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<p class="MsoNormal">Dear Colleagues,</p>
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<p class="MsoNormal">We are excited to invite you to participate in Session SA011 at the 2014 AGU Fall Meeting. This session will focus on the intriguing differences between the Northern and Southern Hemispheres within the atmosphere-ionosphere-magnetosphere
system. Studies targeting on understanding their characteristics, mechanisms and impacts are welcome. The deadline for the abstract submission is July 31 23:59 EDT/03:59 +1 GMT, and you can submit the abstract through
<a href="https://agu.confex.com/agu/agu24/prelim.cgi/Session/224002">https://agu.confex.com/agu/agu24/prelim.cgi/Session/224002</a>.</p>
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<p class="MsoNormal">Here is a brief overview of the session:</p>
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<p class="MsoNormal"><b><span style="color:#212121">SA011- Exploring Interhemispheric Asymmetries in the Atmosphere-Ionosphere-Magnetosphere System: Characteristics, Mechanisms, and Impacts</span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<p class="MsoNormal" style="border:none;padding:0in"><span style="color:#212121">The atmosphere-ionosphere-magnetosphere (AIM) system exhibits intriguing interhemispheric asymmetries (IHA) across various spatiotemporal scales, posing fundamental questions about
their characteristics, drivers, and impacts. This session aims to gather studies based on observations, modeling efforts, and data analysis techniques to deepen our understanding of IHA generations and their broader impacts on the coupled AIM system. Topics
of interest include but are not limited to: 1) Elucidating IHA characteristics in the AIM system during varied geophysical conditions; 2) Investigating the formation mechanisms of IHA characteristics within the AIM system; 3) Assessing the impacts of IHA in
one regime on other regimes in the coupled AIM system; 4) Understanding the significance of the IHA in the AIM system to space weather. Contributions are anticipated to enhance our grasp of IHA complexities, thus informing predictive models and space weather
forecasts, refining mitigation strategies, and complementing future Geospace Dynamics Constellation (GDC) and DYNAMIC missions.</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<p class="MsoNormal">Looking forward to your contributions to the AGU session SA011. Please let us know if you have any questions.
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<p class="MsoNormal">Regards,</p>
<p class="MsoNormal">Qingyu Zhu</p>
<p class="MsoNormal">On behalf of Lynn Harvey, Yue Deng, Daniel Welling and Yun-ju Chen
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<p class="MsoNormal"><span style="font-family:"Calibri",sans-serif">Qingyu Zhu, Ph.D.<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Calibri",sans-serif">Assistant Professor of Physics<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Calibri",sans-serif">University of Texas at Dallas<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:"Calibri",sans-serif">Email: <a href="mailto:qingyu.zhu@utdallas.edu">
<span style="color:#0563C1">qingyu.zhu@utdallas.edu</span></a><o:p></o:p></span></p>
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