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”

Magnetopause Location Under Influence of Large Solar Wind Structures

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10406370" target="_blank" >RIV/00216208:11320/19:10406370 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.mff.cuni.cz/veda/konference/wds/proc/pdf19/WDS19_22_f2_Salohub.pdf" target="_blank" >https://www.mff.cuni.cz/veda/konference/wds/proc/pdf19/WDS19_22_f2_Salohub.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Magnetopause Location Under Influence of Large Solar Wind Structures

  • Original language description

    We investigate the magnetopause (MP) location influenced by large solar wind (SW) structures: magnetic clouds (MCs), interplanetary coronal mass ejections (ICMEs), and intervals following interplanetary shocks (IPs) driven by these structures and compare it with the MP location in the pristine SW. We focus on the differences between predicted and encountered MP locations near the subsolar point. For predictions, we used the MP model of Shue et al. [1997] where Wind plasma and magnetic field parameters from 2007 to 2015 have been applied as input data. Into the model, we added other pressure components reflecting the different alpha particle content and larger magnetic field. We found that differences between the modeled and observed (by the THEMIS spacecraft) MP locations in the subsolar region are small but systematic. We discuss changes in model predictions and other factors which are not included in the model but can affect of the magnetopause location (for example, geomagnetic activity demonstrated by SYM-H and AE indices in our case).

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10305 - Fluids and plasma physics (including surface physics)

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

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

Others

  • Publication year

    2019

  • 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&apos;19 Proceedings of Contributed Papers — Physics

  • ISBN

    978-80-7378-409-6

  • ISSN

  • e-ISSN

  • Number of pages

    7

  • Pages from-to

    124-130

  • Publisher name

    Matfyzpress

  • Place of publication

    Praha

  • Event location

    Praha

  • Event date

    Jun 4, 2019

  • Type of event by nationality

    EUR - Evropská akce

  • UT code for WoS article