Add to ORKGThis "rapporteur" report discusses the solar photosphere and low chromosphere in the context of chemical composition studies. The highly dynamical nature of the photosphere does not seem to jeopardize precise determination of solar abundances in classical fashion. It is still an open question how the highly dynamical nature of the low chromosphere contributes to first ionization potential (FIP) fractionation
The solar corona and chromosphere are often marked by eruptive features, such as flares, prominences...
Context. The solar chromosphere and the lower transition region are believed to play a crucial role ...
The solar photospheric carbon abundance has been determined from [C I], CI, CH vibration-rotation, C...
Abstract. This “rapporteur ” report discusses the solar photosphere and low chromosphere in the cont...
The composition of the solar plasma is an important tool to study several physical processes, e.g. t...
Context. The comparison of coronal and photospheric abundances in cool stars is an essential questi...
The solar chemical composition is an important ingredient in our understanding of the formation, str...
For the purposes of this thesis, the lower ionosphere is defined as the ionized region beneath the E...
Systematic anomalies that seem to follow the first ionisation potential (FIP) of the minor, heavy el...
International audienceThe chemical composition of solar and stellar atmospheres differs from the com...
International audienceContext. The first ionization potential (FIP) bias is currently used to trace ...
The determination of electron density in the solar atmosphere using diagnostic line ratios has been ...
Although it is well known that solar energetic particles are depleted in elements with first ionizat...
Context. The elemental composition of the solar wind differs from the solar photospheric composition...
The relative chemical abundances between CI meteorites and the solar photosphere exhibit a significa...
The solar corona and chromosphere are often marked by eruptive features, such as flares, prominences...
Context. The solar chromosphere and the lower transition region are believed to play a crucial role ...
The solar photospheric carbon abundance has been determined from [C I], CI, CH vibration-rotation, C...
Abstract. This “rapporteur ” report discusses the solar photosphere and low chromosphere in the cont...
The composition of the solar plasma is an important tool to study several physical processes, e.g. t...
Context. The comparison of coronal and photospheric abundances in cool stars is an essential questi...
The solar chemical composition is an important ingredient in our understanding of the formation, str...
For the purposes of this thesis, the lower ionosphere is defined as the ionized region beneath the E...
Systematic anomalies that seem to follow the first ionisation potential (FIP) of the minor, heavy el...
International audienceThe chemical composition of solar and stellar atmospheres differs from the com...
International audienceContext. The first ionization potential (FIP) bias is currently used to trace ...
The determination of electron density in the solar atmosphere using diagnostic line ratios has been ...
Although it is well known that solar energetic particles are depleted in elements with first ionizat...
Context. The elemental composition of the solar wind differs from the solar photospheric composition...
The relative chemical abundances between CI meteorites and the solar photosphere exhibit a significa...
The solar corona and chromosphere are often marked by eruptive features, such as flares, prominences...
Context. The solar chromosphere and the lower transition region are believed to play a crucial role ...
The solar photospheric carbon abundance has been determined from [C I], CI, CH vibration-rotation, C...