67,769 research outputs found
The impact of water on free-falling bodies
Report discussed measures to cushion impact on body falling into water. Heavy loads are generated by impact and by pressures of water cavity collapsing onto the body
Structural, vibrational and thermal properties of densified silicates : insights from Molecular Dynamics
Structural, vibrational and thermal properties of densified sodium silicate
(NS2) are investigated with classical molecular dynamics simulations of the
glass and the liquid state. A systematic investigation of the glass structure
with respect to density was performed. We observe a repolymerization of the
network manifested by a transition from a tetrahedral to an octahedral silicon
environment, the decrease of the amount of non-bridging oxygen atoms and the
appearance of three-fold coordinated oxygen atoms (triclusters). Anomalous
changes in the medium range order are observed, the first sharp diffraction
peak showing a minimum of its full-width at half maximum according to density.
The previously reported vibrational trends in densified glasses are observed,
such as the shift of the Boson peak intensity to higher frequencies and the
decrease of its intensity. Finally, we show that the thermal behavior of the
liquid can be reproduced by the Birch-Murnaghan equation of states, thus
allowing us to compute the isothermal compressibility
Center-commissioned external review of International Water Management Institute: Consolidated report, 19-29 May 2003
Agricultural research / Research institutes / Research policy / Research priorities / Planning / Monitoring / Evaluation / Financial resources / Gender
Simulating Radiative Magnetohydrodynamical Flows with AstroBEAR: Implementation and Applications of Non-equilibrium Cooling
Radiative cooling plays a crucial role in the dynamics of many astrophysical
flows, and is particularly important in the dense shocked gas within
Herbig-Haro (HH) objects and stellar jets. Simulating cooling processes
accurately is necessary to compare numerical simulations with existing and
planned observations of HH objects, such as those from the Hubble Space
Telescope and the James Webb Space Telescope. In this paper we discuss a new,
non-equilibrium cooling scheme we have implemented into the 3-D
magnetohydrodynamic (MHD) code AstroBEAR. The new cooling function includes
ionization, recombination, and excitation of all the important atomic species
that cool below 10000 K. We tested the routine by comparing its predictions
with those from the well-tested 1-D Cox-Raymond shock code (Raymond 1979). The
results show thatAstroBEAR accurately tracks the ionization fraction,
temperature, and other MHD variables for all low-velocity (.90 km/s) magnetized
radiative shock waves. The new routine allows us to predict synthetic emission
maps in all the bright forbidden and permitted lines observed in stellar jets,
including H{\alpha}, [NII], [OI], and [SII]. We present an example as to how
these synthetic maps facilitate a direct comparison with narrowband images of
HH objects.Comment: 8 figure
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Noble gases from the planetary nebula stage of stellar evolution implanted in meteoritic SiC grains
The status of traditional Scottish animal breeds and plant varieties and the implications for biodiversity
The aim of this scoping study was to evaluate the effects on Scottish biodiversity of
changes in the use of traditional breeds and varieties. The overall objectives were:
a) The evaluation of the importance of genetic loss from the reduction in use of these
breeds and varieties, for example, the loss of unusual characteristics that might have
been of particular local use.
b) An assessment of the impacts of reduction in the ability to conduct further breeding or
research on rare and traditional varieties and breeds.
c) Identification of the loss of certain farming techniques associated with particular
varieties and breeds.
d) An assessment of possible losses of biodiversity associated with reduction in the use of
these breeds and varieties and the farming systems associated with them
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Organic components in interplanetary dust particles and their implications for the synthesis of cometary organics
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