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”

A new view of coronal structures: implications for the source and acceleration of the solar wind

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F11%3APU102159" target="_blank" >RIV/00216305:26210/11:PU102159 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    A new view of coronal structures: implications for the source and acceleration of the solar wind

  • Original language description

    We show how the complement of white light and a suite of Fe coronal forbidden line images taken during total solar eclipses since 2006 have yielded new insights into the physical properties of the coronal plasma and the role of the magnetic field. The unique properties of these spectral lines make them ideal diagnostic tools for exploring the first few solar radii above the photosphere where the expansion of the corona and the acceleration of the solar wind occur. In particular, these observations showhow: (1) localized enhancements of the ion densities relative to electrons appear in some magnetic structures, (2) the transition between a collisiondominated to a collisionless plasma occurs within a heliocentric distance of 1.2 - 1.6 Rs, (3) the expanding corona is characterized by an electron temperature of 106 K, and (4) prominences are enshrouded by hot 2 . 1E6 K coronal plasma. We discuss the implications of these observations for the source and acceleration of the solarind.

  • 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%2F1469" target="_blank" >GA205/09/1469: Study of solar coronal structures and their dynamics</a><br>

  • Continuities

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

Others

  • Publication year

    2011

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of the first Asia-Pacific solar physics meeting Editors: Arnab Rai Choudhuri and Dipankar Banerjee

  • ISBN

    978-81-922926-0-1

  • ISSN

  • e-ISSN

  • Number of pages

    11

  • Pages from-to

    259-269

  • Publisher name

    Astronomica Society of India

  • Place of publication

    Dehli

  • Event location

    Bengaluru

  • Event date

    Mar 21, 2011

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article