<?xml version="1.0" encoding="utf-8"?>
<journal>
  <titleid/>
  <issn>2304-9782, 2618-8686, 2405-7223</issn>
  <journalInfo lang="ENG">
    <title>St. Petersburg Polytechnic University Journal: Physics and Mathematics</title>
  </journalInfo>
  <issue>
    <number>1</number>
    <altNumber>116</altNumber>
    <dateUni>2011</dateUni>
    <pages/>
    <articles>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>7-11</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Orlenko</surname>
              <initials>Fedor</initials>
              <email>fadler@mail.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Zegrya</surname>
              <initials>Georgiy</initials>
              <email>zegrya@theory.ioffe.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Metal — insulator transition in a nonmagnetic InSb crystal semiconductor in the magnetic field</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">A Hamiltonian of the exchange interaction in the spin representation is developed for the couples of particles with spins equal to 3/2. The ground antiferromagnetic state is degenerated in respect to the total spin of the acceptor couple. The degeneracy is removed by a strong magnetic field that induces a transition into a magnetic and (at the same time) a conducting state.</abstract>
        </abstracts>
        <codes>
          <udk>539.1(075.8)</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>hamiltonian of particle system</keyword>
            <keyword>spin of 3/2</keyword>
            <keyword>ground state fragmentation</keyword>
            <keyword>removal of degeneracy</keyword>
            <keyword>magnetic field</keyword>
            <keyword>insulator - metal transition</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.1/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>11-18</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Emelyanov</surname>
              <initials>Victor</initials>
              <email>resso2003@bk.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Kalyuzhniy</surname>
              <initials>Nikolai</initials>
              <email>nickk@mail.ioffe.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <surname>Mintairov</surname>
              <initials>Mikhail</initials>
              <email>mamint@mail.ioffe.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <surname>Mintairov</surname>
              <initials>Sergei</initials>
              <email>mintairov@scell.ioffe.ru</email>
            </individInfo>
          </author>
          <author num="005">
            <individInfo lang="ENG">
              <surname>Shvarts</surname>
              <initials>Maxim</initials>
              <email>Shvarts M.Z.</email>
            </individInfo>
          </author>
          <author num="006">
            <individInfo lang="ENG">
              <surname>Lantratov</surname>
              <initials>Vladimir</initials>
              <email>Lantratov V.M.</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Optimization of the concentrator three-junctional solar cells</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The influence of epilayer structure parameters of tandem GalnP/GalnAs/Ge solar cells on sunlight conversion efficiency has been investigated. The optimal choice of thicknesses and doping levels of emitters of GalnP and GalnAs subcells were shown to allow to improve efficiency of the solar cells up to 4 %.</abstract>
        </abstracts>
        <codes>
          <udk>621.383.8:537.313</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>solar cell</keyword>
            <keyword>multijunction</keyword>
            <keyword>simulation</keyword>
            <keyword>optical concentrator</keyword>
            <keyword>chromatic aberration</keyword>
            <keyword>optimization</keyword>
            <keyword>epilayer structure</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.2/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>18-25</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Zelikman</surname>
              <initials>Mark</initials>
              <email>marzelik@mail.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Potseluev</surname>
              <initials>Kirill</initials>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The influence of structural factor on the Meissner state in the 3D-ordered Josephson medium</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The system of difference equations based on the conditions of fluxoid quantization in the cells is obtained. A method of solutions of the system for the Meissner configuration for all values of parameters is proposed. The current configurations as well as the critical field above which the Meissner configuration does not exist are calculated.</abstract>
        </abstracts>
        <codes>
          <udk>538.945</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>granulated superconductors</keyword>
            <keyword>3D-ordered josephson medium</keyword>
            <keyword>Meissner effect</keyword>
            <keyword>conditions of fluxoid quantization</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.3/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>26-28</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Nemov</surname>
              <initials>Sergei</initials>
              <email>nemov_s@mail.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Filippov</surname>
              <initials>Stanislav</initials>
              <email>stanislav.filippov@gmail.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Calculation of parameters of tin impurity states in bismuth telluride using the Hall effect data</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">Basing on experimental temperature dependence of the Hall factor in telluride bismuth crystal doped with tin and iodine, chemical potential of holes and energy of two-electron impurity states of tin have been calculated within framework of two-band model at the temperature range of 77—330 K. Coefficient of temperature drift of tin two-electron level relatively the top of the valence band and value of Hubbard energy were estimated.</abstract>
        </abstracts>
        <codes>
          <udk>621/315.529</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>Hall effect</keyword>
            <keyword>bismuth telluride</keyword>
            <keyword>tin</keyword>
            <keyword>correlation energy</keyword>
            <keyword>impurity states</keyword>
            <keyword>AVBV1</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.4/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>29-36</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Ganin</surname>
              <initials>Pavel</initials>
              <email>ganin-pavel@rambler.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Schmidt</surname>
              <initials>Alexander</initials>
              <email>alexander.schmidt@mail.ioffe.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Theoretical estimation of the diameter of the droplets formed in a breakup of the largest droplets in the process vessel with stirring</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">In a liquid-liquid system with mechanical stirring a mechanism of fine droplets fraction formation doesn't have complete theoretical explanation. The paper presents a theoretical estimation of a diameter of the smallest daughter droplets formed in the process vessel in a breakup of largest droplets of polydispersed emulsion.</abstract>
        </abstracts>
        <codes>
          <udk>532.517.4:532.529.5</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>core of turbulent flow</keyword>
            <keyword>breakup of droplets</keyword>
            <keyword>fine fraction</keyword>
            <keyword>mechanism of formation</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.5/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>36-44</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Pletnev</surname>
              <initials>Alexander</initials>
              <email>AAPletnev@yandex.rii</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Talalov</surname>
              <initials>Victor</initials>
              <email>vtalalov@phmf.spbstu.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Mathematical model of heat and mass transfer in the electric furnace molten slag bath</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">Both mathematical model and economical calculation algorithm for numerical simulation of the heat and mass transfer processes in the molten slag bath of the rectangular electric smelting furnace have been carried out. The high intensive operational conditions of the furnace are investigated.</abstract>
        </abstracts>
        <codes>
          <udk>621.365.23:534.24.001.57</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>electric smelting furnace</keyword>
            <keyword>mathematical model</keyword>
            <keyword>charge</keyword>
            <keyword>intensification of melting process</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.6/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>44-55</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Snegirev</surname>
              <initials>Aleksandr</initials>
              <email>a.snegirev@phmf.spbstu.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Sazhin</surname>
              <initials>Sergei</initials>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <surname>Talalov</surname>
              <initials>Victor</initials>
              <email>vtalalov@phmf.spbstu.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">A model and computational algorithm for heat exchange and evaporation of droplets of dispersed liquid</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The model of unsteady nonisothermal droplet vaporization of atomized liquid is formulated, taking into account the temperature gradient and liquid recirculation inside the droplet. An efficient and absolutely stable algorithm is developed for further use in numerical simulations of turbulent evaporating sprays.</abstract>
        </abstracts>
        <codes>
          <udk>536.423</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>droplet evaporation</keyword>
            <keyword>liquid spray</keyword>
            <keyword>simulation</keyword>
            <keyword>liquid dispersed</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.7/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>55-60</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Krivtsun</surname>
              <initials>Alexander</initials>
              <email>a.krivtcun@gmail.com</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Seteikin</surname>
              <initials>Alexey</initials>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">An analysis of light propagation process in biological media using graphics processing units technique</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">A number of issues arising when solving task of numerical simulating of light propagation process has been considered. Numerical results for media with different sets of optical properties are presented and validated against other groups. A new approach towards increasing of calculating performance is presented.</abstract>
        </abstracts>
        <codes>
          <udk>519.245, 535.34, 535, 36</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>Monte-Carlo method</keyword>
            <keyword>voxel</keyword>
            <keyword>optical properties</keyword>
            <keyword>scattering</keyword>
            <keyword>photon</keyword>
            <keyword>statistical weight</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.8/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>61-70</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>MBN Research Center at Frankfurt Innovation Center of Biotechnology</orgName>
              <surname>Verkhovtsev</surname>
              <initials>Alexei</initials>
              <email>verkhovtsev@mbnexplorer.com</email>
              <address>Frankfurt am Main, Germany</address>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Polozkov</surname>
              <initials>Roman</initials>
              <email>polozkov@tuexph.stu.neva.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <authorCodes>
              <researcherid>M-5766-2013</researcherid>
              <scopusid>57192222016</scopusid>
              <orcid>0000-0002-3584-4583</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Ivanov</surname>
              <initials>Vadim</initials>
              <email>ivanov_vk@spbstu.ru</email>
              <address>Russia, 195251, St.Petersburg, Polytechnicheskaya, 29</address>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <orgName>MBN Research Center at Frankfurt Innovation Center of Biotechnology</orgName>
              <surname>Korol</surname>
              <initials>Andrei</initials>
              <email>korol@mbnexplorer.com </email>
              <address>Frankfurt am Main, Germany </address>
            </individInfo>
          </author>
          <author num="005">
            <authorCodes>
              <scopusid>7003387326</scopusid>
              <orcid>0000-0003-1602-6144</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>MBN Research Center at Frankfurt Innovation Center of Biotechnology</orgName>
              <surname>Solov'yov</surname>
              <initials>Andrei</initials>
              <email>solovyov@mbnresearch.com</email>
              <address>3 Altenhöferallee, Frankfurt am Main, 60438, Germany</address>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">An investigation of the electronic structure of noble gas endohedral fullerenes</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The results of the first self-consistent calculation of the electronic structure of endohedral compounds He@C60, Ne@C60 and Ar@C60 within the Hartree—Fock approximation are presented. The influence of the exchange electron-electron interaction on the hybridization process is studied.</abstract>
        </abstracts>
        <codes>
          <udk>538.915, 539.19, 544.183.2</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>endohedral fullerene</keyword>
            <keyword>noble gas</keyword>
            <keyword>Hartree-Fock approximation</keyword>
            <keyword>central field approximation</keyword>
            <keyword>jellium model</keyword>
            <keyword>orbital</keyword>
            <keyword>hybridization</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.9/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>71-77</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Kozlov</surname>
              <initials>Vladimir</initials>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Trofimov</surname>
              <initials>Pavel</initials>
              <email>fizmattrofimov@mail.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <surname>Akimov</surname>
              <initials>Alexei</initials>
              <email>akimov_ia@mail.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The inverse Hankel transformation for the mixed boundary value problem in the closed interval</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The formula of the inverse Hankel transformation for the mixed boundary value problem for requirements of the first and the third sort is gained. Connection with a solution of the mixed problem for requirements of a first labour is considered.</abstract>
        </abstracts>
        <codes>
          <udk>517.444</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>Hankel transform</keyword>
            <keyword>Bessel functions</keyword>
            <keyword>transformation kernel</keyword>
            <keyword>boundary condition</keyword>
            <keyword>thermal conductivity</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.10/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>78-81</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Ivanov</surname>
              <initials>Yuri</initials>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Nevskiy</surname>
              <initials>Sergei</initials>
              <email>nevskiy_sa@physics.sibsiu.ru</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <surname>Konovalov</surname>
              <initials>Sergey</initials>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <surname>Gromov</surname>
              <initials>Victor</initials>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The influence of electrical potential on changing a dislocation substructure of aluminium at a stress relaxation</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">Aluminium samples tested for stress relaxation both under normal conditions and under electrical potential have been investigated using transmission diffraction electron microscopy. An essential change of dislocation substructure parameters was revealed.</abstract>
        </abstracts>
        <codes>
          <udk>539.8</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>aluminium</keyword>
            <keyword>stress relaxation</keyword>
            <keyword>dislocation substructure</keyword>
            <keyword>electrical potential</keyword>
            <keyword>flexural extinction countour</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.11/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>82-87</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Elizarova</surname>
              <initials>Marina</initials>
              <email>melizl@yandex.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Mironov</surname>
              <initials>Vladimir</initials>
              <email>vladimir.mironov@ymail.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">An estimation of inaccuracy in dosimetric data smoothing when installing the remote radiation therapy planning system</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">Smoothing errors of dosimetric data due to preparation for radiation therapy treatment planning system are considered. Parametrization and numeric estimation of those errors are performed. Practical recommendations concerning smoothing procedure during experimental dosimetric data preparation are given.</abstract>
        </abstracts>
        <codes>
          <udk>34.49.29, 61:539.1.074,53:088</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>photon beams dosimetry</keyword>
            <keyword>smoothing algorithms</keyword>
            <keyword>radiation therapy</keyword>
            <keyword>remote radiation treatment planning system</keyword>
            <keyword>error analysis</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.12/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>88-93</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Charikov</surname>
              <initials>Yuri</initials>
              <email>y.charikov@yandex.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Sklyarova</surname>
              <initials>Elena</initials>
              <email>sklyarova.mhd@mail.ioffe.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The concept of the origin of thermal flares on the Sun</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The paper formulates the main items underlying the concept of the origin of thermal flares on the Sun which generate X-rays in the 1-8 A range with a power not above 10~ Вт/м. An analysis of the data amassed for the 0.5.07.2009 flare provides convincing support for the concept proposed.</abstract>
        </abstracts>
        <codes>
          <udk>523.985.3</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>sun</keyword>
            <keyword>solar activity</keyword>
            <keyword>flares</keyword>
            <keyword>X-RAYS</keyword>
            <keyword>temporal structure</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.13/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>94-98</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Nesterenok</surname>
              <initials>Alexander</initials>
              <email>alex-nlO@yandex.ru</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Naidenov</surname>
              <initials>Victor</initials>
              <email>alex-n10 @yandex.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The simulation of propagation of cosmic rays nucleonic component in the Earth's atmosphere</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The paper is devoted to statistical simulation of propagation processes of secondary cosmic rays and its interaction with the Earth's atmosphere. We present the simulation results of integral and differential fluxes of cosmic rays nucleons. The comparison between our results and experimental data is done.</abstract>
        </abstracts>
        <codes>
          <udk>524.1</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>cosmic rays</keyword>
            <keyword>nucleon1c component</keyword>
            <keyword>cosmogen1c nuclides</keyword>
            <keyword>atmospere</keyword>
            <keyword>earth</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.14/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>99-105</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Kropotina</surname>
              <initials>Yuliya</initials>
              <email>Kropotina Yu.A.</email>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Gustov</surname>
              <initials>Maxim</initials>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <surname>Krasil’shchikov</surname>
              <initials>Alexander</initials>
              <email>kra@astro.ioffe.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <surname>Levenfish</surname>
              <initials>Kseniya</initials>
              <email>ksen@astro.ioffe.ru</email>
            </individInfo>
          </author>
          <author num="005">
            <individInfo lang="ENG">
              <surname>Pavlov</surname>
              <initials>Georgiy</initials>
              <email>pavlov@astro.psu.edu</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Multiprocessor 3D-hybrid code for astrophysical plasma modeling</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">An original multiprocessor 3D divergence-free hybrid code is presented. The code allows for efficient modeling of collisionless processes in plasma on the scale of ion gyroradii. An example of resonant electromagnetic ion-ion instability simulation is provided.</abstract>
        </abstracts>
        <codes>
          <udk>533.9</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>hybrid modeling</keyword>
            <keyword>astrophys1cal plasma</keyword>
            <keyword>divergence-free algorithm</keyword>
            <keyword>parallel programming</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.15/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>106-110</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <orgName>Ioffe Institute</orgName>
              <surname>Bykov</surname>
              <initials>Andrey</initials>
              <email>byk@astro.ioffe.ru</email>
              <address>St. Petersburg, Russian Federation</address>
            </individInfo>
          </author>
          <author num="002">
            <individInfo lang="ENG">
              <surname>Gladilin</surname>
              <initials>Petr</initials>
              <email>peter.gladilin@gmail.com</email>
            </individInfo>
          </author>
          <author num="003">
            <individInfo lang="ENG">
              <surname>Osipov</surname>
              <initials>Sergey</initials>
              <email>osm2004@mail.ru</email>
            </individInfo>
          </author>
          <author num="004">
            <individInfo lang="ENG">
              <surname>Pavlov</surname>
              <initials>Georgiy</initials>
              <email>pavlov@astro.psu.edu</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">A new class of galactic X-ray sources resulting from interaction of stellar wind with a supernova remnant</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">A model of energetic particle acceleration in the vicinity of expanding supernova shell and of young massive star having powerful stellar wind has been considered. The source was shown to be characterized by unusually hard spectral energy distribution in X- and gamma-ray energy bands.</abstract>
        </abstracts>
        <codes>
          <udk>524.3-17, 524.354</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>interstellar medium</keyword>
            <keyword>supernova remnants</keyword>
            <keyword>particles acceleration at shock waves</keyword>
            <keyword>stellar wind</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.16/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>111-115</pages>
        <authors>
          <author num="001">
            <authorCodes>
              <orcid>0000-0003-4292-0959</orcid>
            </authorCodes>
            <individInfo lang="ENG">
              <orgName>Peter the Great St. Petersburg Polytechnic University</orgName>
              <surname>Golovitski</surname>
              <initials>Alexander</initials>
              <email>alexandergolovitski@yahoo.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">The low-current low-pressure glow discharge in the electronegative gases</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The physical mechanisms of the existence of two stages of glow discharge in the electronegative gases have been analysed. The electron attachment is shown to be the main mechanism of electron decay at the low-current stage, whereas the diffusion-aided removing — to be that at the high-current stage.</abstract>
        </abstracts>
        <codes>
          <udk>533.9</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>glow discharge</keyword>
            <keyword>electronegative gases</keyword>
            <keyword>electron attachment</keyword>
            <keyword>plasma modeling</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.17/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>116-122</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Nguyen</surname>
              <initials>Van</initials>
              <email>thangspbstu@mail.ru</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Forces and moments acting on a rapidly rotating floating bearing with allowance of lubrication hydrodynamics and centrifugal force</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The problems of theoretical representation of questions of forces and moments acting on a rapidly rotating floating bearing with allowance of centrifugal force and oil hydrodynamics. The basic results are given with reference to research of short bearing.</abstract>
        </abstracts>
        <codes>
          <udk>621.822.171-251</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>centrifugal forces</keyword>
            <keyword>stability</keyword>
            <keyword>Reynold's equations</keyword>
            <keyword>moment</keyword>
            <keyword>short bearing</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.18/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>122-129</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Zhgutov</surname>
              <initials>Vladimir</initials>
              <email>abc.kitezh@gmail.com</email>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Mathematical models, the research algorythm and the ribbed shells steadiness analysis at finite bending flexure</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG">The mathematical deformation models and the algorithm of the elastic ribbed shells research accounting geometrical nonlinearity, shifting and bending rigidity of the ribs, and the transverse shifts are proposed. The examples of the solutions for the metal, organic-glass and concrete shells are given. The critical load for the elastic behavior of the material is estimated.</abstract>
        </abstracts>
        <codes>
          <udk>539.3</udk>
        </codes>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword>elastic ribbed shells</keyword>
            <keyword>geometrical nonlinearity</keyword>
            <keyword>shifting and bending rigidity of the ribs</keyword>
            <keyword>transverse shifts</keyword>
            <keyword>steadiness</keyword>
            <keyword>critical load</keyword>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.19/</furl>
          <file/>
        </files>
      </article>
      <article>
        <artType>RAR</artType>
        <langPubl>RUS</langPubl>
        <pages>130-140</pages>
        <authors>
          <author num="001">
            <individInfo lang="ENG">
              <surname>Kesamanly</surname>
              <initials>Fagam</initials>
            </individInfo>
          </author>
        </authors>
        <artTitles>
          <artTitle lang="ENG">Andrey Dmitrievich Sakharov (on the occasion of his 90th birthday)</artTitle>
        </artTitles>
        <abstracts>
          <abstract lang="ENG"/>
        </abstracts>
        <codes/>
        <keywords>
          <kwdGroup lang="ENG">
            <keyword/>
          </kwdGroup>
        </keywords>
        <files>
          <furl>https://physmath.spbstu.ru/article/2011.10.20/</furl>
          <file/>
        </files>
      </article>
    </articles>
  </issue>
</journal>
