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Quasi-periodic pulsations in solar and stellar flares: a review of underpinning physical mechanisms and their predicted observational signatures
The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been
known for over 50 years and significant progress has been made in this research area. It has …
known for over 50 years and significant progress has been made in this research area. It has …
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 …
The THESEUS space mission concept: science case, design and expected performances
THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for
investigating the early Universe and at providing a substantial advancement of multi …
investigating the early Universe and at providing a substantial advancement of multi …
A contemporary view of coronal heating
CE Parnell, I De Moortel - Philosophical Transactions of …, 2012 - royalsocietypublishing.org
Determining the heating mechanism (or mechanisms) that causes the outer atmosphere of
the Sun, and many other stars, to reach temperatures orders of magnitude higher than their …
the Sun, and many other stars, to reach temperatures orders of magnitude higher than their …
The stellar CME–flare relation: what do historic observations reveal?
Solar coronal mass ejections (CMEs) and flares have a statistically well-defined relationship,
with more energetic X-ray flares corresponding to faster and more massive CMEs. How this …
with more energetic X-ray flares corresponding to faster and more massive CMEs. How this …
Multiwavelength campaign observations of a young solar-type star, EK Draconis. I. Discovery of prominence eruptions associated with superflares
Young solar-type stars frequently produce superflares, serving as a unique window into the
young Sun-Earth environments. Large solar flares are closely linked to coronal mass …
young Sun-Earth environments. Large solar flares are closely linked to coronal mass …
Magnetic properties of solar active regions that govern large solar flares and eruptions
Solar flares and coronal mass ejections (CMEs), especially the larger ones, emanate from
active regions (ARs). With the aim of understanding the magnetic properties that govern …
active regions (ARs). With the aim of understanding the magnetic properties that govern …
Impacts of energetic particles from T Tauri flares on inner protoplanetary discs
ABSTRACT T Tauri stars are known to be magnetically active stars subject to strong flares
observed in X-rays. These flares are likely due to intense magnetic reconnection events …
observed in X-rays. These flares are likely due to intense magnetic reconnection events …
X-ray flares in Orion young stars. I. Flare characteristics
KV Getman, ED Feigelson, PS Broos… - The Astrophysical …, 2008 - iopscience.iop.org
Abstract Pre-main-sequence (PMS) stars are known to produce powerful X-ray flares, which
resemble magnetic reconnection solar flares scaled by factors up to 10 4. However, there …
resemble magnetic reconnection solar flares scaled by factors up to 10 4. However, there …
Swift and XMM–Newton observations of an RS CVn-type eclipsing binary SZ Psc: superflare and coronal properties
We present an in-depth study of a large and long duration (> 1.3 d) X-ray flare observed on
an RS CVn-type eclipsing binary system SZ Psc using observations from Swift observatory …
an RS CVn-type eclipsing binary system SZ Psc using observations from Swift observatory …