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When Yeomans joined – she was poached from Vogue on her first day – Harpers was a hangover from the Sloane days of the Eighties, chronicling the lives, parties and trends of the upper classes.
The climatic trends of the upper Chinle Formation cumulated with the formation of the massive eolian dune fields of the Glen Canyon Group during Early-Middle Jurassic time (e.g., [117]).
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Figure 8 includes some additional values for maximum fuel and medium steam extraction, which is why a slightly non linear trend of the upper map restriction can be seen for the Ebsilon results.
Figure 2 shows the trend of the upper limits for both pensions and contributions since 1982,9 and the following points are relevant for the simulations carried out in this article: (1) the maximum contribution base has historically increased with inflation at the same time that the different professional categories were grouped together, remaining steady in real terms from the year 2002 onwards.
When we analyzed the data according to tertiles of MR-proANP and MR-proADM (Table 3), a non-significant trend for the upper tertile of MR-proANP for all-cause (HR = 1.76, p = 0.082) and cardiovascular mortality (HR = 2.96, p = 0.053) was observed.
The scenario of trends in the upper atmosphere and ionosphere became more complete and some discrepancies were removed or explained.
The lower Dudley shows similar lithology and thickness trends to that of the upper unit, with the proportion of sand increasing while thinning overall.
The TG-2 of CAWSES-II covered several important problems in the investigation of long-term trends in the upper atmosphere and ionosphere, but not the full spectrum of problems.
Temporal and spatial changes of long-term trends in the upper atmosphere and ionosphere are inevitable (e.g., Laštovička et al. [2012]) because trends of some of these drivers change principally with time (e.g., ozone or geomagnetic activity) or location (e.g., Earth's magnetic field).
Therefore, to obtain an independent picture of long-term trends in the upper ionosphere, the 11-year (132 months) running mean values of the monthly absolute deviations (∆foF2 132 ) were calculated over the entire dataset according to the method set out by Mikhailov (2006).
The TG-2 progress that is reviewed in this paper together with some results reached outside CAWSES-II so as to have the full context of progress in trends in the upper atmosphere and ionosphere.
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