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</o:shapelayout></xml><![endif]--></head><body lang=EN-US link=blue vlink=purple><div class=WordSection1><p class=MsoNormal><b><span style='font-size:14.0pt;font-family:"Times New Roman","serif";color:#000099'>2014 Living With a Star (LWS) Science Meeting: <o:p></o:p></span></b></p><p class=MsoNormal><b><i><span style='font-size:14.0pt;font-family:"Times New Roman","serif";color:#000099'>“Evolving Solar Activity and Its Influence on Space and Earth”<o:p></o:p></span></i></b></p><p class=MsoNormal><b><span style='font-size:14.0pt;font-family:"Times New Roman","serif";color:#000099'>Nov. 2-6, 2014 * Portland, Oregon<o:p></o:p></span></b></p><p class=MsoNormal style='text-align:justify'><span style='font-size:12.0pt;font-family:"Times New Roman","serif"'><o:p> </o:p></span></p><p class=MsoNormal><a href="http://lws-sdo-workshops.org"><b><span style='font-size:12.0pt;font-family:"Times New Roman","serif";color:#7030A0'>http://lws-sdo-workshops.org</span></b></a><b><span style='font-size:12.0pt;font-family:"Times New Roman","serif";color:#7030A0'>/<o:p></o:p></span></b></p><p class=MsoNormal><span style='color:red'><o:p> </o:p></span></p><p class=MsoNormal style='margin-top:.1pt;mso-para-margin-top:.01gd'><span style='font-family:"Times New Roman","serif"'>The 2014 Living with a Star (LWS) Science Meeting will focus on advancing the understanding of the integral system coupling the Sun to the Earth. An important part of this meeting is the inclusion of the Hinode-8 and IRIS-2 meetings with complementary objectives towards improved understanding of the evolving solar activity.<o:p></o:p></span></p><p class=MsoNormal><span style='font-family:"Times New Roman","serif"'><o:p> </o:p></span></p><p class=MsoNormal><b><u><span style='font-family:"Times New Roman","serif"'>Call for Abstracts – Due: August 1, 2014<o:p></o:p></span></u></b></p><p class=MsoNormal><span style='font-family:"Times New Roman","serif"'>The agenda for this interactive 4-day meeting consists of plenary sessions with keynote presentations, as well as many additional splinter and poster sessions. Presentations will be oral, standard poster, and e-poster. We encourage your participation and hope that you will share this announcement with colleagues.<o:p></o:p></span></p><p class=MsoNormal><span style='color:red'><o:p> </o:p></span></p><p class=MsoNormal style='text-align:justify'><span style='font-family:"Times New Roman","serif";mso-fareast-language:JA'>The eight session themes planned for this meeting focus on coupling throughout the heliosphere and are science themes common to many heliophysics disciplines:<o:p></o:p></span></p><p class=MsoNormal style='mso-margin-top-alt:.1pt;margin-right:0in;margin-bottom:0in;margin-left:27.0pt;margin-bottom:.0001pt;mso-margin-top-alt:.01gd;mso-para-margin-right:0in;mso-para-margin-bottom:0in;mso-para-margin-left:27.0pt;mso-para-margin-bottom:.0001pt;text-indent:-13.5pt;line-height:115%;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif"'>Magnetic Energy and Field from Solar Interior to Corona and Heliosphere<o:p></o:p></span></p><p class=MsoNormal style='margin-left:27.0pt;text-indent:-13.5pt;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol;mso-fareast-language:JA'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif";mso-fareast-language:JA'>Reconnection and Magnetic Instabilities in Geospace, Heliosphere, and the Solar Atmosphere<o:p></o:p></span></p><p class=MsoNormal style='mso-margin-top-alt:.1pt;margin-right:0in;margin-bottom:0in;margin-left:27.0pt;margin-bottom:.0001pt;mso-margin-top-alt:.01gd;mso-para-margin-right:0in;mso-para-margin-bottom:0in;mso-para-margin-left:27.0pt;mso-para-margin-bottom:.0001pt;text-indent:-13.5pt;line-height:115%;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif"'>Evolving Coronal Mass Ejections from Corona, through the Heliosphere, into Geospace<o:p></o:p></span></p><p class=MsoNormal style='margin-left:27.0pt;text-indent:-13.5pt;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol;mso-fareast-language:JA'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif";mso-fareast-language:JA'>Dynamics of Energetic Particles, Wave-Particle Interactions, Shocks, and Turbulence<o:p></o:p></span></p><p class=MsoNormal style='margin-left:27.0pt;text-indent:-13.5pt;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol;mso-fareast-language:JA'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif";mso-fareast-language:JA'>Ion-Neutral Interactions within Earth’s Atmosphere and the Solar Atmosphere<o:p></o:p></span></p><p class=MsoNormal style='mso-margin-top-alt:.1pt;margin-right:0in;margin-bottom:0in;margin-left:27.0pt;margin-bottom:.0001pt;mso-margin-top-alt:.01gd;mso-para-margin-right:0in;mso-para-margin-bottom:0in;mso-para-margin-left:27.0pt;mso-para-margin-bottom:.0001pt;text-indent:-13.5pt;line-height:115%;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif"'>Heliosphere-Magnetosphere Interactions from Bowshock to Geotail <o:p></o:p></span></p><p class=MsoNormal style='mso-margin-top-alt:.1pt;margin-right:0in;margin-bottom:0in;margin-left:27.0pt;margin-bottom:.0001pt;mso-margin-top-alt:.01gd;mso-para-margin-right:0in;mso-para-margin-bottom:0in;mso-para-margin-left:27.0pt;mso-para-margin-bottom:.0001pt;text-indent:-13.5pt;line-height:115%;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif"'>Origins of Solar Magnetic Fields, Variability, and Effects at Earth</span><span style='font-family:"Times New Roman","serif"'> <o:p></o:p></span></p><p class=MsoNormal style='mso-margin-top-alt:.1pt;margin-right:0in;margin-bottom:0in;margin-left:27.0pt;margin-bottom:.0001pt;mso-margin-top-alt:.01gd;mso-para-margin-right:0in;mso-para-margin-bottom:0in;mso-para-margin-left:27.0pt;mso-para-margin-bottom:.0001pt;text-indent:-13.5pt;line-height:115%;mso-list:l0 level1 lfo2'><![if !supportLists]><span style='font-family:Symbol'><span style='mso-list:Ignore'>·<span style='font:7.0pt "Times New Roman"'> </span></span></span><![endif]><span style='font-family:"Times New Roman","serif"'>Modeling and Forecasting Space Climate and Space Weather Events<o:p></o:p></span></p><p class=MsoNormal style='text-align:justify'><span style='font-family:"Times New Roman","serif";mso-fareast-language:JA'><o:p> </o:p></span></p><p class=MsoNormal><span style='font-size:10.0pt'>Thanks,<o:p></o:p></span></p><p class=MsoNormal><span style='font-size:10.0pt'>Vanessa George<o:p></o:p></span></p><p class=MsoNormal><span style='font-size:10.0pt'>LASP, Univ. of Colorado, Boulder<o:p></o:p></span></p><p class=MsoNormal><span style='font-size:10.0pt'>303-492-5486</span><o:p></o:p></p><p class=MsoNormal><span style='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></div></body></html>