no code implementations • 4 Jan 2021 • Peijin Zhang, Chuanbing Wang, Eduard P. Kontar
For the first time, the variation of the apparent source size, burst duration, and source position of both fundamental emission and harmonic emission at frequency 35 MHz are simulated as the function of the anisotropic parameter $\alpha$ and the angular scattering rate coefficient $\eta =\epsilon^2/h_0$, where $\epsilon^2={\langle \delta n^2\rangle}/{n^2}$ is the density fluctuation level and $h_0$ is its correlation length near the wave exciting site.
Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
1 code implementation • 23 May 2019 • Peijin Zhang, Chuanbing Wang, Lin Ye, Yuming Wang
In this work, we propose a forward-modeling method to study the trajectory and speed of the interplanetary (IP) Type-III radio burst exciter.
Solar and Stellar Astrophysics Space Physics
