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The space environment of Mercury at the times of the second and third MESSENGER flybys

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F11%3A00381399" target="_blank" >RIV/68378289:_____/11:00381399 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/11:00481685

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.pss.2011.01.018" target="_blank" >http://dx.doi.org/10.1016/j.pss.2011.01.018</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.pss.2011.01.018" target="_blank" >10.1016/j.pss.2011.01.018</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The space environment of Mercury at the times of the second and third MESSENGER flybys

  • Original language description

    The second and third flybys of Mercury by the MESSENGER spacecraft occurred, respectively, on 6 October 2008 and on 29 September 2009. In order to provide contextual information about the solar wind properties and the interplanetary magnetic field (IMF)near the planet at those times, we have used an empirical modeling technique combined with a numerical physics-based solar wind model. The Wang?Sheeley?Arge (WSA) method uses solar photospheric magnetic field observations (from Earth-based instruments) in order to estimate the inner heliospheric radial flow speed and radial magnetic field out to 21.5 solar radii from the Sun. This information is then used as input to the global numerical magnetohydrodynamic model, ENLIL, which calculates solar wind velocity, density, temperature, and magnetic field strength and polarity throughout the inner heliosphere. WSA-ENLIL calculations are presented for the several-week period encompassing the second and third flybys. This information, in conjunc

  • Czech name

  • Czech description

Classification

  • Type

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

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2011

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Planetary and Space Science

  • ISSN

    0032-0633

  • e-ISSN

  • Volume of the periodical

    59

  • Issue of the periodical within the volume

    15

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    9

  • Pages from-to

    2066-2074

  • UT code for WoS article

    000298722800023

  • EID of the result in the Scopus database