<html><head><base href="x-msg://5/"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">Dear All,<div><br></div><div>If you are interested in magnetic modeling of coronal loops, here some new preprints.</div><div><br></div><div>Share and enjoy,</div><div>Markus</div><div><br></div><div><br></div><div><div><div><div><span class="Apple-style-span" style="font-size: 18px;">Aschwanden,M.J. 2012, Solar Physics, (in press)</span></div><div><span class="Apple-style-span" style="font-size: 18px;">URL1="<a href="http://www.lmsal.com/~aschwand/eprints/2012_fff1.pdf">http://www.lmsal.com/~aschwand/eprints/2012_fff1.pdf</a>"</span></div><div><span class="Apple-style-span" style="font-size: 18px;"><b>A nonlinear force-free magnetic field approximation suitable for </b></span></div><div><span class="Apple-style-span" style="font-size: 18px;"><b>fast forward-fitting to coronal loops. I. Theory</b></span></div></div><div><span class="Apple-style-span" style="font-size: 18px;"><br></span></div><div><span class="Apple-style-span" style="font-size: 18px;">Aschwanden,M.J. and Malanushenko,A. 2012, Solar Physics (in press)</span></div><div><span class="Apple-style-span" style="font-size: 18px;">URL1="<a href="http://www.lmsal.com/~aschwand/eprints/2012_fff2.pdf">http://www.lmsal.com/~aschwand/eprints/2012_fff2.pdf</a>" </span></div><div><span class="Apple-style-span" style="font-size: 18px;"><b>A nonlinear force-free magnetic field approximation suitable for </b></span></div><div><span class="Apple-style-span" style="font-size: 18px;"><b>fast forward-fitting to coronal loops. II. Numeric Code and Tests</b></span></div><div><span class="Apple-style-span" style="font-size: 18px;"><br></span></div><div><div><div><span class="Apple-style-span" style="font-size: 18px;">Aschwanden,M.J., Wuelser,J.-P., Nitta,N.V., Lemen, J.R., Schrijver, C.J., DeRosa, M., and </span></div><div><span class="Apple-style-span" style="font-size: 18px;">Malanushenko, A. 2012, The Astrophysical Journal, (in press)</span></div><div><span class="Apple-style-span" style="font-size: 18px;">URL1="<a href="http://www.lmsal.com/~aschwand/eprints/2012_stereo4.pdf">http://www.lmsal.com/~aschwand/eprints/2012_stereo4.pdf</a>"</span></div><div><span class="Apple-style-span" style="font-size: 18px;">URL2="<a href="http://www.lmsal.com/~aschwand/movies/STEREO_fff_movies/">http://www.lmsal.com/~aschwand/movies/STEREO_fff_movies/</a>"</span></div><span class="Apple-style-span" style="font-size: 18px;"><b>First 3D Reconstructions of Coronal Loops with the STEREO A and B Spacecraft: <br>IV. Magnetic Field Modeling with Twisted Force-Free Fields</b></span></div></div><div><span class="Apple-style-span" style="font-size: 18px;"><br></span></div><div><span class="Apple-style-span" style="font-size: 18px;">Aschwanden,M.J., Wuelser, J.P., Nitta, N.V., and Lemen, J.R. 2012, Solar Physics (in press)</span></div><div><span class="Apple-style-span" style="font-size: 18px;">URL1="<a href="http://www.lmsal.com/~aschwand/eprints/2012_sun360.pdf">http://www.lmsal.com/~aschwand/eprints/2012_sun360.pdf</a>" </span></div><div><span class="Apple-style-span" style="font-size: 18px;"><b>Solar Stereoscopy with STEREO/EUVI A and B spacecraft from small (6 deg) </b></span></div><div><span class="Apple-style-span" style="font-size: 18px;"><b>to large (170 deg) spacecraft separation angles</b></span></div><div><div><span class="Apple-style-span" style="font-size: 18px;"><br></span></div><div><br></div></div><div><span class="Apple-style-span" style="font-size: 12px; ">_______________________________________</span></div></div><div><span class="Apple-style-span" style="font-size: 12px; "><span class="Apple-style-span" style="border-collapse: separate; -webkit-border-horizontal-spacing: 0px; -webkit-border-vertical-spacing: 0px; color: rgb(0, 0, 0); font-family: Helvetica; font-size: 12px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; -webkit-text-decorations-in-effect: none; text-indent: 0px; -webkit-text-size-adjust: auto; text-transform: none; orphans: 2; white-space: normal; widows: 2; word-spacing: 0px; "><span class="Apple-style-span" style="border-collapse: separate; -webkit-border-horizontal-spacing: 0px; -webkit-border-vertical-spacing: 0px; color: rgb(0, 0, 0); font-family: Helvetica; font-size: 12px; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; -webkit-text-decorations-in-effect: none; text-indent: 0px; -webkit-text-size-adjust: auto; text-transform: none; orphans: 2; white-space: normal; widows: 2; word-spacing: 0px; "><div>Dr. Markus J. Aschwanden</div><div>Solar & Astrophysics Laboratory</div><div>Lockheed Martin Advanced Techology Center</div><div>Org. ADBS, Bldg. 252</div><div>3251 Hanover St., Palo Alto, CA 94304, USA</div><div>Phone: 650-424-4001, FAX: 650-424-3994</div><div>URL: <a href="http://www.lmsal.com/~aschwand/">http://www.lmsal.com/~aschwand/</a></div><div>e-mail: <a href="mailto:aschwanden@lmsal.com">aschwanden@lmsal.com</a></div><div>_______________________________________</div><br class="Apple-interchange-newline"></span></span></span><br class="Apple-interchange-newline">
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