Coronal loops: observations and modeling of confined plasma
F Reale - Living Reviews in Solar Physics, 2014 - Springer
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 …
Advances in observing various coronal EUV waves in the SDO era and their seismological applications (invited review)
W Liu, L Ofman - Solar Physics, 2014 - Springer
Global extreme-ultraviolet (EUV) waves are spectacular traveling disturbances in the solar
corona associated with energetic eruptions such as coronal mass ejections (CMEs) and …
corona associated with energetic eruptions such as coronal mass ejections (CMEs) and …
Models and data analysis tools for the Solar Orbiter mission
AP Rouillard, RF Pinto, A Vourlidas, A De Groof… - Astronomy & …, 2020 - aanda.org
Context. The Solar Orbiter spacecraft will be equipped with a wide range of remote-sensing
(RS) and in situ (IS) instruments to record novel and unprecedented measurements of the …
(RS) and in situ (IS) instruments to record novel and unprecedented measurements of the …
The width, density, and outflow of solar coronal streamers
H Morgan, AC Cook - The Astrophysical Journal, 2020 - iopscience.iop.org
Characterizing the large-scale structure and plasma properties of the inner corona is crucial
to understanding the source and subsequent expansion of the solar wind and related space …
to understanding the source and subsequent expansion of the solar wind and related space …
Unexpected behavior of the solar wind mass flux during solar maxima: two peaks at middle heliolatitudes
In this work we study the temporal and latitudinal variations of the solar wind mass flux at 1
AU derived from SOHO/SWAN data on backscattered solar Lyman-α α radiation in 1996 …
AU derived from SOHO/SWAN data on backscattered solar Lyman-α α radiation in 1996 …
STEREO observations of fast magnetosonic waves in the extended solar corona associated with EIT/EUV waves
We report white-light observations of a fast magnetosonic wave associated with a coronal
mass ejection observed by STEREO/SECCHI/COR1 inner coronagraphs on 2011 August 4 …
mass ejection observed by STEREO/SECCHI/COR1 inner coronagraphs on 2011 August 4 …
Dynamic three-dimensional tomography of the solar corona
Empirical, three-dimensional electron-density maps of the solar corona can be
tomographically reconstructed using polarized-brightness images measured from ground …
tomographically reconstructed using polarized-brightness images measured from ground …
Solar stereoscopy and tomography
MJ Aschwanden - Living Reviews in Solar Physics, 2011 - Springer
We review stereoscopic and tomographic methods used in the solar corona, including
ground-based and space-based measurements, using solar rotation or multiple spacecraft …
ground-based and space-based measurements, using solar rotation or multiple spacecraft …
CME reconstruction: Pre-STEREO and STEREO era
A Thernisien, A Vourlidas, RA Howard - Journal of Atmospheric and Solar …, 2011 - Elsevier
Since the first observations of coronal mass ejections (CMEs) in 1970s, their three-
dimensional (3D) morphology has been a key ingredient for understanding their origin and …
dimensional (3D) morphology has been a key ingredient for understanding their origin and …
Global coronal seismology in the extended solar corona through fast magnetosonic waves observed by STEREO SECCHI COR1
We present global coronal seismology for the first time, which allows us to determine
inhomogeneous magnetic field strength in the extended corona. From the measurements of …
inhomogeneous magnetic field strength in the extended corona. From the measurements of …