A statistical study of narrow bandwidth, high-latitude geomagnetic pulsations
Thesis/Dissertation
·
OSTI ID:6901914
This study is a survey of micropulsations at three high-latitude ground stations. Results concerning the source region of Pc1/2 waves are discussed. The study revealed a diurnal occurrence pattern for waves in the 0.1-0.4 Hz band (Pc1/2), and showed that the pattern was not due to the effects of sunlight on the ionosphere, but instead from a postnoon magnetospheric source region. The importance of He+ ions in the magnetosphere to wave growth is also indicated. Based on the diurnal and seasonal occurrence patterns of the wave above and below 0.4 Hz, it is concluded that the waves observed on the ground above 0.4 Hz come primarily from plasmapause latitudes. Those below 0.4 Hz, in the Pc1/2 band, come from farther out. The different source locations for waves above and below 0.4 Hz, combined with the typically sharp, approximately 0.4 Hz upper frequency limit of Pc1/2 spectra, suggest strongly that He+ ions in the outer magnetosphere influence wavegrowth and propagation. This fits well with the observations of Anderson, et al. (1990), who showed with spacecraft study that waves above the He+ gyrofrequency are more commonly observed beyond L = 7 than in regions closer to the Earth. This ground study shows that waves above the He+ gyrofrequency from the outer magnetosphere do not readily reach the ground. The organization of ground observations by He+ has never been shown before in previous ground studies. An extensive search for correlations between Pc1/2 occurrence and solar wind pressure and magnetic field orientation rules out the solar wind as a direct source of Pc1/2 generation. They may instead be amplified by plasma sheet ions that drift sunward on the dusk side of the magnetosphere and undergo ion-cyclotron resonance in the afternoon sector. This mechanism is consistent with the diurnal pattern and apparent source location of the Pc1/2.
- Research Organization:
- New Hampshire Univ., Durham, NH (United States)
- OSTI ID:
- 6901914
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
661320* -- Auroral
Ionospheric
& Magnetospheric Phenomena-- (1992-)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHARGED PARTICLES
EARTH ATMOSPHERE
EARTH MAGNETOSPHERE
FREQUENCY RANGE
GYROFREQUENCY
HELIUM IONS
HZ RANGE
IONOSPHERE
IONS
MAGNETIC FIELDS
PLANETARY IONOSPHERES
PLASMA WAVES
PLASMAPAUSE
PULSATIONS
SEASONAL VARIATIONS
SOLAR ACTIVITY
SOLAR WIND
SPECTRA
VARIATIONS
Ionospheric
& Magnetospheric Phenomena-- (1992-)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHARGED PARTICLES
EARTH ATMOSPHERE
EARTH MAGNETOSPHERE
FREQUENCY RANGE
GYROFREQUENCY
HELIUM IONS
HZ RANGE
IONOSPHERE
IONS
MAGNETIC FIELDS
PLANETARY IONOSPHERES
PLASMA WAVES
PLASMAPAUSE
PULSATIONS
SEASONAL VARIATIONS
SOLAR ACTIVITY
SOLAR WIND
SPECTRA
VARIATIONS