3,192 research outputs found
A sensitive optical pyrometer for shock-temperature measurements
A new optical system was used to determine temperatures above 2400 K in shocked materials by measuring the spectral radiance of sub-microsecond pulses of light emitted from initially transparent solid samples in the visible and near infrared (450 to 900 nm). The high sensitivity of this optical pyrometer is attributed to the small number of channels, large aperture (0.03 steradian), the large bandwidth per channel (40 nm), and large photodiode detection area (0.2 sq cm). Improved calibration techniques reduce systematic errors encountered in previous shock-temperature experiments
Orbiting dynamic compression laboratory
In order to examine the feasibility of carrying out dynamic compression experiments on a space station, the possibility of using explosive gun launchers is studied. The question of whether powders of a refractory metal (molybdenum) and a metallic glass could be well considered by dynamic compression is examined. In both cases extremely good bonds are obtained between grains of metal and metallic glass at 180 and 80 kb, respectively. When the oxide surface is reduced and the dynamic consolidation is carried out in vacuum, in the case of molybdenum, tensile tests of the recovered samples demonstrated beneficial ultimate tensile strengths
Jena Soil Model (JSM v1.0; revision 1934): a microbial soil organic carbon model integrated with nitrogen and phosphorus processes
Plant–soil interactions, such as the coupling of plants' below-ground biomass allocation with soil organic matter (SOM) decomposition, nutrient release and plant uptake, are essential to understand the response of carbon (C) cycling to global changes. However, these processes are poorly represented in the current terrestrial biosphere models owing to the simple first-order approach of SOM cycling and the ignorance of variations within a soil profile. While the emerging microbially explicit soil organic C models can better describe C formation and turnover, at present, they lack a full coupling to the nitrogen (N) and phosphorus (P) cycles with the soil profile. Here we present a new SOM model – the Jena Soil Model (JSM) – which is microbially explicit, vertically resolved and integrated with the N and P cycles. To account for the effects of nutrient availability and litter quality on decomposition, JSM includes the representation of enzyme allocation to different depolymerisation sources based on the microbial adaptation approach as well as of nutrient acquisition competition based on the equilibrium chemistry approximation approach. Herein, we present the model structure and basic features of model performance in a beech forest in Germany. The model reproduced the main SOM stocks and microbial biomass as well as their vertical patterns in the soil profile. We further tested the sensitivity of the model to parameterisation and showed that JSM is generally sensitive to changes in microbial stoichiometry and processes
Shock temperatures in anorthite glass
Temperatures of CaAl2Si2O8 (anorthite glass) shocked to pressures between 48 and 117 GPa were measured in the range from 2500 to 5600 K, using optical pyrometry techniques. The pressure dependence of the shock temperatures deviates significantly from predictions based on a single high pressure phase. At least three phase transitions, at pressures of about 55, 85, and 100 GPa and with transition energies of about 0.5 MJ/kg each (approximately 1.5 MJ/kg total) are required to explain the shock temperature data. The phase transition at 100 GPa can possibly be identified with the stishovite melting transition. Theoretical models of the time dependence of the thermal radiation from the shocked anorthite based on the geometry of the experiment and the absorptive properties of the shocked material yields good agreement with observations, indicating that it is not necessary to invoke intrinsic time dependences to explain the data in many cases
A method of determining points on the principal isentropes of molecular liquids
We have examined the feasibility of using a large‐diameter, projectile‐target impact to carry out one‐dimensional, isentropic compression experiments on molecular fluids. By employing a three‐layered target geometry, with a thin foam driver layer and a thick, high‐impedance anvil layer, liquid H_2O can be compressed to a state within 0.1% of its principal isentrope at pressures up to about 30 GPa. The pressure and density of the state achieved can be determined from electromagnetic particle velocity gauges imbedded on the interfaces bounding the sample
Space station impact experiments
Four processes serve to illustrate potential areas of study and their implications for general problems in planetary science. First, accretional processes reflect the success of collisional aggregation over collisional destruction during the early history of the solar system. Second, both catastrophic and less severe effects of impacts on planetary bodies survivng from the time of the early solar system may be expressed by asteroid/planetary spin rates, spin orientations, asteroid size distributions, and perhaps the origin of the Moon. Third, the surfaces of planetary bodies directly record the effects of impacts in the form of craters; these records have wide-ranging implications. Fourth, regoliths evolution of asteroidal surfaces is a consequence of cumulative impacts, but the absence of a significant gravity term may profoundly affect the retention of shocked fractions and agglutinate build-up, thereby biasing the correct interpretations of spectral reflectance data. An impact facility on the Space Station would provide the controlled conditions necessary to explore such processes either through direct simulation of conditions or indirect simulation of certain parameters
Bayesian calibration of a soil organic carbon model using Δ<sup>14</sup>C measurements of soil organic carbon and heterotrophic respiration as joint constraints
Soils of temperate forests store significant amounts of organic matter and
are considered to be net sinks of atmospheric CO<sub>2</sub>. Soil organic carbon
(SOC) turnover has been studied using the Δ<sup>14</sup>C values of bulk SOC
or different SOC fractions as observational constraints in SOC models.
Further, the Δ<sup>14</sup>C values of CO<sub>2</sub> that evolved during the
incubation of soil and roots have been widely used together with
Δ<sup>14</sup>C of total soil respiration to partition soil respiration into
heterotrophic respiration (HR) and rhizosphere respiration. However, these
data have not been used as joint observational constraints to determine SOC
turnover times. Thus, we focus on (1) how different combinations of
observational constraints help to narrow estimates of turnover times and
other parameters of a simple two-pool model, the Introductory Carbon Balance
Model (ICBM); (2) whether relaxing the steady-state assumption in a multiple
constraints approach allows the source/sink strength of the soil to be
determined while estimating turnover times at the same time. To this end ICBM
was adapted to model SOC and SO<sup>14</sup>C in parallel with
litterfall and the Δ<sup>14</sup>C of litterfall as driving variables. The
Δ<sup>14</sup>C of the atmosphere with its prominent bomb peak was used as a
proxy for the Δ<sup>14</sup>C of litterfall. Data from three spruce-dominated
temperate forests in Germany and the USA (Coulissenhieb II, Solling D0 and
Howland Tower site) were used to estimate the parameters of ICBM via Bayesian
calibration. Key findings are as follows: (1) the joint use of all four
observational constraints (SOC stock and its Δ<sup>14</sup>C, HR flux and its
Δ<sup>14</sup>C) helped to considerably narrow turnover times of the young
pool (primarily by Δ<sup>14</sup>C of HR) and the old pool (primarily by
Δ<sup>14</sup>C of SOC). Furthermore, the joint use of all observational
constraints made it possible to constrain the humification factor in ICBM,
which describes the fraction of the annual outflux from the young pool that
enters the old pool. The Bayesian parameter estimation yielded the following
turnover times (mean ± standard deviation) for SOC in the young pool:
Coulissenhieb II 1.1 ± 0.5 years, Solling D0 5.7 ± 0.8 years and
Howland Tower 0.8 ± 0.4 years. Turnover times for the old pool were
377 ± 61 years (Coulissenhieb II), 313 ± 66 years (Solling D0)
and 184 ± 42 years (Howland Tower), respectively. (2) At all three
sites the multiple constraints approach was not able to determine if the soil
has been losing or storing carbon. Nevertheless, the relaxed steady-state
assumption hardly introduced any additional uncertainty for the other
parameter estimates. Overall the results suggest that using Δ<sup>14</sup>C
data from more than one carbon pool or flux helps to better constrain SOC
models
The proposed dropping of the genus crassostrea for all Pacific cupped oysters and its replacement by a new genus magallana: a dissenting view
The World Register of Marine Species (WoRMS) currently
registers all Pacific cupped oysters that were formerly members
of the genus Crassostrea in a new genus, Magallana. Magallana
gigas is designated as an ‘‘accepted name,’’ whereas a search for
Crassostrea gigas results in the message ‘‘no matching results
found.’’ This has caused dismay among many biologists,
aquaculturists, and other stakeholders with an interest in the
Pacific and other oysters. This note, which is authored by 27
interested scientists, presents a dissenting view and a rebuttal of
the proposed change of genus
The Gerasimov-Drell-Hearn Sum Rule and the Spin Structure of the Nucleon
The Gerasimov-Drell-Hearn sum rule is one of several dispersive sum rules
that connect the Compton scattering amplitudes to the inclusive photoproduction
cross sections of the target under investigation. Being based on such universal
principles as causality, unitarity, and gauge invariance, these sum rules
provide a unique testing ground to study the internal degrees of freedom that
hold the system together. The present article reviews these sum rules for the
spin-dependent cross sections of the nucleon by presenting an overview of
recent experiments and theoretical approaches. The generalization from real to
virtual photons provides a microscope of variable resolution: At small
virtuality of the photon, the data sample information about the long range
phenomena, which are described by effective degrees of freedom (Goldstone
bosons and collective resonances), whereas the primary degrees of freedom
(quarks and gluons) become visible at the larger virtualities. Through a rich
body of new data and several theoretical developments, a unified picture of
virtual Compton scattering emerges, which ranges from coherent to incoherent
processes, and from the generalized spin polarizabilities on the low-energy
side to higher twist effects in deep inelastic lepton scattering.Comment: 32 pages, 19 figures, review articl
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