Distribution of MHD wave activity in the foreshock region and properties of backstreaming protons
- 1. Istituto di Fisica dello Spazio Interplanetary, CNR
Description
Magnetic field and plasma data obtained by ISEE 2 experiments in the earth's foreshock region have been used, in conjugation with a shock model, to correlate with geometrical parameters the intensity of MHD trubulence and some moments of the distributions of back-streaming protons. The geometrical parameters are the distance of the observation point from the proton foreshock boundary and the distance from the shock surface. The results obtained allow a preliminary discussion of two basic problem of the physics of the foreshock. These are (1) the relative role of shock struture and/or wave particle interaction in determining the form of the backscattering ion distribution and (2) the physical mechanism determining the observed saturation of the MHD turbulence
Additional details
Publishing Information
- Journal Title
- J. Geophys. Res.
- Journal Volume
- 88
- Journal Issue
- A11
- Series
- J. Geophys. Res.
- Journal Page Range
- 9280-9286
- ISSN
- 0022-1406
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 15058631
- Subject category
- S58: GEOSCIENCES;
- Descriptors DEI
- BACKSCATTERING; EARTH MAGNETOSPHERE; HYDROMAGNETIC WAVES; MAGNETOSHEATH; PLASMA DENSITY; PROTON SPECTRA; SHOCK WAVES; SOLAR WIND; TURBULENCE
- Descriptors DEC
- EARTH ATMOSPHERE; SCATTERING; SOLAR ACTIVITY; SPECTRA; STELLAR WINDS