Effect of magnetic field geometry on the wave signature of the pickup of interstellar neutrals

Details Effect of magnetic field geometry on the wave signature of the pickup of interstellar neutrals Effect of magnetic field geometry on the wave signature of the pickup of interstellar neutrals

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994jgr....9919229w&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 99, no. A10, p. 19,229-19,244

Physics

41

Heliosphere, Interstellar Matter, Ion Distribution, Ions, Magnetic Field Configurations, Magnetic Fields, Magnetohydrodynamic Waves, Power Spectra, Spectral Signatures, Protons, Solar Wind, Wave Propagation

Scientific paper

By using the technique of Johnstone et al. (1991), the asymptotic wave spectrum induced by the pickup of interstellar ions in the heliosphere is derived. This approach is independent of quasi-linear theory. The asymptotic wave spectrum is calculated from the standard resonance condition by assuming that the asymptotic ion distribution is bispherical and by using conservation of energy. The calculation places no restriction on either the ratio of Alfven speed to solar wind flow speed or the particle pitch angle. Spectra for various geometries (relative orientations of the magnetic field and solar wind velocity) are calculated. Absolute upper limits to the expected wave enhancements are calculated. These upper limits are compared to the background fluctuation spectrum extrapolated from 0.87 AU, assuming a spectral index of -5/3 and radial dependences of -2 and -3. The heliocentric radial distances at which the peaks in the various geometry-dependent wave spectra are expected to be observable above the background are identified. Peaks due to pickup hydrogen at the proton gyrofrequency are found to be always stronger relative to the background in parallel than in perpendicular geometries. The parallel-geometry excitations consist only of sunward propagating waves. In perpendicular geometries a peak also occurs, this time near 0.1 of the proton gyrofrequency (corresponding to the peak calculated by Lee and Ip (1987)). However, the steep spectral dependence of the ambient wave field makes it unlikely that this peak will be observed inside 20 AU. A similar result holds for the case of pickup-helium induced excitation at the helium gyrofrequency. Inside 10 AU, peaks at these lower frequencies tend to be obscured by the steep frequency dependence (proportional to -5/3) of the ambient spectrum and then are only observable in parallel geometries.

Affiliated with

Also associated with

No associations

Rating

Effect of magnetic field geometry on the wave signature of the pickup of interstellar neutrals does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Effect of magnetic field geometry on the wave signature of the pickup of interstellar neutrals, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effect of magnetic field geometry on the wave signature of the pickup of interstellar neutrals will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1071795