Spatially resolved plasma composition evolution in a solar flare–The effect of reconnection outflow
Context. Solar flares exhibit complex variations in elemental abundances compared to
photospheric values. These abundance variations, characterized by the first ionization …
photospheric values. These abundance variations, characterized by the first ionization …
Intriguing plasma composition pattern in a solar active region: a result of nonresonant Alfvén waves?
The plasma composition of the solar corona is different from that of the solar photosphere.
Elements that have a low first ionization potential (FIP) are preferentially transported to the …
Elements that have a low first ionization potential (FIP) are preferentially transported to the …
Deciphering the birth region, formation, and evolution of ambient and transient solar wind using heavy ion observations
This paper outlines key scientific topics that are important for the development of solar
system physics and how observations of heavy ion composition can address them. The key …
system physics and how observations of heavy ion composition can address them. The key …
What determines active region coronal plasma composition?
T Mihailescu, D Baker, LM Green… - The Astrophysical …, 2022 - iopscience.iop.org
The chemical composition of the solar corona is different from that of the solar photosphere,
with the strongest variation being observed in active regions (ARs). Using data from the …
with the strongest variation being observed in active regions (ARs). Using data from the …
The case for solar full-disk spectral diagnostics: Chromosphere to corona
In the context of the recent call for white papers for the Decadal Survey for Solar and Space
Physics (Heliophysics) 2024–2033, we present the argument that spatially-resolved spectral …
Physics (Heliophysics) 2024–2033, we present the argument that spatially-resolved spectral …
Comprehensive Analysis of a Filament-embedding Solar Active Region at Different Stages of Evolution
J Zhao, F Yu, SE Gibson, Y Fan, Y Su… - The Astrophysical …, 2024 - iopscience.iop.org
Active regions are the brightest structures seen in the solar corona, so their physical
properties hold important clues to the physical mechanisms underlying coronal heating. In …
properties hold important clues to the physical mechanisms underlying coronal heating. In …
The eruption of a magnetic flux rope observed by Solar Orbiter and Parker Solar Probe
Magnetic flux ropes are a key component of coronal mass ejections, forming the core of
these eruptive phenomena. However, determining whether a flux rope is present prior to …
these eruptive phenomena. However, determining whether a flux rope is present prior to …
The eruption of a magnetic flux rope observed by\textit {Solar Orbiter} and\textit {Parker Solar Probe}
Magnetic flux ropes are a key component of coronal mass ejections, forming the core of
these eruptive phenomena. However, determining whether a flux rope is present prior to …
these eruptive phenomena. However, determining whether a flux rope is present prior to …
[PDF][PDF] The case for solar full-disk spectral diagnostics
In this white paper submitted to the Decadal Survey for Solar and Space Physics
(Heliophysics) 2024-2033 we argue that spatially-resolved spectral diagnostics over the full …
(Heliophysics) 2024-2033 we argue that spatially-resolved spectral diagnostics over the full …
Coronal Plasma Composition Evolution and Solar Activity
ASH To - 2023 - discovery.ucl.ac.uk
Composition of plasma in the solar corona is a tracer of the flow of plasma and energy from
the solar interior. A complete understanding of coronal abundances not only provides us …
the solar interior. A complete understanding of coronal abundances not only provides us …