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 …

Magnetohydrodynamic waves and coronal seismology: an overview of recent results

I De Moortel, VM Nakariakov - … Transactions of the …, 2012 - royalsocietypublishing.org
Recent observations have revealed that magnetohydrodynamic (MHD) waves and
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …

Slow solar wind: observations and modeling

L Abbo, L Ofman, SK Antiochos, VH Hansteen… - Space Science …, 2016 - Springer
While it is certain that the fast solar wind originates from coronal holes, where and how the
slow solar wind (SSW) is formed remains an outstanding question in solar physics even in …

Magnetohydrodynamic waves in open coronal structures

D Banerjee, S Krishna Prasad, V Pant… - Space Science …, 2021 - Springer
Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating

B De Pontieu, P Testa, J Martínez-Sykora… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …

Persistent Doppler shift oscillations observed with Hinode/EIS in the solar corona: spectroscopic signatures of Alfvénic waves and recurring upflows

H Tian, SW McIntosh, T Wang, L Ofman… - The Astrophysical …, 2012 - iopscience.iop.org
Using data obtained by the EUV Imaging Spectrometer on board Hinode, we have
performed a survey of obvious and persistent (without significant damping) Doppler shift …

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 …

What can we learn about solar coronal mass ejections, coronal dimmings, and extreme-ultraviolet jets through spectroscopic observations?

H Tian, SW McIntosh, L Xia, J He… - The Astrophysical …, 2012 - iopscience.iop.org
Solar eruptions, particularly coronal mass ejections (CMEs) and extreme-ultraviolet (EUV)
jets, have rarely been investigated with spectroscopic observations. We analyze several …

Two components of the solar coronal emission revealed by extreme-ultraviolet spectroscopic observations

H Tian, SW McIntosh, B De Pontieu… - The Astrophysical …, 2011 - iopscience.iop.org
Recent spectroscopic observations have revealed the ubiquitous presence of blueward
asymmetries of emission lines formed in the solar corona and transition region. These …

Twisting solar coronal jet launched at the boundary of an active region

B Schmieder, Y Guo, F Moreno-Insertis… - Astronomy & …, 2013 - aanda.org
Aims. A broad jet was observed in a weak magnetic field area at the edge of active region
NOAA 11106 that also produced other nearby recurring and narrow jets. The peculiar shape …