555 research outputs found
A dip in the UHECR spectrum and the transition from galactic to extragalactic cosmic rays
The dip is a feature in the diffuse spectrum of ultra-high energy (UHE)
protons caused by electron-positron pair production on the cosmic microwave
background (CMB) radiation. For a power-law generation spectrum , the
calculated position and shape of the dip is confirmed with high accuracy by the
spectra observed by the Akeno-AGASA, HiRes, Yakutsk and Fly's Eye detectors.
When the particle energies, measured in these detectors, are calibrated by the
dip, their fluxes agree with a remarkable accuracy. The predicted shape of the
dip is quite robust. The dip is only modified strongly when the fraction of
nuclei heavier than protons is high at injection, which imposes some
restrictions on the mechanisms of acceleration operating in UHECR sources. The
existence of the dip, confirmed by observations, implies that the transition
from galactic to extragalactic cosmic rays occurs at E \lsim 1\times 10^{18}
eV. We show that at energies lower than a characteristic value eV, the spectrum of extragalactic cosmic rays
flattens in all cases of interest, and it provides a natural transition to a
steeper galactic cosmic ray spectrum. This transition occurs at some energy
below , corresponding to the position of the so-called second knee.
We discuss extensively the constraints on this model imposed by current
knowledge of acceleration processes and sources of UHECR and compare it with
the traditional model of transition at the ankle.Comment: Version Accepted for Publication in Astroparticle Physics (minor
changes
Ionospheric effects during first 2 hours after the Chelyabinsk meteorite impact
This paper presents the analysis of ionospheric effects in the region close
to the Chelyabinsk meteorite explosion at 03:20UT 2013 February 15 from the
Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of
Sciences (ISTP SB RAS) EKB radar data, and from the Institute of Geophysics of
Ural Branch of Russian Academy of Sciences (IG UB RAS) PARUS ionosonde data.
Both instruments are located within the IG UB RAS Arti Observatory
approximately 200 km northward from the estimated explosion site. According to
the data obtained, the ionospheric disturbance caused by the meteorite flyby,
explosion, and impact had high dynamics and amplitude. However, it obviously
did not lead to a variation in the ionosphere mean parameters in the region
above the disturbance center during the first 2 hours. Essential effects,
however, were observed at more than 100-200 km from the explosion site and
farther up to 1500 km.Comment: 30 pages, 15 figures, submitted to JAST
Electric Field Effect in Atomically Thin Carbon Films
We report a naturally-occurring two-dimensional material (graphene that can
be viewed as a gigantic flat fullerene molecule, describe its electronic
properties and demonstrate all-metallic field-effect transistor, which uniquely
exhibits ballistic transport at submicron distances even at room temperature
Assessing the quality of medical care and developing the ratings of health services: experience of using Medicare program in the USA
To provide patient's security is the main goal in some spheres of health care, that is why methods of statistical monitoring were developed to detect abnormalities in the course of medical work quickly and confidentially. This includes, for example, excessive intervention even without further damage to a patient's safety. Therefore, it is very important to determine whether the risk to a patient's life exists or how abnormal the situation is. At the present moment health care in Russia has already passed the initial stage of formation of ratings to assess the quality of medical care services. Almost all regions of the Russian Federation have their own ratings. The question is how objectively they reflect the quality of medical services. The article presents main features to assess the quality of health care to rate medical organizations on the example of state program Medicare (USA) in order to compare them with the ones used in Russian ratings
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