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<p> <span style=" color: #000; font-family: Verdana, Arial,
Helvetica, sans-serif; font-size: 10pt; background: #fff; ">Dear
colleagues,</span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "></span></p>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span> <span
style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span> <span
style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> We invite you to
submit an abstract to the following 2018 AGU Fall Meeting session
"<i>New and Emerging Magnetosphere-Ionosphere-Thermosphere
Coupling Science from Remote and In Situ Spacecraft
Measurements: The First 5 Years of Swarm</i>". We encourage
abstracts "</span><span style=" color: #000; font-family: Verdana,
Arial, Helvetica, sans-serif; font-size: 10pt; background: #fff; "><span
style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; ">focusing on the
major theoretical, modeling, and experimental MIT science
results from the first 5 years of Swarm and Swarm-E" in addition
to abstracts</span> "</span><span style=" color: #000;
font-family: Verdana, Arial, Helvetica, sans-serif; font-size:
10pt; background: #fff; "><span style=" color: #000; font-family:
Verdana, Arial, Helvetica, sans-serif; font-size: 10pt;
background: #fff; ">that focus on multi-point, multi-instrument
(including ground-based instruments), and/or multi-spacecraft
measurements, including those from other spacecraft missions".</span></span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "><span style="
color: #000; font-family: Verdana, Arial, Helvetica, sans-serif;
font-size: 10pt; background: #fff; "> </span></span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "><span style="
color: #000; font-family: Verdana, Arial, Helvetica, sans-serif;
font-size: 10pt; background: #fff; "> </span><b>Session ID:</b>
50201 </span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> <b>Session
Title:</b> SA014. New and Emerging
Magnetosphere-Ionosphere-Thermosphere Coupling Science from Remote
and In Situ Spacecraft Measurements: The First 5 Years of Swarm </span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "><b> </b><b>Section/Focus
Group:</b> SPA-Aeronomy </span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "><b> </b><b>View
Session Details:</b> <a moz-do-not-send="true"
href="https://agu.confex.com/agu/fm18/prelim.cgi/Session/50201">https://agu.confex.com/agu/fm18/prelim.cgi/Session/50201</a></span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> <b>Description:</b>
The Swarm constellation recently became a quartet with the
addition of the CASSIOPE Enhanced Polar Outflow Probe (e-POP) as
Swarm-E. Since their launch in the Fall of 2013, Swarm and Swarm-E
have formed the vanguard of remote and in situ diagnostics of the
coupled magnetosphere-ionosphere-thermosphere (MIT) system. As a
quartet, Swarm will enable new insight into MIT coupling processes
and wave-particle interactions across multiple spatiotemporal
scales. We solicit contributions focusing on the major
theoretical, modeling, and experimental MIT science results from
the first 5 years of Swarm and Swarm-E, as well as contributions
that identify new and emerging MIT science targets for the
mission. Papers regarding MIT coupling processes at all latitudes
are welcome. In particular, we seek contributions that focus on
multi-point, multi-instrument (including ground-based
instruments), and/or multi-spacecraft measurements, including
those from other spacecraft missions.</span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span><span
style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; ">Please note that
the abstract deadline is <b>August 1, 2018, 11:59 PM EDT</b>.
Sincerely,</span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> Gareth Perry,
University of Calgary (<a class="moz-txt-link-abbreviated"
href="mailto:perry@phys.ucalgary.ca" moz-do-not-send="true">perry@phys.ucalgary.ca</a>)</span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> Rune
Floberghagen, European Space Agency</span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span><span
style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "><span style="
color: #000; font-family: Verdana, Arial, Helvetica, sans-serif;
font-size: 10pt; background: #fff; ">David Knudsen, University
of Calgary</span></span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "><span style="
color: #000; font-family: Verdana, Arial, Helvetica, sans-serif;
font-size: 10pt; background: #fff; "> </span>Andrew Yau,
University of Calgary</span><br>
<span style=" color: #000; font-family: Verdana, Arial, Helvetica,
sans-serif; font-size: 10pt; background: #fff; "> </span><br>
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