Variations of cosmic rays according to the data of interplanetary probes Zond-3 and Venus-2

Cosmic ray intensity variation measured by Zond 3 and Venus 2 interplanetary probe

Cosmic Ray Investigation in the Stratosphere and Space: Results from Instruments on Russian Satellites and Balloons

Selected activities aimed to investigate cosmic ray fluxes and to contribute to the understanding of the mechanisms behind, over a long-time period using space research tools in the former USSR/Russia and Slovakia, are reviewed, and some of the results obtained are presented. As the selection is connected with the institutes where the authors are working, it represents only a partial review of this wide topic

Quiet time fluxes and radial gradients of low-energy protons in the inner and outer heliosphere

Radial variations of low-energy (~1-8 MeV) quiet-time fluxes of protons are examined at distances of 20-85 AU during low solar activity periods using Voyager 1-2 data and compared with Ulysses fluxes at 1-5 AU as well as IMP-8 and SOHO at Earth and Helios between 0.3 and 1 AU. To obtain nearly background-free fluxes, the data are based on a careful pulse-height analysis. Except for high solar activity periods, contaminated with solar particles, all fluxes are very low, of the order of, and below 10^(-5) /(cm^2 s sr MeV). The Ulysses fluxes seem to be the lowest, whereas Helios and Voyager fluxes are nearly at the same level. The radial variation in 1-8 MeV suggests a negative gradient from 0.5 to about 2 AU that gradually turns positive beyond 2 AU. Whereas the true variation is difficult to infer between 5 and 17 AU due to solar contribution, from 30 to about 60 AU it exhibits a wide plateau, beyond which a slight increasing tendency is observed. At energies above ~6 MeV a clear contribution of anomalous hydrogen is observed

Radial diffusion of electrons with energy greater than 100 keV in the outer radiation belt

Electron diffusion and intensity variations in outer radiation bel

LONG LASTING ENERGETIC PARTICLE INJECTION FROM A WEAK FLARE

ABSTRACT A relatively weak solar cosmic ray event registered at the Earth orbit following the flare of December 17, 1976 is discussed. The ma.in feature of the event is the existence of a prolonged unusually high proton and electron anisotropy; even at the end of the decay phase of the flare the motion of the particles were mainly directed away from the Sun.The durations of proton and electron anisotropies were different If prolonged particle injection is neglected the value of the anisotropy considerable exceeds all diffusive estimates. Time-intensity and anisotropy profiles of electrons and protons are fitted by a diffusive model including prolonged particle injection at the Sun The best agreement with the data is obtained if the duration of injection equals about 20 and 7 hours for protons and electrons, respectively

Measurement of the branching fraction of J/ψ→ρπJ/\psi\rightarrow\rho\pi at KEDR

We present the study of the decay $J/\psi \rightarrow \rho \pi$. The results are based on of 5.2 million $J/\psi$ events collected by the KEDR detector at VEPP-4M collider. The branching fraction is measured to be $\mathcal{B}(J/\psi\rightarrow\rho\pi) = \big(2.072\pm 0.017 \pm 0.056 \big)\cdot 10^{-2}$ where the first uncertainty is statistical, the second one is systematic. This is the most precise single measurement of this quantity at the moment

Ожирение и метаболические нарушения у больных хронической обструктивной болезнью легких: возможности фенотипирования

The aim of the study was to compare clinical and functional features and healthrelated quality of life (HRQoL) in patients with chronic obstructive pulmonary disease (COPD) regarding to comorbid obesity as a phenotypic sign. Methods. Patient classification was performed using Kmeans clustering analysis (MacQueen). It resulted in the classification of subjects into four clinical groups with marked differences in COPD symptoms.Results. Subjects with obesity had severe airflow limitation and dyspnoea, frequent exacerbations, severely impaired HRQoL, poor survival, decreased physical activity, insulin resistance and increased systemic inflammation.Conclusion. Thus, COPD with comorbid obesity could be considered as a distinct phenotype of COPD with severe symptoms.Целью исследования явилось изучение клиникофункциональных параметров и качества жизни (КЖ) больных хронической обструктивной болезнью легких (ХОБЛ) c сопутствующим ожирением и метаболическими нарушениями с оценкой возможности их фенотипирования. На основании кластерного анализа, проведенного по методу kсредних МакКуина, выделены 4 группы пациентов с отличительными особенностями течения ХОБЛ. Установлено, что наличие сопутствующего ожирения у больных ХОБЛ ассоциировано со значительным снижением легочной функции, переносимости физической нагрузки, показателей КЖ и выживаемости, частыми обострениями, развитием инсулинорезистентности и активацией системных воспалительных реакций. Предполагается, что клинический вариант ХОБЛ с сопутствующим ожирением целесообразно рассматривать в качестве отдельного фенотипа заболевания, характеризующегося тяжелым течением

Investigations of Structural-Functional Aspects of Epizootic Process in Natural Plague Foci in Siberia

Comprehensively studied have been structural elements of ecosystems of Siberian natural plague foci, as well as levels of integration among epizootic process components, and ways of their functional interaction. Application of the complex approach to the surveillance over structural-functional elements of the parasitic system along with investigations of epizootic process dynamics has provided for identification of peculiarities as regards epizootics development, transformation and evolution of population and carrier/vector coenosis structure in time and space. Revealed is the genetic diversity of plague microbe circulating within the bounds of separate foci and zones of focality. Determined is a long-lasting anti-epidemic effect (more than 20 years) of the field desinsection in the Saglinsk meso-focus of the Tuva natural plague focus

Energetic particle influence on the Earth's atmosphere

This manuscript gives an up-to-date and comprehensive overview of the effects of energetic particle precipitation (EPP) onto the whole atmosphere, from the lower thermosphere/mesosphere through the stratosphere and troposphere, to the surface. The paper summarizes the different sources and energies of particles, principally galactic cosmic rays (GCRs), solar energetic particles (SEPs) and energetic electron precipitation (EEP). All the proposed mechanisms by which EPP can affect the atmosphere are discussed, including chemical changes in the upper atmosphere and lower thermosphere, chemistry-dynamics feedbacks, the global electric circuit and cloud formation. The role of energetic particles in Earth’s atmosphere is a multi-disciplinary problem that requires expertise from a range of scientific backgrounds. To assist with this synergy, summary tables are provided, which are intended to evaluate the level of current knowledge of the effects of energetic particles on processes in the entire atmosphere