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<p><strong>Abstract.</strong> Thermospheric mass densities from the GOCE (Gravity field and steady-state Ocean Circulation Explorer) satellite for Sun-synchronous orbits between 83.5°<span class="thinspace"></span>S and 83.5°<span class="thinspace"></span>N, normalized to 270<span class="thinspace"></span>km during 2009–2013, have been used to develop an empirical mass density model at dawn/dusk local solar time (LST) sectors based on the empirical orthogonal function (EOF) method. The maindoi:10.5194/angeo-36-489-2018 fatcat:usx343vharc4xdjpy52vcf3by4