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Study of the Proton Beam Parameters Near the Sun

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10513138" target="_blank" >RIV/00216208:11320/25:10513138 - isvavai.cz</a>

  • Result on the web

    <a href="https://physics.mff.cuni.cz/wds/proc/pdf25/WDS25_05_f2_Satyasmita.pdf" target="_blank" >https://physics.mff.cuni.cz/wds/proc/pdf25/WDS25_05_f2_Satyasmita.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Study of the Proton Beam Parameters Near the Sun

  • Original language description

    The solar wind often shows two proton populations: a dense proton core anda faster, less dense proton beam. The relative abundance of the proton beam is typically10-20 %, and it drifts relative to the core along the interplanetary magnetic field at about1.2 local Alfven speed. The origin and evolution of the proton beam are not yet fully &apos;understood. Previous studies using Helios data suggest that the seed of the proton beamforms close to the Sun. In the paper, we investigate the radial evolution of various protonbeam parameters observed by the Parker Solar Probe between 0.05 and 0.7 AU. Wefind that the largest changes of the proton beam parameters (such as relative abundanceand drift velocity) occur up to 0.3 AU. We also study and discuss how the proton beamcharacteristics vary under different conditions in the solar wind, classified by collisionalage and cross-helicity

  • 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

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

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

Others

  • Publication year

    2025

  • 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;25 Proceedings of Contributed Papers - Physics

  • ISBN

    978-80-7378-532-1

  • ISSN

  • e-ISSN

  • Number of pages

    6

  • Pages from-to

    47-52

  • Publisher name

    Matfyzpress

  • Place of publication

    Prague

  • Event location

    Praha

  • Event date

    Jun 3, 2025

  • Type of event by nationality

    EUR - Evropská akce

  • UT code for WoS article