15,414 research outputs found
Weather-based estimation of wildfire risk
Catastrophic wildfires in California have become more frequent in past decades, while insured losses per event have been rising substantially. On average, California ranks the highest among states in the U.S. in the number of fires as well as the number of acres burned each year. The study of catastrophic wildfire models plays an important role in the prevention and mitigation of such disasters. Accurate forecasts of potential large fires assist fire managers in preparing resources and strategic planning for fire suppression. Furthermore, fire forecasting can a priori inform insurers on potential financial losses due to large fires. This paper describes a probabilistic model for predicting wildland fire risks using the two-stage Heckman procedure. Using 37 years of spatial and temporal information on weather and fire records in Southern California, this model measures the probability of a fire occurring and estimates the expected size of the fire on a given day and location, offering a technique to predict and forecast wildfire occurrences based on weather information that is readily available at low cost.biased sampling, forest fires, fire occurrence probabilities, fire weather
Resolving 3D Disk Orientation using High-Resolution Images: New Constraints on Circumgalactic Gas Inflows
We constrain gas inflow speeds in star-forming galaxies with color gradients
consistent with inside-out disk growth. Our method combines new measurements of
disk orientation with previously described circumgalactic absorption in
background quasar spectra. Two quantities, a position angle and an axis ratio,
describe the projected shape of each galactic disk on the sky, leaving an
ambiguity about which side of the minor axis is tipped toward the observer.
This degeneracy regarding the 3D orientation of disks has compromised previous
efforts to measure gas inflow speeds. We present HST and Keck/LGSAO imaging
that resolves the spiral structure in five galaxies at redshift .
We determine the sign of the disk inclination for four galaxies, under the
assumption that spiral arms trail the rotation. We project models for both
radial infall in the disk plane and circular orbits onto each quasar sightline.
We compare the resulting line-of-sight velocities to the observed velocity
range of Mg II absorption in spectra of background quasars, which intersect the
disk plane at radii between 69 and 115 kpc. For two sightlines, we constrain
the maximum radial inflow speeds as 30-40 km s. We also rule out a
velocity component from radial inflow in one sightline, suggesting that the
structures feeding gas to these growing disks do not have unity covering
factor. We recommend appropriate selection criteria for building larger samples
of galaxy--quasar pairs that produce orientations sensitive to constraining
inflow properties.Comment: 15 pages with 8 figures and 2 tables; accepted for publication in Ap
Object-oriented construction of a multigrid electronic-structure code with Fortran 90
We describe the object-oriented implementation of a higher-order
finite-difference density-functional code in Fortran 90. Object-oriented models
of grid and related objects are constructed and employed for the implementation
of an efficient one-way multigrid method we have recently proposed for the
density-functional electronic-structure calculations. Detailed analysis of
performance and strategy of the one-way multigrid scheme will be presented.Comment: 24 pages, 6 figures, to appear in Comput. Phys. Com
Static Properties of a Simulated Supercooled Polymer Melt: Structure Factors, Monomer Distributions Relative to the Center of Mass, and Triple Correlation Functions
We analyze structural and conformational properties in a simulated
bead-spring model of a non-entangled, supercooled polymer melt. We explore the
statics of the model via various structure factors, involving not only the
monomers, but also the center of mass (CM). We find that the conformation of
the chains and the CM-CM structure factor, which is well described by a
recently proposed approximation [Krakoviack et al., Europhys. Lett. 58, 53
(2002)], remain essentially unchanged on cooling toward the critical glass
transition temperature of mode-coupling theory. Spatial correlations between
monomers on different chains, however, depend on temperature, albeit smoothly.
This implies that the glassy behavior of our model cannot result from static
intra-chain or CM-CM correlations. It must be related to inter-chain
correlations at the monomer level. Additionally, we study the dependence of
inter-chain correlation functions on the position of the monomer along the
chain backbone. We find that this site-dependence can be well accounted for by
a theory based on the polymer reference interaction site model (PRISM). We also
analyze triple correlations by means of the three-monomer structure factors for
the melt and for the chains. These structure factors are compared with the
convolution approximation that factorizes them into a product of two-monomer
structure factors. For the chains this factorization works very well,
indicating that chain connectivity does not introduce special triple
correlations in our model. For the melt deviations are more pronounced,
particularly at wave vectors close to the maximum of the static structure
factor.Comment: REVTeX4, 16 pages, 16 figures, accepted for publication in Physical
Review
Butterfly Factorization
The paper introduces the butterfly factorization as a data-sparse
approximation for the matrices that satisfy a complementary low-rank property.
The factorization can be constructed efficiently if either fast algorithms for
applying the matrix and its adjoint are available or the entries of the matrix
can be sampled individually. For an matrix, the resulting
factorization is a product of sparse matrices, each with
non-zero entries. Hence, it can be applied rapidly in operations.
Numerical results are provided to demonstrate the effectiveness of the
butterfly factorization and its construction algorithms
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