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Newly discovered source of turbulence and heating in the solar chromosphere
Above the Sun's luminous photosphere lies the solar chromosphere, where the temperature increases from below 4000 K to over 1 million K. Though physicists do not understand the...
University Corporation for Atmospheric Research100
Shock wave formation heights using 2D density and Alfvén maps of the corona
Poster Presented at the National Astronomy Meeting (NAM) 2013 by Pietro Zucca
Figshare2016-01-18 更新70
Net radiative cooling rates and partial ionization in cool coronal condensations
Provided data files contain voxel-based Net Radiative Cooling Rate (NRCR) values and also the electron densities (in 1/cm3) for each combination of temperature (T), pressure (p) and the distance from
Zenodo2025-05-22 更新10
Coronal plasma diagnostics from ground-based observations
In this paper we discuss the potential of ground-based visible observations of the solar corona to address the key open problems in the physics of the solar atmosphere and of...
DASH Search90
Quiet-sun hydrogen Lyman-alpha line profile
The solar radiation in the Lyman-alpha spectral line of hydrogen plays a significant role in the illumination of chromospheric and coronal structures, such as prominences,...
B2FIND40
