Radio bursts provide important diagnostics of energetic phenomena of the Sun. In particular,
bursts in decimetric and metric wavelengths probe the physical conditions and the energy …

According to the standard scenario of plasma emission, escaping radiations are generated
by the nonlinear development of the kinetic bump-on-tail instability driven by a single beam …

The plasma weak turbulence theory is a perturbative nonlinear theory, which has been
proven to be quite valid in a number of applications. However, the standard weak turbulence …

Plasma emission (PE), ie, electromagnetic radiation at the plasma frequency and its second
harmonic, is a general process occurring in both astrophysical and laboratory plasmas. The …

Context. AD Leo is a young and active M dwarf with high flaring rates across the X-ray-to-
radio bands. Flares accelerate particles in the outer coronal layers and often impact exo …

Numerical procedures to generate random variates that follow loss‐cone velocity
distributions in particle simulations are presented. We propose a simple summation …

Ring-beam energetic electrons can drive two different kinetic instabilities, including the
bump-on-tail instability by the beam component and the electron cyclotron maser instability …

Solar flares release magnetic energy through reconnection, accelerating electrons into
nonthermal velocity distributions, including crescent-shaped electron populations. These …

The spaceborne solar observation system is crucial for the study of space phenomena such
as solar flares, which requires high tracking accuracy. This study presents a coupling model …

Solar radio zebras are used in the determination of the plasma density and magnetic field in
solar flare plasmas. Analyzing observed zebra stripes and assuming their generation by the …