Reversal-free Ca II H profiles: a challenge for solar chromosphere modeling in quiet inter-network

2008/04/15 by R. Rezaei, J. H. M. J. Bruls, W. Schmidt +3 · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Biology #Botany #Chromosphere #Magnetic field #Physics #QUIET #Solar and Space Plasma Dynamics #Solar atmosphere #Spectral line #Stellar, planetary, and galactic studies #Stratification (seeds) #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079050

8 pages, accepted in A&A

arxiv created 2008/04/15 · openalex publication_date 2008/04/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. We study chromospheric emission to understand the temperature stratification in the solar chromosphere.

Citations

• Observation of a short-lived pattern in the solar chromosphere
• Physical properties of solar chromospheric plages

Cited by

• The energy of waves in the photosphere and lower chromosphere
• The energy of waves in the photosphere and lower chromosphere