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<p class="MsoPlainText"><span style="font-size:12.0pt;font-family:"Times New Roman",serif">Dear Colleagues,<o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif">We would like to invite you to submit your abstracts to 2017 AGU session SA004:
</span><span style="font-size:12.0pt;font-family:"Times New Roman",serif"><br>
“Monitoring Geospace Variations Through Remote Sensing”<o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif;color:black;background:white"><a href="https://agu.confex.com/agu/fm17/preliminaryview.cgi/Session22803">https://agu.confex.com/agu/fm17/preliminaryview.cgi/Session22803</a></span><span style="font-size:12.0pt;font-family:"Times New Roman",serif"><o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif">Session ID#: </span>
<span style="font-size:12.0pt;font-family:"Times New Roman",serif">22803<o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif">Session Description:</span><span style="font-size:12.0pt;font-family:"Times New Roman",serif"><o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif">Geospace (the ionosphere, thermosphere, plasmasphere and magnetosphere) is driven by energy and momentum inputs from the Sun, internal processes within these regions, and energy from the surface
and lower atmosphere. Satellite-based remote sensing (X-ray, UV, visible, IR and radio frequencies) provides a cost-effective way to understand the system and its global response as well as those regions where in situ measurements are difficult. We welcome
all contributions on imaging techniques, data analysis, modeling/simulations for geospace studies and future sensor improvement.<o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif"><o:p> </o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif">Conveners: Yongliang Zhang, Larry J Paxton, David G Sibeck, and Robert K Schaefer<o:p></o:p></span></p>
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<span style="font-size:12.0pt;font-family:"Times New Roman",serif"><o:p> </o:p></span></p>
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