TRANSPORT OF ANISOTROPIC INTERSTELLAR PICKUP IONS ON BENT FLUX TUBES

Citation
Pa. Isenberg et Ma. Lee, TRANSPORT OF ANISOTROPIC INTERSTELLAR PICKUP IONS ON BENT FLUX TUBES, J GEO R-S P, 103(A6), 1998, pp. 12037-12047
Citations number
22
Categorie Soggetti
Geosciences, Interdisciplinary","Astronomy & Astrophysics","Metereology & Atmospheric Sciences",Oceanografhy,"Geochemitry & Geophysics
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
103
Issue
A6
Year of publication
1998
Pages
12037 - 12047
Database
ISI
SICI code
2169-9380(1998)103:A6<12037:TOAIPI>2.0.ZU;2-B
Abstract
We present a simple model of anisotropic pickup ion distributions on a flux tube containing both a radial segment and segments oriented perp endicular to the radial direction. The flux tube is carried away from the Sun by a constant speed solar wind. We model the pitch-angle scatt ering of these ions by a hemispherical approximation, which assumes th at the scattering is instantaneous except through the pitch angle of 9 0 degrees, where the scattering is finite. The model includes a radial ly dependent ionization of pickup ions, with the newly created ions co ncentrated in the sunward hemisphere within the radial segment but dis tributed equally between the hemispheres in the perpendicular segments . The pickup ions stream along the magnetic field and decelerate in th e expanding solar wind, but we assume that the radial segment is short enough that the effects of adiabatic focusing may be neglected. For w eak scattering through 90 degrees, the distributions exhibit nonlocal properties due to ion streaming along the field from regions where con ditions are different than observed locally. We find that this model c an yield a depletion of antisunward ions in the radial segment of the flux tube, such as has been observed, but the streaming of ions into t he radial region limits the size of this effect unless the radial segm ent is very long.