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000017488 084__ $$2WoS$$aChemistry, Multidisciplinary
000017488 084__ $$2WoS$$aEnergy & Fuels
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000017488 1001_ $$0P:(DE-Juel1)129164$$aVogel, B.$$b0$$uFZJ
000017488 245__ $$aImpact of a possible future global hydrogen economy on Arctic stratospheric ozone loss
000017488 260__ $$aCambridge$$bRSC Publ.$$c2012
000017488 300__ $$a6445 - 6452
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000017488 440_0 $$025784$$aEnergy & Environmental Science$$v5$$y4
000017488 500__ $$3POF3_Assignment on 2016-02-29
000017488 500__ $$aThe authors gratefully acknowledge Piers Forster for giving an introduction to the radiative transfer model RAD and for helpful discussions about the radiative forcing calculations. We would like to thank Karlheinz Nogai for assisting with figures. The work by B. Vogel was partly funded by the European Commission as part of the project "A European Network for Atmospheric Hydrogen Observations and Studies (EUROHYDROS)" under contract 036916.
000017488 520__ $$aThe potential role of molecular hydrogen (H-2) as a future alternative energy carrier has generated widespread interest. The possible amount of additional hydrogen emission into the atmosphere in a hydrogen-based economy depends on future hydrogen production and leakage rates throughout the complete process chain. However, the expected emissions are highly uncertain. Based on the current literature an upper limit is estimated. Additional hydrogen emissions yield enhanced water vapor concentrations in the stratosphere which will have an impact on stratospheric temperatures and on polar ozone loss. Both stratospheric water vapor and ozone are important drivers of climate change. The potential environmental risks are described and assessed to be low compared to the environmental benefits.
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000017488 7001_ $$0P:(DE-HGF)0$$aFeck, T.$$b1
000017488 7001_ $$0P:(DE-Juel1)129122$$aGrooß, J.-U.$$b2$$uFZJ
000017488 7001_ $$0P:(DE-Juel1)129145$$aRiese, M.$$b3$$uFZJ
000017488 773__ $$0PERI:(DE-600)2439879-2$$a10.1039/c2ee03181g$$gVol. 5, p. 6445 - 6452$$p6445 - 6452$$q5<6445 - 6452$$tEnergy & environmental science$$v5$$x1754-5692$$y2012
000017488 8567_ $$uhttp://dx.doi.org/10.1039/C2EE03181G
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