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<span style="font-size:12.0pt; color:black">CEDAR community-</span></p>
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<span style="font-size:12.0pt; color:black">Please consider submitting an abstract to the session below<a href="https://nam12.safelinks.protection.outlook.com/?url=https%3A%2F%2Fagu.confex.com%2Fagu%2Ffm22%2Fprelim.cgi%2FSession%2F159741&data=05%7C01%7CKristina.A.Lynch%40dartmouth.edu%7C8199d62af45244b5dbb708da6e57e5b7%7C995b093648d640e5a31ebf689ec9446f%7C0%7C0%7C637943621039439359%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=1wRp5FONtRUZq%2F4REi9uH45mEuHri682i4QDi8DC%2FMs%3D&reserved=0" data-auth="Verified" originalsrc="https://agu.confex.com/agu/fm22/prelim.cgi/Session/159741" shash="SRnVn4BxuyIgr89GYKpvIwrbKOI3WbyOOHOGkIzLOkE39S7Ugxww1xCpwGJQ6OYhUA8V+lvEJIewtXGKJYB5ggmePV7HBSw5RFJ1BI8jkiCTrWAteC2nawj8gtFjyiQGUrAAoZDrx4DtPBRQ4Y/qu/7qupiIJriTZ40WNraBHMM=" title="https://agu.confex.com/agu/fm22/prelim.cgi/Session/159741">
(SA009)</a> on the use of heterogeneous distributed data and data-driven simulations for auroral system science. Invited speakers will include Doug Rowland (NASA/GSFC) and Shasha Zou (Michigan).</span></p>
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<span style="font-size:12.0pt; color:black">Thank you</span></p>
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<span style="font-size:12.0pt; color:black">K Lynch (Dartmouth)</span></p>
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<span style="font-size:12.0pt; color:black">R Nikoukar (APL)</span></p>
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<span style="font-size:12.0pt; color:black">D Hampton (UAF/GI)</span></p>
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<span style="font-size:12.0pt; color:black">M Burleigh (NRL)</span></p>
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<b><span style="font-size:11.5pt; font-family:"Lucida Grande",sans-serif; color:#222222">Session Title:</span></b></p>
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<span style="font-size:11.5pt; font-family:"Lucida Grande",sans-serif; color:#222222">Distributed auroral measurements and heterogeneous-data-driven physics-based simulations for ionospheric system science</span></p>
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<b><span style="font-size:11.5pt; font-family:"Lucida Grande",sans-serif; color:#222222">Session Description:</span></b></p>
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<span style="font-size:11.5pt; font-family:"Lucida Grande",sans-serif; color:#222222">The Earth’s auroral ionosphere as a coupled, driven, and active system is governed by Maxwell’s equations and a description of plasma motions. The drivers of the auroral ionosphere
are delivered over multiple spatial and temporal scales that draw dramatically different responses in the ionosphere-thermosphere system. It is not possible to disentangle mesoscale processes of auroral arc systems with traditional single-point observations.
Ionospheric system science benefits now from (a) the advent of distributed and heterogeneous sensor platform arrays, together with (b) newly capable three-dimensional self-consistent computational models which bypass standard idealizations<span class="x_xxxxxxxxapple-converted-space"> </span>
and (c) new computational tools built on machine learning platforms. Constraining auroral system science requires distributed fine-grained observations, as well as physics-based models capable of constructing simulations consistent with a multiplicity of observations.
We welcome observational, modeling, and data science presentations that are enabled by distributed measurements of the auroral ionosphere.</span></p>
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