156 research outputs found
The impact of atmospheric pCO2 on carbon isotope ratios of the atmosphere and ocean
It is well known that the equilibration timescale for the isotopic ratios 13C/12C and 14C/12C in the ocean mixed layer is on the order of a decade, 2 orders of magnitude slower than for oxygen. Less widely appreciated is the fact that the equilibration timescale is quite sensitive to the speciation of dissolved inorganic carbon (DIC) in the mixed layer, scaling linearly with the ratio DIC/CO2, which varies inversely with atmospheric pCO2. Although this effect is included in models that resolve the role of carbon speciation in air-sea exchange, its role is often unrecognized, and it is not commonly considered in the interpretation of carbon isotope observations. Here we use a global three-dimensional ocean model to estimate the redistribution of the carbon isotopic ratios between the atmosphere and ocean due solely to variations in atmospheric pCO2. Under Last Glacial Maximum (LGM) pCO2, atmospheric Î14C is increased by ~30â° due to the speciation change, all else being equal, raising the surface reservoir age by about 250 years throughout most of the ocean. For 13C, enhanced surface disequilibrium under LGM pCO2 causes the upper ocean, atmosphere, and North Atlantic Deep Water ÎŽ13C to become at least 0.2â° higher relative to deep waters ventilated by the Southern Ocean. Conversely, under high pCO2, rapid equilibration greatly decreases isotopic disequilibrium. As a result, during geological periods of high pCO2, vertical ÎŽ13C gradients may have been greatly weakened as a direct chemical consequence of the high pCO2, masquerading as very well ventilated or biologically dead Strangelove Oceans. The ongoing anthropogenic rise of pCO2 is accelerating the equilibration of the carbon isotopes in the ocean, lowering atmospheric Î14C and weakening ÎŽ13C gradients within the ocean to a degree that is similar to the traditional fossil fuel âSuessâ effect
Asymptotic Dynamics of Breathers in Fermi-Pasta-Ulam Chains
We study the asymptotic dynamics of breathers in finite Fermi-Pasta-Ulam
chains at zero and non-zero temperatures. While such breathers are essentially
stationary and very long-lived at zero temperature, thermal fluctuations tend
to lead to breather motion and more rapid decay
Energy Relaxation in Nonlinear One-Dimensional Lattices
We study energy relaxation in thermalized one-dimensional nonlinear arrays of
the Fermi-Pasta-Ulam type. The ends of the thermalized systems are placed in
contact with a zero-temperature reservoir via damping forces. Harmonic arrays
relax by sequential phonon decay into the cold reservoir, the lower frequency
modes relaxing first. The relaxation pathway for purely anharmonic arrays
involves the degradation of higher-energy nonlinear modes into lower energy
ones. The lowest energy modes are absorbed by the cold reservoir, but a small
amount of energy is persistently left behind in the array in the form of almost
stationary low-frequency localized modes. Arrays with interactions that contain
both a harmonic and an anharmonic contribution exhibit behavior that involves
the interplay of phonon modes and breather modes. At long times relaxation is
extremely slow due to the spontaneous appearance and persistence of energetic
high-frequency stationary breathers. Breather behavior is further ascertained
by explicitly injecting a localized excitation into the thermalized array and
observing the relaxation behavior
Evidence for a mixed mass composition at the `ankle' in the cosmic-ray spectrum
We report a first measurement for ultra-high energy cosmic rays of the
correlation between the depth of shower maximum and the signal in the water
Cherenkov stations of air-showers registered simultaneously by the fluorescence
and the surface detectors of the Pierre Auger Observatory. Such a correlation
measurement is a unique feature of a hybrid air-shower observatory with
sensitivity to both the electromagnetic and muonic components. It allows an
accurate determination of the spread of primary masses in the cosmic-ray flux.
Up till now, constraints on the spread of primary masses have been dominated by
systematic uncertainties. The present correlation measurement is not affected
by systematics in the measurement of the depth of shower maximum or the signal
in the water Cherenkov stations. The analysis relies on general characteristics
of air showers and is thus robust also with respect to uncertainties in
hadronic event generators. The observed correlation in the energy range around
the `ankle' at differs significantly from
expectations for pure primary cosmic-ray compositions. A light composition made
up of proton and helium only is equally inconsistent with observations. The
data are explained well by a mixed composition including nuclei with mass . Scenarios such as the proton dip model, with almost pure compositions, are
thus disfavoured as the sole explanation of the ultrahigh-energy cosmic-ray
flux at Earth.Comment: Published version. Added journal reference and DOI. Added Report
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Effectiveness of an mHealth intervention combining a smartphone app and smart band on body composition in an overweight and obese population: Randomized controlled trial (EVIDENT 3 study)
Background: Mobile health (mHealth) is currently among the supporting elements that may contribute to an improvement in health markers by helping people adopt healthier lifestyles. mHealth interventions have been widely reported to achieve greater weight loss than other approaches, but their effect on body composition remains unclear.
Objective: This study aimed to assess the short-term (3 months) effectiveness of a mobile app and a smart band for losing weight and changing body composition in sedentary Spanish adults who are overweight or obese.
Methods: A randomized controlled, multicenter clinical trial was conducted involving the participation of 440 subjects from primary care centers, with 231 subjects in the intervention group (IG; counselling with smartphone app and smart band) and 209 in the control group (CG; counselling only). Both groups were counselled about healthy diet and physical activity. For the 3-month intervention period, the IG was trained to use a smartphone app that involved self-monitoring and tailored feedback, as well as a smart band that recorded daily physical activity (Mi Band 2, Xiaomi). Body composition was measured using the InBody 230 bioimpedance device (InBody Co., Ltd), and physical activity was measured using the International Physical Activity Questionnaire.
Results: The mHealth intervention produced a greater loss of body weight (â1.97 kg, 95% CI â2.39 to â1.54) relative to standard counselling at 3 months (â1.13 kg, 95% CI â1.56 to â0.69). Comparing groups, the IG achieved a weight loss of 0.84 kg more than the CG at 3 months. The IG showed a decrease in body fat mass (BFM; â1.84 kg, 95% CI â2.48 to â1.20), percentage of body fat (PBF; â1.22%, 95% CI â1.82% to 0.62%), and BMI (â0.77 kg/m2, 95% CI â0.96 to 0.57). No significant changes were observed in any of these parameters in men; among women, there was a significant decrease in BMI in the IG compared with the CG. When subjects were grouped according to baseline BMI, the overweight group experienced a change in BFM of â1.18 kg (95% CI â2.30 to â0.06) and BMI of â0.47 kg/m2 (95% CI â0.80 to â0.13), whereas the obese group only experienced a change in BMI of â0.53 kg/m2 (95% CI â0.86 to â0.19). When the data were analyzed according to physical activity, the moderate-vigorous physical activity group showed significant changes in BFM of â1.03 kg (95% CI â1.74 to â0.33), PBF of â0.76% (95% CI â1.32% to â0.20%), and BMI of â0.5 kg/m2 (95% CI â0.83 to â0.19).
Conclusions: The results from this multicenter, randomized controlled clinical trial study show that compared with standard counselling alone, adding a self-reported app and a smart band obtained beneficial results in terms of weight loss and a reduction in BFM and PBF in female subjects with a BMI less than 30 kg/m2 and a moderate-vigorous physical activity level. Nevertheless, further studies are needed to ensure that this profile benefits more than others from this intervention and to investigate modifications of this intervention to achieve a global effect
Densidade da madeira de ĂĄrvores em savanas do norte da AmazĂŽnia brasileira
Densidade da madeira (DM) Ă© uma variĂĄvel importante para estimativas de estoques de carbono arbĂłreo em ecossistemas terrestres. Este tema Ă© pobremente investigado em ĂĄreas de savana da AmazĂŽnia brasileira. O objetivo deste estudo foi investigar a DM das oito principais espĂ©cies arbĂłreas que ocorrem na savana aberta de Roraima, a maior ĂĄrea de savana do norte do bioma AmazĂŽnia. Foram verificadas as variaçÔes na DM em função da espĂ©cie e dos diferentes diĂąmetros observados ao longo da dimensĂŁo vertical de 75 indivĂduos amostrados em seis sĂtios de coleta. Foi utilizado o mĂ©todo direto para obtenção de peças de madeira do fuste e da copa. Os resultados indicaram discrepĂąncia significativa interespecĂfica, sendo Roupala montana Aubl. a espĂ©cie de maior DM mĂ©dia (0,674 g cm-3). Foi detectado que existe variação significativa da DM entre as peças do fuste e da copa, independente da espĂ©cie e do sĂtio de coleta. A densidade da madeira de peças da copa com diĂąmetro entre 5 e 10 cm pode ser utilizada como preditora da DM mĂ©dia do indivĂduo arbĂłreo. NĂłs concluimos que a DM das oito espĂ©cies arbĂłreas investigadas possui variabilidade interespecĂfica, com discrepĂąncias entre a DM do fuste e das partes lenhosas da copa. As distinçÔes aqui detectadas devem ser considerados como uma importante ferramenta para melhorar as estimativas de estoque de carbono em ĂĄreas de savanas na AmazĂŽnia
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