73 research outputs found

    Water Upconing in Underground Hydrogen Storage: Sensitivity Analysis to Inform Design of Withdrawal

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    The gas–water interface in Underground Hydrogen Storage (UHS) reservoirs creates the possibility that water will upcone to the well during hydrogen (H2) withdrawal with detrimental impacts. We study the upconing of water to a hydrogen injection/withdrawal (I/W) well using both an analytical solution and numerical simulation. We carried out sensitivity analyses of the engineered properties (e.g., distance of well bottom to gas–water interface, withdrawal rate) and the intrinsic properties (e.g., reservoir permeability, porosity) of an idealized UHS system. Horizontal permeability is the main parameter controlling the height of upconing. Daily I/W cycles to some degree mitigate upconing because injection pushes down the gas–water interface. Sampling-based global sensitivity analyses show clearly that reservoirs with large horizontal permeability are preferred for avoiding upconing. Minimizing withdrawal rate and maximizing either the distance from well to gas–water interface or the length of the perforated well interval are important engineering controls to minimize upconing

    Total Solar Irradiance measured by PREMOS/PICARD

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    We report Total Solar Irradiance (TSI) measurements made by the space experiment PREMOS on the French micro satellite PICARD and compare them to other operating TSI space experiments. PREMOS/PICARD is the first SItraceable TSI experiment in space and it confirms the value measured by TIM/SORCE that the solar constant is 1361 W/m2. We discuss the accuracy of absolute and relative measurements of TSI and conclude on the reliability of the TSI composite 1979-2012.We find that over a decade, the relative accuracy is 0.2 W/m2 and that within this uncertainty it cannot be decided whether the solar irradiance in the past solar minimum of 2008 was lower than in the minimum of 1996. Reconstructions back to 1979 have even larger uncertainties

    Gossamer roadmap technology reference study for a solar polar mission

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    A technology reference study for a solar polar mission is presented. The study uses novel analytical methods to quantify the mission design space including the required sail performance to achieve a given solar polar observation angle within a given timeframe and thus to derive mass allocations for the remaining spacecraft sub-systems, that is excluding the solar sail sub-system. A parametric, bottom-up, system mass budget analysis is then used to establish the required sail technology to deliver a range of science payloads, and to establish where such payloads can be delivered to within a given timeframe. It is found that a solar polar mission requires a solar sail of side-length 100 – 125 m to deliver a ‘sufficient value’ minimum science payload, and that a 2. 5μm sail film substrate is typically required, however the design is much less sensitive to the boom specific mass
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