Abstract:
Large-amplitude electrostatic waves propagating parallel to the background magnetic
field have been observed at the Earth’s magnetopause by the Magnetospheric Multiscale (MMS)
spacecraft. These waves are observed in the region where there is an intermixing of magnetosheath
and magnetospheric plasmas. The plasma in the intermixing region is modeled as a five-component
plasma consisting of three types of electrons, namely, two counterstreaming hot electron beams and
cold electrons, and two types of ions, namely, cold background protons and a hot proton beam.
Sagdeev pseudo-potential technique is used to study the parallel propagating nonlinear electrostatic
solitary structures. The model predicts four types of modes, namely, slow ion-acoustic mode, fast
ion-acoustic mode, slow electron-acoustic mode and fast electron-acoustic modes. Except the fast
ion-acoustic mode, all other modes support solitons. Whereas slow ion-acoustic solitons have positive
potentials, both slow and fast electron-acoustic solitons have negative potentials. For the case of
4% cold electron density, the slow ion-acoustic solitons have electric field (40–120) mV m1. The fast
Fourier transforms (FFT) of slow ion-acoustic solitons produce broadband frequency spectra having
peaks between 100 Hz to 1000 Hz. These theoretical predictions are in good agreement with
the observations. The slow and fast electron-acoustic solitons could be relevant in explaining the
low-intensity high (>1 kHz) frequency waves which are also observed at the same time.
