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Secondary Emission From Clusters Composed of Spherical Grains

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F16%3A10334190" target="_blank" >RIV/00216208:11320/16:10334190 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1109/TPS.2015.2509238" target="_blank" >http://dx.doi.org/10.1109/TPS.2015.2509238</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1109/TPS.2015.2509238" target="_blank" >10.1109/TPS.2015.2509238</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Secondary Emission From Clusters Composed of Spherical Grains

  • Original language description

    Dust grains or their clusters can be frequently found in many space environments-interstellar clouds, atmospheres of planets, tails of comets, or planetary rings are only typical examples. Space dust grains are formed by various processes and their shapes are complex. These grains are exposed to electrons with different energies, and thus, they can acquire positive or negative charge during this interaction. We present a systematic study of well-defined systems-clusters consisting of different numbers of small spherical (1 mu m) grains and such objects can be considered as examples of real irregularly shaped space grains. The charges acquired by investigated objects as well as their secondary emission yields are calculated using the secondary emission model. We have found that: 1) the charge and surface potential of clusters exposed to the electron beam are influenced by the number of grains and by their geometry within a particular cluster; 2) the model results are in an excellent agreement with the experiment; and 3) there is a large difference between charging of a cluster levitating in the free space and that attached to a planar surface. The calculation provides a reduction of the secondary electron emission yield of the surface covered by dust clusters by a factor of 1.5 with respect to the yield of a smooth surface.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BL - Plasma physics and discharge through gases

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2016

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    IEEE Transactions on Plasma Science

  • ISSN

    0093-3813

  • e-ISSN

  • Volume of the periodical

    44

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    7

  • Pages from-to

    505-511

  • UT code for WoS article

    000374162900012

  • EID of the result in the Scopus database

    2-s2.0-84953297929