<div>Thanks you to all of you. Your informartion help me a lot.</div>
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<div><span class="gmail_quote">On 7/31/06, <b class="gmail_sendername">Bill Bua</b> <<a href="mailto:Bill.Bua@noaa.gov">Bill.Bua@noaa.gov</a>> wrote:</span>
<blockquote class="gmail_quote" style="PADDING-LEFT: 1ex; MARGIN: 0px 0px 0px 0.8ex; BORDER-LEFT: #ccc 1px solid">Christian --<br><br>The c00 is the T126 (spectral resolution) control run for the ensemble.<br>The others, p01, p02,...,up to p14, are perturbation runs. The
<br>perturbations are developed by using a method called ETKF (Ensemble<br>Transform Kalman Filter), where the initial conditions that will produce<br>the most spread in the ensemble are determined using statistical means.
<br>For more information on this, I'd go to:<br><br><a href="http://www.emc.ncep.noaa.gov/gmb/ens/">http://www.emc.ncep.noaa.gov/gmb/ens/</a> and then click on the link named<br>"Implementation News" toward the bottom of the page.
<br><br>Let me know if you have additional questions.<br><br>Bill<br><br>Christian Gonzalez wrote:<br>> Hello,<br>> Could anyone tell me what are the differences between gec00 y gep01,<br>> gep02, ..., gep14 for a selected hour?
<br>> <a href="http://nomad5.ncep.noaa.gov:9090/dods/gens/archive/">http://nomad5.ncep.noaa.gov:9090/dods/gens/archive/</a><br>> Thanks a lot.<br>><br>><br>> Christian Gonzalez<br>> CEPROPA<br>> Argentina
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