Detail publikačního výsledku

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

HABBAL, S.; MORGAN, H.; DRUCKMÜLLER, M.

Originální název

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

Anglický název

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

Druh

Stať ve sborníku v databázi WoS či Scopus

Originální abstrakt

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 show how: (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.

Anglický abstrakt

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 show how: (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.

Klíčová slova

Sun, corona, solar wind, eclipses

Klíčová slova v angličtině

Sun, corona, solar wind, eclipses

Autoři

HABBAL, S.; MORGAN, H.; DRUCKMÜLLER, M.

Rok RIV

2013

Vydáno

21.04.2011

Nakladatel

Astronomica Society of India

Místo

Dehli

ISBN

978-81-922926-0-1

Kniha

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

Edice

ASI Conference Series, 2011, Vol. 2

Strany od

259

Strany do

269

Strany počet

11

BibTex

@inproceedings{BUT97460,
  author="Shadia Rifai {Habbal} and Huw {Morgan} and Miloslav {Druckmüller}",
  title="A new view of coronal structures: implications for the source and acceleration of the solar wind",
  booktitle="Proceedings of the first Asia-Pacific solar physics meeting Editors: Arnab Rai Choudhuri and Dipankar Banerjee",
  year="2011",
  series="ASI Conference Series, 2011, Vol. 2",
  number="1",
  pages="259--269",
  publisher="Astronomica Society of India",
  address="Dehli",
  isbn="978-81-922926-0-1"
}