Magnetohydrodynamic oscillations in the solar corona and Earth's magnetosphere: towards consolidated understanding

VM Nakariakov, V Pilipenko, B Heilig, P Jelínek… - Space Science …, 2016 - Springer
Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

[HTML][HTML] Large-scale globally propagating coronal waves

A Warmuth - Living Reviews in Solar Physics, 2015 - Springer
Large-scale, globally propagating wave-like disturbances have been observed in the solar
chromosphere and by inference in the corona since the 1960s. However, detailed analysis …

> 25 MeV proton events observed by the high energy telescopes on the STEREO A and B spacecraft and/or at Earth during the first∼ seven years of the STEREO …

IG Richardson, TT Von Rosenvinge, HV Cane… - Coronal …, 2014 - Springer
Using observations from the High Energy Telescopes (HETs) on the STEREO A and B
spacecraft and similar observations from near-Earth spacecraft, we summarize the …

The first widespread solar energetic particle event of solar cycle 25 on 2020 November 29-Shock wave properties and the wide distribution of solar energetic particles

A Kouloumvakos, RY Kwon… - Astronomy & …, 2022 - aanda.org
Context. On 2020 November 29, an eruptive event occurred in an active region located
behind the eastern solar limb as seen from Earth. The event consisted of an M4. 4 class …

Simultaneous horizontal and vertical oscillation of a quiescent filament observed by CHASE and SDO

J Dai, Q Zhang, Y Qiu, C Li, Z Li, S Li… - The Astrophysical …, 2023 - iopscience.iop.org
In this paper, we present the imaging and spectroscopic observations of the simultaneous
horizontal and vertical large-amplitude oscillation of a quiescent filament triggered by an …

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 …

The driver of coronal mass ejections in the low corona: a flux rope

X Cheng, J Zhang, MD Ding, Y Liu… - The Astrophysical …, 2013 - iopscience.iop.org
ABSTRACT Recent Solar Dynamic Observatory observations reveal that coronal mass
ejections (CMEs) consist of a multi-temperature structure: a hot flux rope and a cool leading …

Chromosphere to 1 AU simulation of the 2011 March 7th event: a comprehensive study of coronal mass ejection propagation

M Jin, WB Manchester, B Van Der Holst… - The Astrophysical …, 2017 - iopscience.iop.org
We perform and analyze the results of a global magnetohydrodynamic simulation of the fast
coronal mass ejection (CME) that occurred on 2011 March 7. The simulation is made using …

Large-scale coronal propagating fronts in solar eruptions as observed by the atmospheric imaging assembly on board the solar dynamics observatory—an ensemble …

NV Nitta, CJ Schrijver, W Liu - The Astrophysical Journal, 2013 - iopscience.iop.org
This paper presents a study of a large sample of global disturbances in the solar corona with
characteristic propagating fronts as intensity enhancement, similar to the phenomena that …

ICME evolution in the inner heliosphere: Invited review

JG Luhmann, N Gopalswamy, LK Jian, N Lugaz - Solar Physics, 2020 - Springer
ICMEs (interplanetary coronal mass ejections), the heliospheric counterparts of what is
observed with coronagraphs at the Sun as CMEs, have been the subject of intense interest …