All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Interplanetary shock-bow shock interaction: Comparison of a global MHD model and observation

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10319613" target="_blank" >RIV/00216208:11320/15:10319613 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.pss.2014.12.001" target="_blank" >http://dx.doi.org/10.1016/j.pss.2014.12.001</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.pss.2014.12.001" target="_blank" >10.1016/j.pss.2014.12.001</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Interplanetary shock-bow shock interaction: Comparison of a global MHD model and observation

  • Original language description

    A fast forward shock passing through the bow shock would generate a train of new discontinuities that differ with the distance from the Sun-Earth line. However, interplanetary (IP) shocks are often followed by a rotation of the interplanetary magnetic field (IMF) over a large angle and a presence of this rotation can modify the interaction process. The present paper analyzes in detail one IP shock where data measured by Wind are used as an input to a global BATS-R-US MHD model and the model prediction is compared with Geotail magnetosheath observations. The study is based on three runs of the global MHD model that use different modifications of upstream conditions. We have found that (1) about 45% of IP shocks is followed by a significant IMF rotationwithin 15 min after the shock ramp; (2) the IMF rotation modifies the dynamics of the magnetospheric response to the IP shock arrival; (3) a train of new discontinuities created by an interaction of the IP shock with bow shock can be iden

  • 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

    S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2015

  • 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

    115

  • Issue of the periodical within the volume

    Sep

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    8

  • Pages from-to

    4-11

  • UT code for WoS article

    000360512300002

  • EID of the result in the Scopus database

    2-s2.0-84938749334