Origin and structures of solar eruptions I: magnetic flux rope
Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
A type II radio burst driven by a blowout jet on the Sun
Type II radio bursts are often associated with coronal shocks that are typically driven by
coronal mass ejections (CMEs) from the Sun. Here we conduct a case study of a type II radio …
coronal mass ejections (CMEs) from the Sun. Here we conduct a case study of a type II radio …
Characteristics of late-phase> 100 MeV gamma-ray emission in solar eruptive events
GH Share, RJ Murphy, SM White… - The Astrophysical …, 2018 - iopscience.iop.org
We characterize and catalog 30 solar eruptive events observed by the Fermi Large Area
Telescope (LAT) having late-phase> 100 MeV γ-ray emission (LPGRE), identified 30 yr ago …
Telescope (LAT) having late-phase> 100 MeV γ-ray emission (LPGRE), identified 30 yr ago …
A new tool for CME arrival time prediction using machine learning algorithms: CAT-PUMA
Coronal mass ejections (CMEs) are arguably the most violent eruptions in the solar system.
CMEs can cause severe disturbances in interplanetary space and can even affect human …
CMEs can cause severe disturbances in interplanetary space and can even affect human …
Spatially resolved radio signatures of electron beams in a coronal shock
Context. Type II radio bursts are a type of solar radio bursts associated with coronal shocks.
Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of …
Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of …
Solar coronal density turbulence and magnetic field strength at the source regions of two successive metric type II radio bursts
We report spectral and polarimeter observations of two weak, low-frequency (≈ 85–60 MHz)
solar coronal type II radio bursts that occurred on 2020 May 29 within a time interval≈ 2 …
solar coronal type II radio bursts that occurred on 2020 May 29 within a time interval≈ 2 …
The acceleration of high-energy protons at coronal shocks: the effect of large-scale streamer-like magnetic field structures
Recent observations have shown that coronal shocks driven by coronal mass ejections can
develop and accelerate particles within several solar radii in large solar energetic particle …
develop and accelerate particles within several solar radii in large solar energetic particle …
Acceleration of solar energetic particles through CME-driven shock and streamer interaction
F Frassati, M Laurenza, A Bemporad… - The Astrophysical …, 2022 - iopscience.iop.org
On 2013 June 21, a solar prominence eruption was observed, accompanied by an M2. 9
class flare, a fast coronal mass ejection, and a type II radio burst. The concomitant emission …
class flare, a fast coronal mass ejection, and a type II radio burst. The concomitant emission …
Source imaging of a moving type IV solar radio burst and its role in tracking coronal mass ejection from the inner to the outer corona
Source imaging of solar radio bursts can be used to track energetic electrons and
associated magnetic structures. Here we present a combined analysis of data at different …
associated magnetic structures. Here we present a combined analysis of data at different …
Verification of the standard theory of plasma emission with particle-in-cell simulations
Z Zhang, Y Chen, S Ni, C Li, H Ning, Y Li… - The Astrophysical …, 2022 - iopscience.iop.org
The standard theory of plasma emission is based on kinetic couplings between a single
beam of energetic electrons and unmagnetized thermal plasmas, involving multistep …
beam of energetic electrons and unmagnetized thermal plasmas, involving multistep …