687 research outputs found

    Cummings v. Barber, 136 Nev. Adv. Op. 18 (April 2, 2020)

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    State, Dep’t of Bus. & Indus. v. TitleMax, 135 Nev. Adv. Op. 44 (Sept. 26, 2019)

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    In an en banc opinion, the Nevada Supreme Court answered whether title lender TitleMax’s Grace Period Deferment Agreement (“GPPDA”), which applied to short-term, high-interest loans offered to Nevada consumers in 2014 and 2015, qualified as a true grace period under NRS 604A.210. The Court concluded that the GPPDA was not a true grace period, but was instead an impermissible extension of the 210-day loans. The Court reasoned that the GPPDA was an extension because TitleMax charged borrowers additional interest during the extended period and thus violated NRS 604A.445, a statute enacted by the Nevada Legislature in part to protect consumers from predatory lending, by explicitly forbidding the charging of additional interest during grace periods. Further, the Court concluded that TitleMax’s violation was not willful, but was instead a reasonable interpretation of the pertinent statutes, and thus sanctions were inappropriate

    Iron Oxides Synthesized in Hypersaline Solutions

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    Iron oxides were synthesized in conditions similar to those that prevail in deeps of the Red Sea (2–5M NaCl, temperatures 60–80°C, and pH 6.5–10.4). The main phase that was crystallized was submicron magnetite. Additional phases of feroxyhyte, goethite, and akagenéite were also detected. Magnetite morphology observed through high-resolution scanning electron microscopy (HRSEM) varied between euhedral plates and octahedral or unhedral crystals. The euhedral plates were probably crystallized pseudomorphically after platy green rust or Fe(OH)2 due to its quick crystallization. Size of magnetite varied between 18 and 45 nm. The addition of Si retarded crystal growth, and at Si/Fe = 0.5, short-range ordered phases are formed and not magnetite. This finding is in line with earlier laboratory experiments in which Si was found to retard goethite and lepidocrocite crystallization

    Equilibrium temperatures of mass transfer cooled walls in high-speed flow of an absorbing-emitting gas

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    Equilibrium temperatures of mass transfer cooled walls in high speed flow of absorbing-emitting ga

    Minerals Observed by Scanning Electron Microscopy (SEM), Transmission Electron Microscopy (TEM) and High Resolution Transmission Electron Microscopy (HRTEM)

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    Pictures from a scanning electron microscopy, transmission electron microscopy and high resolution microscopy are presented. Samples were collected from the marl layer in Judean Mountains in Israel, and the minerals observed were dolomite, calcite, goethite, and K-feldspar. In sands along the Mediterranean Seashore and the coastal plain in Israel, dark grains were rich in Ti, and quartz grains were covered by clays and hematite. Dust samples included clay minerals, Ti and Fe oxides. Iron oxides (goethite, akaganéite and lepidocrocite) were preserved within halite crystals at the Dead Sea area. In the Atlantis II and Thetis Deeps, in the central Red Sea, hot brines feel the deeps and minerals found in cores were magnetite, goethite, ferroxyhyte, manganite, todorokite, groutite and short range ordered ferrihydrite and singerite. Observation by electron microscopy enables us to see the size of euhedral or unhedral phases. Relations between the minerals are observed. Point analyses yield the chemical composition of the mineral with impurities, and Electron diffraction identifies the crystallography of the minerals

    Nano-Sized Minerals from Lower Cretaceous Sandstones in Israel Observed by Transmission Electron Microscopy (TEM)

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    Fine fraction in quartz arenite sandstones from Lower Cretaceous Hatira formation in Israel was observed by Transmission electron microscope (TEM). Samples were collected from Hatira and Ramon craters located in southern part of Israel and from Manara cliff from the northern part of Israel. The additional phases cause yellow, red, dark red and dark violet colors of the layered sandstones. The motivation was to identify the minerals of the fine factions that cause the variations in the colors. The minerals observed were clay minerals, mainly kaolinite (Al4Si4O20(OH)8), some illite (K0.65Al2.0[Al0.65Si3.35O10](OH)2) and smectite. Iron oxides were goethite (FeOOH) and hematite (Fe2O3), Titanium-iron oxides observed was ilmenite (FeTiO3), and Titanium-oxides were rutile (TiO2), and anatase (TiO2). Sulphates observed were jarosite (KFe3(SO4)2(OH)6) and alunite (KAl3(SO4)2(OH)6). Some of the hematite was formed by recrystallization of goethite. Ilmenite disintegrated into small iron oxides mainly hematite. Euhedral to sub-hedral rutile (TiO2) and anatase (TiO2) were preserved in clay-minerals. Crystals of alunite and jarosite were observed in sandstones in both craters. They probably crystallized due to some transgression of the Thetis Sea
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