Harmonic electron-cyclotron maser emissions driven by energetic electrons of the horseshoe distribution with application to solar radio spikes^⋆

¹ Institute of Space Sciences, Shandong University, Shandong, PR China
e-mail: yaochen@sdu.edu.cn
² Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, PR China

Received: 27 January 2021
Accepted: 11 May 2021

Abstract

Context. Electron-cyclotron maser emission (ECME) is the favored mechanism for solar radio spikes and has been investigated extensively since the 1980s. Most studies relevant to solar spikes employ a loss-cone-type distribution of energetic electrons, generating waves mainly in the fundamental X/O mode (X1/O1), with a ratio of plasma oscillation frequency to electron gyrofrequency (ω_pe/Ω_ce) lower than 1. Despite the great progress made in this theory, one major problem is how the fundamental emissions pass through the second-harmonic absorption layer in the corona and escape. This is generally known as the escaping difficulty of the theory.

Aims. We study the harmonic emissions generated by ECME driven by energetic electrons with the horseshoe distribution to solve the escaping difficulty of ECME for solar spikes.

Methods. We performed a fully kinetic electromagnetic particle-in-cell simulation with ω_pe/Ω_ce = 0.1, corresponding to the strongly magnetized plasma conditions in the flare region, with energetic electrons characterized by the horseshoe distribution. We also varied the density ratio of energetic electrons to total electrons (n_e/n₀) in the simulation. To analyze the simulation result, we performed a fast Fourier transform analysis on the fields data.

Results. We obtain efficient amplification of waves in Z and X2 modes, with a relatively weak growth of O1 and X3. With a higher-density ratio, the X2 emission becomes more intense, and the rate of energy conversion from energetic electrons into X2 modes can reach ∼0.06% and 0.17%, with n_e/n₀ = 5% and 10%, respectively.

Conclusions. We find that the horseshoe-driven ECME can lead to an efficient excitation of X2 and X3 with a low value of ω_pe/Ω_ce, providing novel means for resolving the escaping difficulty of ECME when applied to solar radio spikes. The simultaneous growth of X2 and X3 can be used to explain some harmonic structures observed in solar spikes.