The ERA-Interim reanalysis: configuration and performance of the data assimilation system

ERA-Interim is the latest global atmospheric reanalysis produced by the European Centre for Medium-Range Weather Forecasts (ECMWF). The ERA-Interim project was conducted in part to prepare for a new atmospheric reanalysis to replace ERA-40, which will extend back to the early part of the twentieth century. This article describes the forecast model, data assimilation method, and input datasets used to produce ERA-Interim, and discusses the performance of the system. Special emphasis is placed on various difficulties encountered in the production of ERA-40, including the representation of the hydrological cycle, the quality of the stratospheric circulation, and the consistency in time of the reanalysed fields. We provide evidence for substantial improvements in each of these aspects. We also identify areas where further work is needed and describe opportunities and objectives for future reanalysis projects at ECMWF

Atmospheric conservation properties in ERA-Interim

We study the global atmospheric budgets of mass, moisture, energy and angular momentum in the latest reanalysis from the European Centre for Medium-Range Weather Forecasts (ECMWF), ERA-Interim, for the period 1989–2008 and compare with ERA-40. Most of the measures we use indicate that the ERA-Interim reanalysis is superior in quality to ERA-40. In ERA-Interim the standard deviation of the monthly mean global dry mass of 0.7 kg m−2 (0.007%) is slightly worse than in ERA-40, and long time-scale variations in dry mass originate predominately in the surface pressure field. The divergent winds are improved in ERA-Interim: the global standard deviation of the time-averaged dry mass budget residual is 10 kg m−2 day−1 and the quality of the cross-equatorial mass fluxes is improved. The temporal variations in the global evaporation minus precipitation (E − P) are too large but the global moisture budget residual is 0.003 kg m−2 day−1 with a spatial standard deviation of 0.3 kg m−2 day−1. Both the E − P over ocean and P − E over land are about 15% larger than the 1.1 Tg s−1 transport of water from ocean to land. The top of atmosphere (TOA) net energy losses are improved, with a value of 1 W m−2, but the meridional gradient of the TOA net energy flux is smaller than that from the Clouds and the Earth's Radiant Energy System (CERES) data. At the surface the global energy losses are worse, with a value of 7 W m−2. Over land however, the energy loss is only 0.5 W m−2. The downwelling thermal radiation at the surface in ERA-Interim of 341 W m−2 is towards the higher end of previous estimates. The global mass-adjusted energy budget residual is 8 W m−2 with a spatial standard deviation of 11 W m−2, and the mass-adjusted atmospheric energy transport from low to high latitudes (the sum for the two hemispheres) is 9.5 PW

The response of ionospheric convection in the polar cap to substorm activity

We report multi-instrument observations during an isolated substorm on 17 October 1989. The EISCAT radar operated in the SP-UK-POLI mode measuring ionospheric convection at latitudes 71°-78°. SAMNET and the EISCAT Magnetometer Cross provide information on the timing of substorm expansion phase onset and subsequent intensifications, as well as the location of the field aligned and ionospheric currents associated with the substorm current wedge. IMP-8 magnetic field data are also included. Evidence of a substorm growth phase is provided by the equatorward motion of a flow reversal boundary across the EISCAT radar field of view at 2130 MLT, following a southward turning of the interplanetary magnetic field (IMF). We infer that the polar cap expanded as a result of the addition of open magnetic flux to the tail lobes during this interval. The flow reversal boundary, which is a lower limit to the polar cap boundary, reached an invariant latitude equatorward of 71° by the time of the expansion phase onset. A westward electrojet, centred at 65.4°, occurred at the onset of the expansion phase. This electrojet subsequently moved poleward to a maximum of 68.1° at 2000 UT and also widened. During the expansion phase, there is evidence of bursts of plasma flow which are spatially localised at longitudes within the substorm current wedge and which occurred well poleward of the westward electrojet. We conclude that the substorm onset region in the ionosphere, defined by the westward electrojet, mapped to a part of the tail radially earthward of the boundary between open and closed magnetic flux, the “distant” neutral line. Thus the substorm was not initiated at the distant neutral line, although there is evidence that it remained active during the expansion phase. It is not obvious whether the electrojet mapped to a near-Earth neutral line, but at its most poleward, the expanded electrojet does not reach the estimated latitude of the polar cap boundary.

Effect of sonication on the particle size of montmorillonite clays

This paper reports on the effect of sonication on SAz-1 and SWy-1 montmorillonite suspensions. Changes in the size of the particles of these materials and modifications of their properties have been investigated. The variation of the particle size has been analyzed by DLS (dynamic light scattering). In all cases the clay particles show a bimodal distribution. Sonication resulted in a decrease of the larger modal diameter, as well as a reduction of its volume percentage. Simultaneously, the proportion of the smallest particles increases. After 60 min of sonication, SAz-1 presented a very broad particle size distribution with a modal diameter of 283 nm. On the other hand, the SWy-1 sonicated for 60 min presents a bimodal distribution of particles at 140 and 454 nm. Changes in the properties of the clay suspensions due to sonication were evaluated spectroscopically from dye-clay interactions, using Methylene Blue. The acidic sites present in the interlamellar region, which are responsible for dye protonation, disappeared after sonication of the clay. The changes in the size of the scattering particles and the lack of acidic sites after sonication suggest that sonication induces delamination of the clay particles. (c) 2008 Elsevier Inc. All rights reserved.

Estudo cinético da reação de formação de reticulados tridimensionais

Poli(butadieno) foi reticulado, em solução, com 4,4'-(4,4'-difenilmetileno)-bis-1 ,2,4-triazolina- 3, 5 - diona (BPMTD). Para monitoramento da reação foi medida a absorbância de uma transição n -> pi * do sistema 1,2,4-triazolina-3,5-diona. Segundo os estudos realizados, para baixas conversões a reação segue um esquema cinético de pseudo-primeira ordem e o processo não é controlado pela difusão, pois independe da viscosidade inicial do sistema. Para altas conversões, o processo torna-se dependente do peso molecular e da concentração do polímero inicial, devido à ocorrência de uma difusão impedida a nível de segmentos de cadeia. Estudos preliminares da reação de reticulação da borracha butílica com a BPMTD mostraram que, como o número de ligações duplas por cadeia polimérica é menor neste caso, ocorre formação de um menor número de ligações intramoleculares e a quantidade de BPMTD necessária para que ocorra gelificação é muito menor do que no caso do poli(butadieno).

Estudo da transição de fase sol-gel em reticulados de polibutadieno

A transição de fase sol-gel em reticulados de poli-(butadieno) sintetizados com 1,6-hexano-bis-1,2,4-triazolina-3,5-diona (HMTD) foi caracterizada através de um estudo cinético e de um estudo viscosimétrico. Verificou-se que a reação de reticulação segue um esquema cinético de pseudo-primeira ordem, o qual a baixas conversões é equivalente a um de primeira ordem, sendo a reação neste estágio controlada por processo de ativação. A conversões mais altas ocorre um desvio do comportamento inicial, tornando-se a reção acentuadamente mais lenta. Através de medidas de viscosidade intrínseca de sistemas ramificados (estado de sol), determinou-se o ponto de gelificação em função da concentração inicial HMTD. Verificou-se ser necessário observar-se um aumento acentuado da viscosidade intrínseca com a concentração de HMTD, para que o ponto de gelificação obtido seja coerente aos dados experimentais. Relacionando-se a cinética da reação à viscosimetria, calculou-se o tempo de gelificação, i.e. o ponto de gelificação em função do tempo. Através da constante de velocidade da reação, do ponto de gelificação em função da concentração de HMTD, da conversão crítica e do tempo de gelificação, caracterizou-se a transição de fase sol-gel do sistema estudado.