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<p class="MsoNormal"><span style="font-size:11.0pt">Hello, <o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt">I was wondering if you could include this AGU 2021 session announcement in your next email digest. The announcement is copied below as well as attached in a word document.
<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt">Thank you so much,<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt">Adam Michael <o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
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<p class="MsoNormal"><span style="font-family:"Arial",sans-serif">Dear Colleagues,<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Arial",sans-serif"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Arial",sans-serif">We would like to draw your attention to the Fall AGU 2021 session
</span><span style="font-family:"Arial",sans-serif;color:black">“The Importance of Mesoscale Magnetotail Processes in Global and Kinetic-scale Magnetospheric Dynamics,” more info is below. The session focuses on
</span><span style="font-family:"Arial",sans-serif">the role mesoscale processes in the plasma sheet and ionosphere play in mediating interactions across geospace. For those interested, we hope you consider contributing and submit an abstract to our session.
Abstracts are due on Wednesday, August 4, 2021. <o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Arial",sans-serif;color:black"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Arial",sans-serif"><a href="https://agu.confex.com/agu/fm21/prelim.cgi/Session/121758">https://agu.confex.com/agu/fm21/prelim.cgi/Session/121758</a><o:p></o:p></span></p>
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<p class="MsoNormal"><b><span style="font-family:"Arial",sans-serif;color:black">Session ID:</span></b><span style="font-family:"Arial",sans-serif;color:black"> 121758 <br>
<b>Session Title:</b> SM031. The Importance of Mesoscale Magnetotail Processes in Global and Kinetic-scale Magnetospheric Dynamics <br>
<b>Section:</b> SPA-Magnetospheric Physics<b> <o:p></o:p></b></span></p>
<p class="MsoNormal"><b><span style="font-family:"Arial",sans-serif;color:black"> </span></b><span style="font-family:"Arial",sans-serif;color:black"><o:p></o:p></span></p>
<p class="MsoNormal"><b><span style="font-family:"Arial",sans-serif;color:black">Session Description: </span></b><span style="font-family:"Arial",sans-serif;color:#262626;background:white">Various mesoscale processes play a vital role in mediating the complex
interactions across different regions in geospace. It is important to delineate their role from, and contribution to, large-scale and kinetic-scale processes, as well as to ascertain their impacts throughout the system. For example, the explosive process of
dipolarization, which occurs on meso- and large-scales while also dissipating energy and accelerating particles via kinetic processes, is a significant component of particle transport and acceleration from the magnetotail plasma sheet to the inner magnetosphere,
current generation in the magnetosphere-ionosphere system, and wave generation that further accelerates and/or scatter particles. It is imperative to couple the outer- and inner-magnetosphere with each other and the ionosphere by understanding these processes.
This session solicits contributions using in situ and/or ground-based observations as well as global and regional models and theory that incorporate mesoscale processes to examine their impacts<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Arial",sans-serif;color:#262626;background:white"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Arial",sans-serif;color:#262626;background:white">Conveners: Christine Gabrielse, Slava Merkin, David Malaspina, Adam Michael</span><span style="font-family:"Arial",sans-serif;color:black"><o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
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