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<p class=MsoNormal>Dear <span style='color:#1F497D'>CEDAR</span> Editor<o:p></o:p></p>
<p class=MsoNormal><o:p> </o:p></p>
<p class=MsoNormal>We would be grateful if you would distribute the message
below in the <span style='color:#1F497D'>CEDAR</span> newsletter.<o:p></o:p></p>
<p class=MsoNormal><o:p> </o:p></p>
<p class=MsoNormal>Best wishes,<o:p></o:p></p>
<p class=MsoNormal>jesper<o:p></o:p></p>
<p class=MsoNormal><o:p> </o:p></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>~~~~~~~~~~~~~~~~~~~~~~<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>Jesper
W. Gjerloev, Ph.D.<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'> Senior
Staff Scientist<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'> PI
- SuperMAG Initiative<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'> Applied
Physics Laboratory<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'> Johns
Hopkins University<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'> 11100
Johns Hopkins Road<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'> Laurel,
MD 20723-6099<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'><o:p> </o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>Work
Phone : +1 240 228 5014<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>Work
FAX : +1 240 228 1641<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>E-mail:
<a href="mailto:jesper.gjerloev@jhuapl.edu">jesper.gjerloev@jhuapl.edu</a><o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>SuperMAG:
<a href="http://supermag.jhuapl.edu">http://supermag.jhuapl.edu</a><o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'><o:p> </o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>-->
I used to be indecisive but now I am not sure.<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:10.0pt;font-family:"Arial","sans-serif"'>~~~~~~~~~~~~~~~~~~~~~~<o:p></o:p></span></p>
<p class=MsoNormal><o:p> </o:p></p>
<p class=MsoNormal><o:p> </o:p></p>
<p class=MsoNormal>-----------------------------------------<o:p></o:p></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Dear colleagues,<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Please note the session on " Auroral Forms And Their Role In
The Dungey Convection Cycle", to be held at the upcoming AGU 2010 Fall
Meeting, 13–17 December 2010, in San Francisco. Papers based on
observations from ground-based or space assets, theoretical studies, or
simulations/modeling are all welcome.<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Best regards,<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Jesper W Gjerloev, Brian Anderson, Larry Lyons, and William Lotko<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>AGU Fall Meeting 2010<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>SM13: Auroral Forms And Their Role In The Dungey Convection Cycle<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Sponsor: SPA-Magnetospheric Physics <o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Co-Sponsor: SPA-Aeronomy<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoNormal><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black;text-transform:uppercase'>AURORAL FORMS and their role in THE
DUNGEY CONVECTION CYCLE<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Closing the Dungey global convection cycle is a fundamental space
physics problem that all driven magnetospheres have to resolve. At Earth this
cycle is intimately tied to the electrodynamics of the meso-scale auroral forms
seen in the nighttime sector. These recurrent forms are associated with
the field-aligned currents which determine the pattern and degree of return
flow on the nightside. The closure processes spawn a multitude of
scale sizes whose roles in energy and momentum transport are not currently
understood. Papers based on observations from ground-based or space assets,
theoretical studies, or simulations/modeling are all welcome.<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Abstract submission for the AGU Fall Meeting 2010 is now open. <o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Submission deadline of Thursday 2 September 2010. <o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Also note that Friday 27 August is the last day to join the AGU in
order to submit an abstract as a member. More details will be posted on the AGU
fall meeting website at <a href="http://www.agu.org/meetings/fm10/"><span
style='color:black'>http://www.agu.org/meetings/fm10/</span></a>.<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Convenors:<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Jesper W Gjerloev, Johns Hopkins University APL, Jesper.Gjerloev@jhuapl.edu<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Brian Anderson, Johns Hopkins University APL,
Brian.Anderson@jhuapl.edu<o:p></o:p></span></p>
<p class=MsoPlainText><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'><o:p> </o:p></span></p>
<p class=MsoNormal><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>Larry Lyons, UCLA, larry@atmos.ucla.edu<o:p></o:p></span></p>
<p class=MsoNormal><span style='font-size:12.0pt;font-family:"Times New Roman","serif";
color:black'>William Lotko, Dartmouth University, William.Lotko@dartmouth.edu<o:p></o:p></span></p>
<p class=MsoNormal><o:p> </o:p></p>
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