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Analytic Modeling of Magnetic Field in the Magnetosheath and Outer Magnetosphere

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00519278" target="_blank" >RIV/67985815:_____/19:00519278 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1029/2018ja026006" target="_blank" >https://doi.org/10.1029/2018ja026006</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1029/2018JA026006" target="_blank" >10.1029/2018JA026006</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Analytic Modeling of Magnetic Field in the Magnetosheath and Outer Magnetosphere

  • Original language description

    Magnetosheath is a region surrounded by the bow shock and the magnetopause. According to statistical analysis, the boundaries can be treated as nonconfocal paraboloids of rotations. It is not easy to meet boundary conditions simultaneously on both sides. This problem is treated here and its solution is presented. A linear combination of harmonics that satisfy the condition on the magnetopause are selected in order to meet the condition on the bow shock. The method allows to calculate surface currents on the magnetopause. It is applied for typical conditions in solar wind. A modified magnetic dipole is used as a model of the magnetospheric field. Its modification is found by the method of potentials using cylindrical harmonics. Magnetopause currents are compared with results from a model with confocal paraboloids, which is commonly used in literature.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA17-06065S" target="_blank" >GA17-06065S: Solar wind variations and their impact on magnetospheric dynamics</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Journal of Geophysical Research: Space Physics

  • ISSN

    2169-9402

  • e-ISSN

  • Volume of the periodical

    124

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    14

  • Pages from-to

    2697-2710

  • UT code for WoS article

    000477707800024

  • EID of the result in the Scopus database

    2-s2.0-85064546809