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Fuel Indexes: A Novel Method for the Evaluation of Relevant ...

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Energy & <strong>Fuel</strong>sArticleFigure 10. Molar (K + Na)/[x(2S + Cl)] ratio versus HCl emissions and <strong>the</strong> conversion <strong>of</strong> fuel Cl to HCl. Explanation: both correlations are notstatistically significant.Figure 11. Molar Si/(Ca + Mg) ratio versus ash-sintering temperature<strong>for</strong> different biomass fuels. Explanation: if grass pellets are excluded,<strong>the</strong> correlation is statistically significant (p < 0.05); ash-sinteringtemperature according to prCEN/TS 15370-1.<strong>of</strong> fuel N to NO x emissions has been derived, showing anonlinear correlation <strong>of</strong> <strong>the</strong> NO x emissions with rising fuel Ncontent. When this correlation is applied, a first estimation <strong>of</strong><strong>the</strong> NO x emissions can be made. During combustion, easilyvolatile and semi-volatile elements (K, Na, S, Cl, Zn, and Pb)are partly released from <strong>the</strong> fuel to <strong>the</strong> gas phase, where <strong>the</strong>yundergo chemical reactions and finally contribute to problemsconcerning emissions, deposit <strong>for</strong>mation, and corrosion. With adecreasing molar 2S/Cl ratio, <strong>for</strong> instance, <strong>the</strong> amount <strong>of</strong>alkaline chlorides in ash deposits on heat-exchanger surfacesincreases. According to <strong>the</strong> literature, 25 a molar ratio <strong>of</strong> 2S/Cl 0.5, it is very likely that most S and Cl will be embedded in <strong>the</strong>ashes. The molar ratio <strong>of</strong> Si/(Ca + Mg) can provide firstin<strong>for</strong>mation about ash-melting tendencies in systems dominatedby Si, Ca, Mg, and K (decreasing melting temperatureswith an increasing value). The molar ratio <strong>of</strong> (Si + P + K)/(Ca+ Mg) is also valid <strong>for</strong> P-rich fuels and is <strong>the</strong>re<strong>for</strong>e an index thatcan generally be applied regarding <strong>the</strong> pre-evaluation <strong>of</strong> ashmeltingtendencies.Jdx.doi.org/10.1021/ef201282y | Energy <strong>Fuel</strong>s XXXX, XXX, XXX−XXX

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