Magnetic structure of the solar transition region as observed in various ultraviolet lines emitted at different temperatures

2006/08/04 by E. Marsch, G.-Q. Zhou, Guangsu Zhou +4 · 2 citations
Physics and Astronomy · #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #Astro and Planetary Science

paper · pdf · doi:10.1051/0004-6361:20065665

Abstract

Aims.The structure of the solar transition region (TR) in a polar coronal hole of the Sun is studied. In particular, the detailed association of the coronal magnetic field (carpet) with the radiance patterns of the TR, when seen in various far ultraviolet (FUV) emission lines, is investigated.

Citations

• On the outflow in an equatorial coronal hole
• Coronal plasma flows and magnetic fields in solar active regions

Cited by

• Sizes of transition-region structures in coronal holes and in the quiet Sun
• The Solar Orbiter mission

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