Production of ion conics by oblique double layers
Journal Article
·
· J. Geophys. Res.; (United States)
Magnetized test ions are subjected to acceleration through a numerically simulated oblique double layer in order to determine whether they emerge with velocity vectors aligned with or oblique to the ambient magnetic field. A criterion for oblique alignment, depending on the double-layer parameters and on the external magnetization, is obtained. When it is applied to observed and theoretical auroral double layers, this criterion predicts that accelerated heavy ions will be substantially less magnetic field aligned than will accelerated hydrogen ions, thus suggesting auroral double layers as a source of high-energy ion conics. Test particle simulations are also used to investigate the perpendicular heating of ions at low altitudes by the electric fields associated with moving auroral arcs. The rapid motion of small-scale structures in the arces is suggested as a source of low-energy conical ion distributions, and the slow drifts of the entire arc forms are inferred to heat ionospheric ions.
- Research Organization:
- Los Alamos National Laboratory
- OSTI ID:
- 6673970
- Journal Information:
- J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 89:A4; ISSN JGREA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Effects of oblique double layers on upgoing ion pitch angle and gyrophase
Center of excellence in theoretical geoplasma research. Final report, 1 October 1986-30 September 1989
Generation of ion-conic distribution by upgoing ionospheric electrons
Journal Article
·
Tue May 01 00:00:00 EDT 1984
· J. Geophys. Res.; (United States)
·
OSTI ID:6662612
Center of excellence in theoretical geoplasma research. Final report, 1 October 1986-30 September 1989
Technical Report
·
Thu Nov 09 23:00:00 EST 1989
·
OSTI ID:7253439
Generation of ion-conic distribution by upgoing ionospheric electrons
Journal Article
·
Tue Sep 01 00:00:00 EDT 1981
· J. Geophys. Res.; (United States)
·
OSTI ID:5801938
Related Subjects
640201* -- Atmospheric Physics-- Auroral
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
AURORAE
CHARGED PARTICLES
EARTH ATMOSPHERE
ELECTRIC FIELDS
ELECTRIC POTENTIAL
HEAVY IONS
IONOSPHERE
IONS
LAYERS
NUMERICAL SOLUTION
PLANETARY IONOSPHERES
PLASMA ACCELERATION
PLASMA SIMULATION
SIMULATION
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
AURORAE
CHARGED PARTICLES
EARTH ATMOSPHERE
ELECTRIC FIELDS
ELECTRIC POTENTIAL
HEAVY IONS
IONOSPHERE
IONS
LAYERS
NUMERICAL SOLUTION
PLANETARY IONOSPHERES
PLASMA ACCELERATION
PLASMA SIMULATION
SIMULATION