><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">,<span></span></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB"><span> </span></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;text-indent:12pt;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">The AGU Fall Meeting is
returning to San Francisco this year (9-13 December 2019), with its centennial
edition. Planetary sciences are part of the celebrations. We would be delighted
if you consider your participation and </span><span style="font-family:"Times New Roman",serif;color:black" lang="FR">encourage
submissions of cross-disciplinary presentations </span><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">in our session <b>P028: </b><b>Planetary
Atmospheres and Evolution. <span></span></b></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;text-indent:12pt;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">The deadline for abstract
submission will be <b>Wednesday 31 July 2019. </b>The goals and objectives of
the session are presented below.<span></span></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;text-indent:12pt;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">Please pass this invitation to
your colleagues who might be interested, and of course we are happy to answer
any questions that you might have. We hope to see you in San Francisco!</span><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB"><span></span></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB"><span> </span></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">Best regards,<span></span></span></p>

<p class="MsoNormal" style="margin:0cm 0cm 0.0001pt;text-align:justify;line-height:normal;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;font-family:"Times New Roman",serif" lang="EN-GB">Feng, Cedric
and Vladimir<span></span></span></p>

<p class="MsoNormal" style="text-align:justify;margin:0cm 0cm 10pt;line-height:115%;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB"><span> </span></span></p>

<p class="MsoNormal" style="text-align:justify;margin:0cm 0cm 10pt;line-height:115%;font-size:11pt;font-family:"Calibri",sans-serif"><span class="gmail-m_-1288664183002484785gmail-finalnumber"><b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="FR">P028</span></b></span><b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="FR">
- Planetary Atmospheres and Evolution</span></b><b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="FR"> </span></b><b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB"><span></span></span></b></p>

<p class="MsoNormal" style="text-align:justify;margin:0cm 0cm 10pt;line-height:115%;font-size:11pt;font-family:"Calibri",sans-serif"><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB">(</span><span lang="FR"><a href="https://agu.confex.com/agu/fm19/prelim.cgi/Session/79425" style="color:blue;text-decoration:underline" target="_blank"><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB">https://agu.confex.com/agu/fm19/prelim.cgi/Session/79425</span></a></span><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB">)<span></span></span></p>

<p class="MsoNormal" style="text-align:justify;margin:0cm 0cm 10pt;line-height:115%;font-size:11pt;font-family:"Calibri",sans-serif"><span class="gmail-m_-1288664183002484785gmail-topdisplay"><b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB">Description:</span></b></span><span class="gmail-m_-1288664183002484785gmail-topdisplay"><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB"> </span></span><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="FR">Understanding the nature
and variability of (exo)planetary atmospheres, the physical mechanisms
governing these atmospheres, and their chemical evolution are strong driving
forces of planetary science and solar system exploration mission planning.
While the long-term evolution of the Earth is constrained by geological studies
and isotopic analyses, the evolutionary paths of other planets must be
reconstructed from data obtained through astronomical observations and
planetary missions. Models of planetary atmospheres use these observations to
illuminate governing physical processes operating from the Earth to other planets
in our solar system and beyond. The rapidly increasing number of discovered
exoplanets provides a new opportunity for interdisciplinary collaborations
between heliophysicists, astrophysicists, geoscientists, biochemists, planetary
and climate scientists concerning the physical and chemical evolution of
(exo)planetary atmospheres and planetary habitability. This session welcomes
observational, theoretical, experimental, and field studies relevant to the
atmospheres, evolution, and habitability of planets in and outside of our solar
system.<span></span></span></p>

<p class="MsoNormal" style="text-align:justify;margin:0cm 0cm 10pt;line-height:115%;font-size:11pt;font-family:"Calibri",sans-serif"><b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB">Convenors:</span></b><span style="font-size:12pt;line-height:115%;font-family:"Times New Roman",serif" lang="EN-GB"> <span class="gmail-m_-1288664183002484785gmail-topdisplay"><b>Feng Tian</b> (Macau
University of Science and Technology), <b>Cedric Gillmann </b>(Free University
of Belgium) and <b>Vladimir Airapetian</b> (NASA Goddard Space Flight Center/SEEC
& American University).</span></span></p>

</div><div dir="ltr"><br></div><br><div class="gmail_quote"><div dir="ltr" class="gmail_attr">On Thu, Jul 11, 2019 at 2:40 AM Gauthier Hulot via Cedar_email <<a href="mailto:cedar_email@mailman.ucar.edu" target="_blank">cedar_email@mailman.ucar.edu</a>> wrote:<br></div><blockquote class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><div><div><div style="margin:0in 0in 0.0001pt"><span style="font-size:14px">Dear colleagues,</span></div><div style="margin:0in 0in 0.0001pt"><span style="font-size:14px"><br></span></div><div style="margin:0in 0in 0.0001pt"><span style="font-size:14px">If you intend to attend AGU this fall, please consider submitting (BEFORE JULY 31, 2019) an abstract to the session below to present your latest results and contribute to some exciting discussion </span><span style="font-size:14px">about what we believe is a bright future for space magnetometry ! </span></div><div style="margin:0in 0in 0.0001pt"><span style="font-size:14px"> </span></div></div><div><b><span class="gmail-m_4639280454536064050gmail-m_-4120694960625586974finalNumber" style="font-size:14px">GP010</span><span style="font-size:14px"> </span><span style="font-size:14px">- Investigating Earth Processes Using Low Earth Orbiting Space Magnetometry, Successes and Opportunities</span></b></div><div><div><span style="font-size:14px"><br></span></div><div><span style="font-size:14px">Over the past 40 years, missions such as Magsat, Oersted, Champ and the ongoing Swarm mission have demonstrated the unique ability of Low Earth Orbiting (LEO) missions with magnetometry and ionospheric sensing payloads for investigating a wide variety of Earth processes, ranging from the geodynamo to the coupling between the ionosphere, thermosphere and magnetosphere. Recent opportunities have also arisen for increasing our ability to monitor and investigate these, and other, processes using data from LEO magnetometry and companion payloads, such as those from the e-POP instrument of the Canadian Space Agency's CASSIOPE mission, from the Chinese Seismo-Electromagnetic Satellite recently launched, and from platform magnetometers routinely used on many LEO satellites as part of attitude control subsystem. This session invites contributions illustrating the achievements of such LEO magnetometry for investigating all types of Earth processes, as well as contributions describing ongoing initiatives towards designing innovative new LEO magnetometry missions.</span></div><div><span style="font-size:14px"><br></span></div><div><span style="font-size:14px">Conveners: G. Hulot (IPGP, France), P. Alken (University of Colorado, USA), X. Shen (Institute for Crustal Dynamics, China Earthquake Administration, China)</span></div></div><div><span style="font-size:14px"><br></span></div><div><span style="font-size:14px">More details on the session can be found here: <a href="https://agu.confex.com/agu/fm19/prelim.cgi/Session/80436" target="_blank">https://agu.confex.com/agu/fm19/prelim.cgi/Session/80436</a></span></div></div>_______________________________________________<br>
Cedar_email mailing list<br>
<a href="mailto:Cedar_email@mailman.ucar.edu" target="_blank">Cedar_email@mailman.ucar.edu</a><br>
<a href="http://mailman.ucar.edu/mailman/listinfo/cedar_email" rel="noreferrer" target="_blank">http://mailman.ucar.edu/mailman/listinfo/cedar_email</a></blockquote></div>