The Coronal Pulse Identification and Tracking Algorithm (CorPITA) for automated detection of “EIT Waves”

<div> What is the Astrophysics Research Group at TCD doing to understand Space Weather? <div> <p>Poster presented during <a href="" rel="nofollow">"The Science of Weather Forecasting"</a> conference organized by the <a href="" rel="nofollow">Irish Metereological Society</a> in Dublin on March 24, 2012.</p> <p>Extra material, bibliography and links:<br><a href="" rel="nofollow">Astrophysics Research Group</a> at <a href="" rel="nofollow">Trinity College Dublin</a><br><a href="" rel="nofollow"></a><br><a href="" rel="nofollow">Rosse Observatory</a> at <a href="" rel="nofollow">Birr Castle</a>, Co. Offaly, Ireland.<br>Space weather effects image comes from a modified version of <a href="" rel="nofollow">Jan Wera's image</a>.<br>Events on the time line comes from <a href="" rel="nofollow">Space weather effects on Communication</a> by Lanzerotti (2007) [<a href="" rel="nofollow">e-print</a>].<br>SMART code is described in <a href="" rel="nofollow">Solar Magnetic Feature Detection and Tracking for Space Weather Monitoring"</a> (Higgins et al., 2010) [<a href="" rel="nofollow">e-print</a>].<br>Magnetic extrapolation comes from a modified version of Figure 10 in <a href="" rel="nofollow">"Testing magnetofrictional extrapolation with the Titov-Démoulin model of solar active regions"</a> by Valori et al. (2010) [<a href="" rel="nofollow">e-print</a>].<br>Solar images from SOHO/EIT, SoHO/MDI, SDO/AIA and SDO/HMI instruments obtained using <a href="" rel="nofollow"></a>.<br>Radio shock observed on April 20, 1998 from <a href="" rel="nofollow">Nançay Radioheliograph</a> (France).<br>Flare model cartoon is a modifed version of <a href="" rel="nofollow"> flare diagram</a>.<br>Space weather session at <a href="" rel="nofollow">Euroscience Open Forum 2012</a> will happen at 13'30 on July 15, 2012.</p> </div> </div>
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