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Comparison of the solar corona and the coronae above accretion disks surrounding black holes

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F05%3A00031566" target="_blank" >RIV/67985815:_____/05:00031566 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Comparison of the solar corona and the coronae above accretion disks surrounding black holes

  • Original language description

    We develop a model of an accretion disk corona motivated by the observed solar corona.

  • Czech name

    Porovnání vlastností sluneční koróny s vlastnostmi koróny akrečních disků okolo černých děr

  • Czech description

    Diskutujeme model akrečního disku motivovaný vlastnostmi sluneční koróny.

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/IAA300030510" target="_blank" >IAA300030510: Radiation processes near compact objects: timing and polarimetry studies</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2005

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Astrophysical Sources of High Energy Particles and Radiation

  • ISBN

    0-7354-0290-6

  • ISSN

  • e-ISSN

  • Number of pages

    4

  • Pages from-to

    188-191

  • Publisher name

    Springer

  • Place of publication

    New York

  • Event location

    Torun

  • Event date

    Jun 20, 2005

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article