1,393 research outputs found
Spatially Dependent Parameter Estimation and Nonlinear Data Assimilation by Autosynchronization of a System of Partial Differential Equations
Given multiple images that describe chaotic reaction-diffusion dynamics,
parameters of a PDE model are estimated using autosynchronization, where
parameters are controlled by synchronization of the model to the observed data.
A two-component system of predator-prey reaction-diffusion PDEs is used with
spatially dependent parameters to benchmark the methods described. Applications
to modelling the ecological habitat of marine plankton blooms by nonlinear data
assimilation through remote sensing is discussed
A Portrait of Cold Gas in Galaxies at 60pc Resolution and a Simple Method to Test Hypotheses That Link Small-Scale ISM Structure to Galaxy-Scale Processes
The cloud-scale density, velocity dispersion, and gravitational boundedness
of the interstellar medium (ISM) vary within and among galaxies. In turbulent
models, these properties play key roles in the ability of gas to form stars.
New high fidelity, high resolution surveys offer the prospect to measure these
quantities across galaxies. We present a simple approach to make such
measurements and to test hypotheses that link small-scale gas structure to star
formation and galactic environment. Our calculations capture the key physics of
the Larson scaling relations, and we show good correspondence between our
approach and a traditional "cloud properties" treatment. However, we argue that
our method is preferable in many cases because of its simple, reproducible
characterization of all emission. Using, low-J 12CO data from recent surveys,
we characterize the molecular ISM at 60pc resolution in the Antennae, the Large
Magellanic Cloud, M31, M33, M51, and M74. We report the distributions of
surface density, velocity dispersion, and gravitational boundedness at 60pc
scales and show galaxy-to-galaxy and intra-galaxy variations in each. The
distribution of flux as a function of surface density appears roughly lognormal
with a 1sigma width of ~0.3 dex, though the center of this distribution varies
from galaxy to galaxy. The 60pc resolution line width and molecular gas surface
density correlate well, which is a fundamental behavior expected for virialized
or free-falling gas. Varying the measurement scale for the LMC and M31, we show
that the molecular ISM has higher surface densities, lower line widths, and
more self-gravity at smaller scales.Comment: Accepted for publication in the Astrophysical Journal, 36 pages
(24+appendix), 21 figures (12+appendix), until publication high resolution
version at http://www.astronomy.ohio-state.edu/~leroy.42/cloudscale.pd
The Initial Economic Burden of Femur Fractures on Informal Caregivers in Dar es Salaam, Tanzania
BackgroundFemur fracture patients require significant in-hospital care. The burden incurred by caregivers of such patients amplifies the direct costs of these injuries and remains unquantified. Aim Here we aim to establish the in-hospital economic burden faced by informal caregivers of femur fracture patients. Methods
70 unique caregivers for 46 femoral shaft fracture patients were interviewed. Incurred economic burden was determined by the Human Capital Approach, using standardized income data to quantify productivity loss (in 149, 9% of a caregiver’s annual income and positively correlated with patient time in hospital (p<0.01). Conclusion Caregivers of patients treated operatively for femur fractures lost a large portion of their annual income, and this loss increased with patient time in hospital. These indirect costs of femur fracture treatment constitute an important component of the total injury burden
On the speed of convergence to stationarity of the Erlang loss system
We consider the Erlang loss system, characterized by servers, Poisson arrivals and exponential service times, and allow the arrival rate to be a function of We discuss representations and bounds for the rate of convergence to stationarity of the number of customers in the system, and display some bounds for the total variation distance between the time-dependent and stationary distributions. We also pay attention to time-dependent rates
SGLT2 inhibition versus sulfonylurea treatment effects on electrolyte and acid-base balance:secondary analysis of a clinical trial reaching glycemic equipoise: Tubular effects of SGLT2 inhibition in Type 2 diabetes
Sodium-glucose transporter (SGLT)2 inhibitors increase plasma magnesium and plasma phosphate and may cause ketoacidosis, but the contribution of improved glycemic control to these observations as well as effects on other electrolytes and acid-base parameters remain unknown. Therefore, our objective was to compare the effects of SGLT2 inhibitors dapagliflozin and sulfonylurea gliclazide on plasma electrolytes, urinary electrolyte excretion, and acid-base balance in people with Type 2 diabetes (T2D). We assessed the effects of dapagliflozin and gliclazide treatment on plasma electrolytes and bicarbonate, 24-hour urinary pH and excretions of electrolytes, ammonium, citrate, and sulfate in 44 metformin-treated people with T2D and preserved kidney function. Compared with gliclazide, dapagliflozin increased plasma chloride by 1.4 mmol/l (95% CI 0.4-2.4), plasma magnesium by 0.03 mmol/l (95% CI 0.01-0.06), and plasma sulfate by 0.02 mmol/l (95% CI 0.01-0.04). Compared with baseline, dapagliflozin also significantly increased plasma phosphate, but the same trend was observed with gliclazide. From baseline to week 12, dapagliflozin increased the urinary excretion of citrate by 0.93 ± 1.72 mmol/day, acetoacetate by 48 μmol/day (IQR 17-138), and β-hydroxybutyrate by 59 μmol/day (IQR 0-336), without disturbing acid-base balance. In conclusion, dapagliflozin increases plasma magnesium, chloride, and sulfate compared with gliclazide, while reaching similar glucose-lowering in people with T2D. Dapagliflozin also increases urinary ketone excretion without changing acid-base balance. Therefore, the increase in urinary citrate excretion by dapagliflozin may reflect an effect on cellular metabolism including the tricarboxylic acid cycle. This potentially contributes to kidney protection
Low CO Luminosities in Dwarf Galaxies
[Abridged] We present maps of CO 2-1 emission covering the entire
star-forming disks of 16 nearby dwarf galaxies observed by the IRAM HERACLES
survey. The data have 13 arcsec angular resolution, ~250 pc at our average
distance of 4 Mpc, and sample the galaxies by 10-1000 resolution elements. We
apply stacking techniques to perform the first sensitive search for CO emission
in dwarfs outside the Local Group ranging from single lines-of-sight, stacked
over IR-bright regions of embedded star formation, and stacked over the entire
galaxy. We detect 5 dwarfs in CO with total luminosities of L_CO = 3-28 1e6
Kkmspc2. The other 11 dwarfs remain undetected in CO even in the stacked data
and have L_CO < 0.4-8 1e6 Kkmspc2. We combine our sample of dwarfs with a large
literature sample of spirals to study scaling relations of L_CO with M_B and
metallicity. We find that dwarfs with metallicities of Z ~ 1/2-1/10 Z_sun have
L_CO about 1e2-1e4x smaller than spirals and that their L_CO per unit L_B is
10-100x smaller. A comparison with tracers of star formation (FUV and 24
micron) shows that L_CO per unit SFR is 10-100x smaller in dwarfs. One possible
interpretation is that dwarfs form stars much more efficiently, however we
argue that the low L_CO/SFR ratio is due to significant changes of the CO-to-H2
conversion factor, alpha_CO, in low metallicity environments. Assuming a
constant H2 depletion time of 1.8 Gyr (as found for nearby spirals) implies
alpha_CO values for dwarfs with Z ~ 1/2-1/10 Z_sun that are more than 10x
higher than those found in solar metallicity spirals. This significant increase
of alpha_CO at low metallicity is consistent with previous studies, in
particular those which model dust emission to constrain H2 masses. Even though
it is difficult to parameterize the metallicity dependence of alpha_CO, our
results suggest that CO is increasingly difficult to detect at lower
metallicities.Comment: Accepted for publication in the Astronomical Journal, 19 pages, 7
figure
Integer Quantum Hall Effect in Double-Layer Systems
We consider the localization of independent electron orbitals in double-layer
two-dimensional electron systems in the strong magnetic field limit. Our study
is based on numerical Thouless number calculations for realistic microscopic
models and on transfer matrix calculations for phenomenological network models.
The microscopic calculations indicate a crossover regime for weak interlayer
tunneling in which the correlation length exponent appears to increase.
Comparison of network model calculations with microscopic calculations casts
doubt on their generic applicability.Comment: 14 pages, 12 figures included, RevTeX 3.0 and epsf. Additional
reference
Predicted distribution of the Sunda Stink-badger Mydaus javanensis (Mammalia: Carnivora: Mephitidae) on Borneo
The Sunda stink-badger Mydaus javanensis is a small carnivore inhabiting the South-east Asian islands
of Java, Sumatra, Borneo and Natuna Islands. It occurs in a wide variety of vegetation types and is presently listed
by The IUCN Red List of Threatened Species as Least Concern. We analysed 15 (Balanced Model) or 77 (Spatial
Filtering Model) location records to predict habitat suitability across Borneo. The analysis suggests that most of the suitable habitat is located in Sabah, northeast Sarawak and North Kalimantan. In addition, this species is also recorded, mostly historically, patchily in west Sarawak, and West, Central, South and East Kalimantan. Although this species appears to be disturbance-tolerant and is frequently observed in village areas, some conservation action – such as limiting large-scale forest conversion to oil palm plantations – is warranted because most lowland habitat is unprotected. Further research in central and southern Borneo needs to focus on showing if there are any further sizable populations. Also, hunting of Sunda stink-badger has been reported in some parts of Borneo and might be a possible driver for the species’s patchy distribution. More research is warranted to understand what determines
the species’s distribution and density, based on which proper conservation strategies, if needed, can be developed
to preserve the species
Trust in governance networks: Its impacts on outcomes
__Abstract__
Governance networks are characterized by complex interaction and decision making, and much uncertainty. Surprisingly, there is very little research on the impact of trust in achieving results in governance networks. This article asks two questions: (a) Does trust influence the outcomes of environmental projects? and (b) Does active network management improve the level of trust in networks? The study is based on a Web-based survey of respondents involved in environmental projects. The results indicate that trust does matter for perceived outcomes and that network management strategies enhance the level of trust
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