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</o:shapelayout></xml><![endif]--></head><body lang=EN-US link=blue vlink=purple><div class=WordSection1><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Dear colleagues,<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p>&nbsp;</o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>We cordially invite you to submit an abstract to the special session that we are organizing at the American Geophysical Union - Meeting of the Americas to be held in Cancun, Mexico, 14-17 May 2013. Abstract submission deadline is Wednesday, 6 February, 11:59 p.m. Eastern Time. <o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p>&nbsp;</o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Meeting website: http://moa.agu.org/2013/<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p>&nbsp;</o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Session title: Equatorial Ionospheric Electrodynamics and Disturbances<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p>&nbsp;</o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Session description: The equatorial ionosphere behaves very differently under different solar and geomagnetic conditions. This session focuses on how the equatorial ionospheric plasma drift responds to magnetic storms, what determines the generation of equatorial spread F and plasma bubbles, how significantly seeding perturbations affect the generation of plasma bubbles, how the occurrence of equatorial spread F depends on longitude and solar activity, and how ionospheric scintillation is correlated with spread F irregularities. We welcome observational and simulation studies that address these topics and that aim to improve the current capability of forecasting low-latitude ionospheric disturbances, spread F irregularities, and scintillation activities.<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p>&nbsp;</o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Thank you.<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p>&nbsp;</o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Conveners<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Chaosong Huang, AFRL, US<o:p></o:p></span></p><p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'>Endawoke Yizengaw, Boston College, US<o:p></o:p></span></p></div></body></html>