145 research outputs found
Meteoric phenomena in the earth's atmosphere. Investigations of meteors, no. 2
Meteoritic radiance and ionization observations in earth atmospher
On inconsistency of experimental data on primary nuclei spectra with sea level muon intensity measurements
For the first time a complete set of the most recent direct data on primary
cosmic ray spectra is used as input into calculations of muon flux at sea level
in wide energy range GeV. Computations have been performed
with the CORSIKA/QGSJET and CORSIKA/VENUS codes. The comparison of the obtained
muon intensity with the data of muon experiments shows, that measurements of
primary nuclei spectra conform to sea level muon data only up to several tens
of GeV and result in essential deficit of muons at higher energies. As it
follows from our examination, uncertainties in muon flux measurements and in
the description of nuclear cascades development are not suitable to explain
this contradiction, and the only remaining factor, leading to this situation,
is underestimation of primary light nuclei fluxes. We have considered
systematic effects, that may distort the results of the primary cosmic ray
measurements with the application of the emulsion chambers. We suggest, that
re-examination of these measurements is required with the employment of
different hadronic interaction models. Also, in our point of view, it is
necessary to perform estimates of possible influence of the fact, that sizable
fraction of events, identified as protons, actually are antiprotons. Study of
these cosmic ray component begins to attract much attention, but today nothing
definite is known for the energies GeV. In any case, to realize whether
the mentioned, or some other reasons are the sources of disagreement of the
data on primaries with the data on muons, the indicated effects should be
thoroughly analyzed
Bluetooth Mesh under the Microscope: How much ICN is Inside?
Bluetooth (BT) mesh is a new mode of BT operation for low-energy devices that
offers group-based publish-subscribe as a network service with additional
caching capabilities. These features resemble concepts of information-centric
networking (ICN), and the analogy to ICN has been repeatedly drawn in the BT
community. In this paper, we compare BT mesh with ICN both conceptually and in
real-world experiments. We contrast both architectures and their design
decisions in detail. Experiments are performed on an IoT testbed using NDN/CCNx
and BT mesh on constrained RIOT nodes. Our findings indicate significant
differences both in concepts and in real-world performance. Supported by new
insights, we identify synergies and sketch a design of a BT-ICN that benefits
from both worlds
The enhancement of phase separation aspect in electron doped manganite Ca0.8Sm0.16Nd0.04MnO3
The complex lanthanide doping of electron manganites results in enhancement
of various phase separation effects in physical properties of these compounds.
Selecting Ca0.8Sm0.16Nd0.04MnO3 as a model case we show that the first order
structural phase transition from paramagnetic semi-metallic phase into
anti-ferromagnetic semi-metallic phase at TS ~ 158 +- 4 K is marked by an
abrupt decrease in magnetization, a step like anomaly DL/L = 10-4 in thermal
expansion and large latent heat DQ = 610 J/mol. In a certain temperature range
below TS, the high field magnetization exhibits hysteretic metamagnetic
behavior due to field-induced first order transformation. ac-susceptibility,
magnetization and resistivity data suggest rather a non-uniform state in
Ca0.8Sm0.16Nd0.04MnO3 at low temperatures. The metal - insulator transition
occurs at TMI ~112 +- 3 K, accompanied by a step-like increase in
magnetization. These features could be ascribed to "sponging" of electrons from
neighboring anti-ferromagnetic matrix by clusters undergoing the ferromagnetic
ordering.Comment: submitted to J.Phys. Cond. Matte
Trends in autoionization of Rydberg states converging to the 4s threshold in the Kr-Rb⁺-Sr²⁺ isoelectonic sequence: theory and experiment
We have measured the photoabsorption spectra of the Kr-like ions Rb+ and Sr2+ at photon energies corresponding to the excitation of 4s-np resonances using, the dual laser plasma photoabsorption technique. Dramatic changes in the line profiles, with increasing ionization and also proceeding along the Rydberg series of each ion, are observed and explained by the trends in 4s-transition amplitudes computed within a framework of configuration-interaction Pauli-Fock calculations. Total photoionization cross sections show very good agreement with relative absorption data extracted from the measured spectra
Design and construction of new central and forward muon counters for CDF II
New scintillation counters have been designed and constructed for the CDF
upgrade in order to complete the muon coverage of the central CDF detector, and
to extend this coverage to larger pseudorapidity. A novel light collection
technique using wavelength shifting fibers, together with high quality
polystyrene-based scintillator resulted in compact counters with good and
stable light collection efficiency over lengths extending up to 320 cm. Their
design and construction is described and results of their initial performance
are reported.Comment: 20 pages, 15 figure
Measuring extensive air showers with Cherenkov light detectors of the Yakutsk array: The energy spectrum of cosmic rays
The energy spectrum of cosmic rays in the range 10^15 eV to 6*10^19 eV has
been studied using the air Cherenkov light detectors of the Yakutsk array. The
total flux of photons produced by relativistic electrons (including positrons
as well, hereafter) of extensive air showers in the atmosphere is used as the
energy estimator of the primary particle initiating a shower. The resultant
differential flux of cosmic rays exhibits, in accordance with previous
measurements, a knee and ankle features at energies 3*10^15 and ~10^19 eV,
respectively. A comparison of observational data with simulations is made in
the knee and ankle regions in order to choose the models of galactic and
extragalactic components of cosmic rays which describe better the energy
spectrum measured.Comment: 27 pages, 22 figures, accepted for publication in New Journal of
Physics (Focus Issue
A study on the sharp knee and fine structures of cosmic ray spectra
The paper investigates the overall and detailed features of cosmic ray (CR)
spectra in the knee region using the scenario of nuclei-photon interactions
around the acceleration sources. Young supernova remnants can be the physical
realities of such kind of CR acceleration sites. The results show that the
model can well explain the following problems simultaneously with one set of
source parameters: the knee of CR spectra and the sharpness of the knee, the
detailed irregular structures of CR spectra, the so-called "component B" of
Galactic CRs, and the electron/positron excesses reported by recent
observations. The coherent explanation serves as evidence that at least a
portion of CRs might be accelerated at the sources similar to young supernova
remnants, and one set of source parameters indicates that this portion mainly
comes from standard sources or from a single source.Comment: 13 pages, 4 figures, accepted for publication in SCIENCE CHINA
Physics, Mechanics & Astronomy
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