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”

Multi-spacecraft Investigation of ICME-driven Interplanetary Shock Interaction on the Solar Wind Turbulence in the Inner Heliosphere

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F23%3A10477797" target="_blank" >RIV/00216208:11320/23:10477797 - isvavai.cz</a>

  • Result on the web

    <a href="https://physics.mff.cuni.cz/wds/proc/pdf23/WDS23_04_f2_Park.pdf" target="_blank" >https://physics.mff.cuni.cz/wds/proc/pdf23/WDS23_04_f2_Park.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Multi-spacecraft Investigation of ICME-driven Interplanetary Shock Interaction on the Solar Wind Turbulence in the Inner Heliosphere

  • Original language description

    Recent space missions enable multi-point analysis of solar wind turbulence inthe inner heliosphere. We identify an ICME event in March 2022, and estimate changes ofspectral properties such as spectral index, magnetic helicity, and magnetic compressibilityacross an ICME-driven shock using the spacecraft of Solar Orbiter, ACE, DSCOVR, andWind. Another ICME event identified by Trotta et al. [2023] is adopted for the comparisonof these properties. Despite a small number of events leading to inconclusive results ofevolution with the heliocentric distance, several common trends are observed in both cases:little change of spectral steepness, decreasing jump of magnetic helicity and compressibility, and increasing power enhancement of fluctuations from up- to downstream with theheliocentric distance. However, for a deeper insight on the nature of the radial propagationof these parameters, statistical analyses with a larger number of events are essential.

  • 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/GA23-06401S" target="_blank" >GA23-06401S: Where and how the solar wind is accelerated and heated and how these processes affect its evolution?</a><br>

  • Continuities

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

Others

  • Publication year

    2023

  • 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;23 Proceedings of Contributed Papers - Physics

  • ISBN

    978-80-7378-503-1

  • ISSN

  • e-ISSN

  • Number of pages

    7

  • Pages from-to

    28-34

  • Publisher name

    Matfyzpress

  • Place of publication

    Praha

  • Event location

    Praha

  • Event date

    May 30, 2023

  • Type of event by nationality

    EUR - Evropská akce

  • UT code for WoS article