Abstract
WHILE methods of representing the 100-mb. wind field were under investigation, diurnal and semidiurnal variations were detected in winds observed at the 100-mb. level from British upper air stations. These periodic variations of wind appear to be associated with the atmospheric solar tides. 100-mb. wind observations are particularly suitable for study in connexion with tidal oscillations, since, at least between latitudes 30° N. and 60° N., the synoptic variations of wind are considerably smaller at that level than in the upper troposphere. The lower stratosphere is also free from the smaller-scale effects which may mask tidal wind variations occurring in the lower troposphere.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Bartels, J., “Handbuch der Experimentalphysik”, 25, 163 (1928).
Simpson, G. C., Quart. J. Roy. Met. Soc., 44, 20 (1918).
Wilkes, M. V., “Oscillations of the Earth's Atmosphere” (Camb. Univ. Press, 1949).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
JOHNSON, D. Solar Tides in the Lower Stratosphere. Nature 174, 363–364 (1954). https://doi.org/10.1038/174363a0
Issue Date:
DOI: https://doi.org/10.1038/174363a0
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.