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Helicon modes driven by ionospheric O + ions in the plasma sheet region
Author(s) -
Lakhina Gurbax S.,
Tsurutani Bruce T.
Publication year - 1997
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/97gl01208
Subject(s) - helicon , substorm , physics , atomic physics , plasma sheet , ion , instability , plasma , ionosphere , electron , magnetosphere , geophysics , mechanics , quantum mechanics
The presence of ionospheric‐origin oxygen ions in the plasma sheet region results in only partial cancellation of the electron Hall current leading to the occurrence of the helicon mode rather than the Alfvén mode. It is shown that the presence of ionospheric‐origin oxygen ion beams with anisotropic pressure can excite helicon mode instability in the near‐Earth plasma sheet region provided their Alfvénic Mach numbers lie in a certain range. The helicon modes are easily excited under the conditions when the usual long wave‐lengths fire‐hose modes are stable. The typical real frequencies of the excited helicon modes are between 1 to 10 mHz, and the typical e‐folding time of the instability is about 3 to 15 minutes at wavelengths of 1 to 5 R E . Therefore these modes are likely to attain saturation during enhanced convection events lasting for a few hours. Large amplitude helicon modes would distort the ambient magnetic field and may be observable as flux ropes. Low‐frequency turbulence produced by these modes could scatter electrons and help excitation of the ion tearing modes leading to substorm onset.