The FIP and inverse FIP effects in solar and stellar coronae
We review our state of knowledge of coronal element abundance anomalies in the Sun and
stars. We concentrate on the first ionization potential (FIP) effect observed in the solar …
stars. We concentrate on the first ionization potential (FIP) effect observed in the solar …
Coronal loops: observations and modeling of confined plasma
Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …
brightness to the dense confined plasma, and this review focuses on loops mostly as …
Multi-scale variability of coronal loops set by thermal non-equilibrium and instability as a probe for coronal heating
Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
A systematic survey of high-temperature emission in solar active regions
The recent analysis of observations taken with the EUV Imaging Spectrometer and X-Ray
Telescope instruments on Hinode suggests that well-constrained measurements of the …
Telescope instruments on Hinode suggests that well-constrained measurements of the …
Achievements of Hinode in the first eleven years
Hinode Review Team, K Al-Janabi… - Publications of the …, 2019 - academic.oup.com
Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …
Evidence for widespread cooling in an active region observed with the SDO atmospheric imaging assembly
ABSTRACT A well-known behavior of EUV light curves of discrete coronal loops is that the
peak intensities of cooler channels or spectral lines are reached at progressively later times …
peak intensities of cooler channels or spectral lines are reached at progressively later times …
Observing coronal nanoflares in active region moss
ABSTRACT The High-resolution Coronal Imager (Hi-C) has provided Fe xii 193Å images of
the upper transition region moss at an unprecedented spatial (∼ 0 farcs 3–0 farcs 4) and …
the upper transition region moss at an unprecedented spatial (∼ 0 farcs 3–0 farcs 4) and …
Enthalpy-based thermal evolution of loops. II. Improvements to the model
This paper develops the zero-dimensional (0D) hydrodynamic coronal loop model" Enthalpy-
based Thermal Evolution of Loops"(EBTEL) proposed by Klimchuk et al., which studies the …
based Thermal Evolution of Loops"(EBTEL) proposed by Klimchuk et al., which studies the …
Patterns of nanoflare storm heating exhibited by an active region observed with solar dynamics observatory/atmospheric imaging assembly
It is largely agreed that many coronal loops—those observed at a temperature of about 1 MK—
are bundles of unresolved strands that are heated by storms of impulsive nanoflares. The …
are bundles of unresolved strands that are heated by storms of impulsive nanoflares. The …
The origin of reconnection-mediated transient brightenings in the solar transition region
The ultraviolet emission from the solar transition region is dominated by dynamic, low-lying
magnetic loops. The enhanced spatial and temporal resolution of the solar observation …
magnetic loops. The enhanced spatial and temporal resolution of the solar observation …