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Austral thermospheric wind circulation and interplanetary magnetic field orientation

Journal Article · · Journal of Geophysical Research; (United States)
DOI:https://doi.org/10.1029/90JA02458· OSTI ID:6096270
 [1];  [2];  [3]
  1. Univ. of Washington, Seattle (USA)
  2. Queen's University, Belfast (Northern Ireland)
  3. University of Alaska, Fairbanks (USA)
Ground-based high-resolution spectral measurements of the OI {sup 1}D emission at 15,867 K (630 nm; 1 K = 1 cm{sup {minus}1}) from thermospheric altitudes at the geographic south pole are used to determine the relationship between the southern hemisphere high-latitude thermospheric wind circulation and the interplanetary magnetic field (IMF) during the austral winter of 1989. A clear dependence is shown between the thermospheric wind direction and magnitude and the IMF. In the midnight sector, the zonal wind magnitude is dependent on B{sub y}, and the meridonal component on B{sub z}. The magnetic local times of the largest polar cap electric fields are also inferred for either sign of B{sub y}. In addition, it is shown that the field angle {Psi} of the IMF in the Y-Z plane is also useful for ordering the neutral wind data. These ground-based wind measurements also reflect the polarity and magnitude of the IMF, at least near the observing station's magnetic midnight.
OSTI ID:
6096270
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 96:A4; ISSN 0148-0227; ISSN JGREA
Country of Publication:
United States
Language:
English