Transpolar auroras, their particle precipitation, and IMF B sub y component
- Takushoku Univ., Tokyo (Japan)
- Johns Hopkins Univ., Laurel, MD (United States)
- Univ. of Alaska, Fairbanks (United States)
Transpolar auroras, their associated particle precipitation, and their occurrence with respect to the IMF B{sub y} polarity are examined on the basis of DMSP F6 auroral images and the corresponding particle data. It is found that the transpolar arcs are located in the poleward edge of the soft particle precipitation region extending from either the dawn or dusk part of the auroral oval precipitation; they are not embedded in the polar rain region. This finding suggests that the transpolar arcs are located along the poleward boundary of the closed field line region (or the equatorward boundary of the open region) as suggested by Meng. Further, the appearance of the extended precipitation region from the oval depends on the polarity of the IMF B{sub y}, in the northern hemisphere morning sector for IMF B{sub y} < 0 or in the evening sector for IMF B{sub y} > 0. In general, the precipitating particle flux in the extended precipitation region is not high enough to produce appreciable luminosity. Thus only the transpolar arcs (associated with relatively intense precipitation) near the poleward boundary tend to become much more luminous, forming the so-called theta aurora.
- OSTI ID:
- 5255838
- Journal Information:
- Journal of Geophysical Research; (United States), Vol. 96:A8; ISSN 0148-0227
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
GENERAL PHYSICS
POLAR-CAP AURORAE
EVALUATION
AURORAL OVAL
CHARGED-PARTICLE PRECIPITATION
CORRELATIONS
ELECTRIC CURRENTS
IMAGES
INTERPLANETARY MAGNETIC FIELDS
LUMINOSITY
MAGNETIC BAYS
SATELLITES
AURORAE
CURRENTS
MAGNETIC FIELDS
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
640201* - Atmospheric Physics- Auroral
Ionospheric
& Magetospheric Phenomena