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Improving the Ni I atomic model for solar and stellar atmospheric models
(IOP Publishing, 2013-05-10)
Neutral nickel (Ni I) is abundant in the solar atmosphere and is one of the important elements that contribute to the emission and absorption of radiation in the spectral range between 1900 and 3900 Å. Previously, the Solar ...
Shallow extra mixing in solar twins inferred from Be abundances
(EDP Sciences, 2015-03-10)
Context. Lithium and beryllium are destroyed at different temperatures in stellar interiors. As such, their relative abundances offer excellent probes of the nature and extent of mixing processes within and below the ...
Lower and middle atmosphere and ozone layer responses to solar variation
(Cambridge University Press, 2010-02)
Global warming in the troposphere and the decrease of stratospheric ozone concentration has become a major concern to the scientific community. The increase in greenhouse gases and aerosols concentration is believed to be ...
Energy input flux in the global quiet-sun corona
(IOP Publishing, 2017-07)
We present first results of a novel technique that provides, for the first time, constraints on the energy input flux at the coronal base (r ∼ 1.025 R o) of the quiet Sun at a global scale. By combining differential emission ...
Hydrostatic equilibrium preservation in MHD numerical simulation with stratified atmospheres: Explicit Godunov-type schemes with MUSCL reconstruction
(EDP Sciences, 2019-11)
Many astrophysical processes involving plasma flows are produced in the context of a gravitationally stratified atmosphere in hydrostatic equilibrium, in which strong gradients can exist with gas properties that vary in ...
Evolution of the solar activity over time and effects on planetary atmospheres. ii. κ1 ceti, an analog of the sun when life arose on earth∗
(American Astronomical Society, 2020)
Magnetic reconnection along quasi-separatrix layers as a drivers of ubiquitous active region outflows
(IOP Publishing, 2009-11)
Hinode´s EUV Imaging Spectrometer (EIS) has discovered ubiquitous outflows of a few to 50 km s<sup>-1</sup> from active regions (ARs). These outflows are most prominent at the AR boundary and appear over monopolar magnetic ...