Inter-network regions of the Sun at millimetre wavelengths

2007/05/18 by S. Wedemeyer-Böhm, S. Wedemeyer-Boehm, H.‐G. Ludwig +5 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20077588

15 pages, 10 figures, accepted for publication in A&A (15.05.07)

arxiv created 2007/05/18 · openalex publication_date 2007/05/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01

Abstract

Aims.The continuum intensity at wavelengths around 1 mm provides an excellent way to probe the solar chromosphere and thus valuable input for the ongoing controversy on the thermal structure and the dynamics of this layer. The synthetic continuum intensity maps for near-millimetre wavelengths presented here demonstrate the potential of future observations of the small-scale structure and dynamics of internetwork regions on the Sun.

Citations

• Solar atmospheric oscillations and the chromospheric magnetic topology

Cited by

• A First Comparison of Millimeter Continuum and Mg ii Ultraviolet Line Emission from the Solar Chromosphere