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  • GEOPHYSICS  (2)
  • 1
    Publication Date: 2011-08-18
    Description: A field campaign, using three magnetometer stations spaced in latitude around the equatorial magnetic field distance L approximately 1.9, was conducted in early 1979 to investigate the polarization characteristics of hydromagnetic waves at low geomagnetic latitudes. The magnetic pulsations are observed to have periods in the range approximately 20-25 s and to occur primarily in the local morning hours. Statistically, the polarizations at all three stations were predominantly left handed in the local morning hours and right handed in the local afternoon. At the highest-latitude station (L approximately 2) the orientation of the major axis of the polarization ellipse changed from a predominantly NW-SE direction in the local morning to a mixed NW-SE/NE-SW direction in the afternoon. These two statistical results are consistent with the excitation of the waves by the Kelvin-Helmholtz instability at the magnetopause. However, frequent changes in phase are often observed in the magnetic variations, which result in polarization variations on the time scale of minutes, a situation not readily reconcilable with the Kelvin-Helmholtz instability. The existence of the waves at very low latitudes, furthermore, places constraints on the damping rate of externally excited surface waves inside the magnetosphere. We conclude that present theories for hydromagnetic waves in the geomagnetosphere cannot readily incorporate all of these low-latitude results.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 86; July 1
    Format: text
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  • 2
    Publication Date: 2019-07-12
    Description: A study of the transmission of magnetosheath hydromagnetic fluctuations with f of about 23 mHz and f of about 13 mHz through the magnetopause is reported. The study involves measurements of the fluctuations inside the magnetosphere on the ISEE-2 spacecraft near the equator and on the ground near the boundary flux tube connecting with the spacecraft. The magnetic energy of the fluctuations inside the magnetopause is about 1 percent of those in the magnetosheath. This ratio is consistent with that expected for the transmission of fast-mode waves through a magnetopause with a tangential discontinuity.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research (ISSN 0148-0227); 94; 6933-693
    Format: text
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