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”

Far Magnetotail Observations of an Interplanetary Shock

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10192206" target="_blank" >RIV/00216208:11320/13:10192206 - isvavai.cz</a>

  • Result on the web

    <a href="http://www.mff.cuni.cz/veda/konference/wds/proc/pdf13/WDS13_203_f2_Grygorov.pdf" target="_blank" >http://www.mff.cuni.cz/veda/konference/wds/proc/pdf13/WDS13_203_f2_Grygorov.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Far Magnetotail Observations of an Interplanetary Shock

  • Original language description

    We present a study of the impact of the interplanetary (IP) shock on December 7, 2003 in the distant tail of the Earth's magnetosphere. Using the data from the several spacecraft located in the solar wind in front of the Earth, we monitor the propagationof the IP shock from the L1 point to the magnetosphere and to magnetotail. Taking into account its velocity and beginning of the substorm onset from the ground, we considered the plasma parameters on the Wind spacecraft located downstream at XGSM MINUSSIGN 230 RE. Shortly after the shock arrival, Wind crossed consequentially southern and northern lobes in between which observed a flux rope and the tailward fast plasma flow ( 780 km/s) in the plasmasheet. We found that a orientation of the nominal tailaxis is affected by VY components of the solar wind. Also, according to Wind data, we present a sketch how the distant tail moves with respect to the IP shock passage.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BL - Plasma physics and discharge through gases

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GA205%2F09%2F0170" target="_blank" >GA205/09/0170: The role of solar wind disturbances in Space Weather</a><br>

  • Continuities

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

Others

  • Publication year

    2013

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    WDS'13 Proceedings of Contributed Papers: Part II - Physics of Plasmas and Ionized Media

  • ISBN

    978-80-7378-251-1

  • ISSN

  • e-ISSN

  • Number of pages

    10

  • Pages from-to

    20-29

  • Publisher name

    Matfyzpress

  • Place of publication

    Praha

  • Event location

    Praha

  • Event date

    Jun 4, 2013

  • Type of event by nationality

    EUR - Evropská akce

  • UT code for WoS article