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The fluxes of carbon dioxide generated during this degradation were deduced from differences in the carbon isotope abundance ratios of glucose δ13C = -11.4 per mil) and SOM δ13C = -27.01 per mil).
      
Analytical expressions for the direct and reverse fluxes of molecular aggregates over the first and second potential barriers of the aggregation work in the presence of spherical and cylindrical micelles in non-ionic surfactant solution were derived.
      
Analytical expressions for the direct and reverse fluxes of molecular aggregates over the first and second potential barriers of the aggregation work in the presence of spherical and cylindrical micelles in non-ionic surfactant solution were derived.
      
These bursts were identified with powerful solar flares, during which time fluxes of hard X-ray radiation, meter-wave radio bursts (types II and IV), and coronal transients were observed.
      
The results of measuring the fluxes of ionospheric ions in the nightside polar cap at an altitude of about 20 000 km are presented.
      
Based on the earlier measurements by the AKEBONO satellite, nothing could be said about the fluxes of thermal ions in this zone, because of the insufficient sensitivity of the instrument aboard this satellite.
      
Emphasis is placed on research into the fluxes of electrons, whose possibility to be accelerated by shock waves is problematic.
      
Various possibilities of the origination of the steplike variations of the background fluxes of protons and helium nuclei with energies of 0.3-10 MeV per nucleon, correlated with similar GCR variations, are discussed.
      
Prediction of Absorbed Doses for Spacecraft Irradiated by Particle Fluxes of Solar Cosmic Rays
      
A new method of evaluating the absorbed dose onboard spacecraft under the action of particle fluxes of solar cosmic rays (SCR) is described.
      
We consider cases of simultaneous detection of the absorbed doses produced by proton fluxes of powerful solar events onboard the Mir and ISS orbital stations and the Ekspress A3 geosynchronous satellite.
      
Statistical Correlation of the Rate of Failures on Geosynchronous Satellites with Fluxes of Energetic Electrons and Protons
      
Fluxes of Quasi-trapped Electrons with Energies >0.08 MeV in the Near-Earth Space on Drift Shells L >lt; 2
      
These data are compared to the results of observation of the solar wind and interplanetary magnetic field, as well as to the data on fluxes of solar cosmic rays.
      
Radio bursts in the frequency range 100-1500 kHz and fluxes of energetic electrons with energies of 20-450 keV recorded onboard the Interball-1 satellite during prominent chromospheric flares on the Sun are studied.
      
Variations in fluxes of quasi-trapped energetic protons were studied on the basis of the data of the CORONAS-I satellite.
      
Short increases of the fluxes of electrons with energies > 0.08 MeV at low-latitude (L >lt; 2) regions of near-Earth space
      
Statistical properties of the fluxes of energetic ions and solar wind in the region of intersection of shock wave fronts in the
      
For a binary eletrolyte in the leading approximation in the small parameter rD(R2 - r1)-1, where rD is the Debye radius, the migration current can be eliminated, and one need consider only the diffusion and convective fluxes of the ions [2].
      
The Stefan-Maxwell equations for diffusion fluxes of plasma in a magnetic field
      
 

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