Abstract
IT is well known that the maximum in the lunar tide variation of f0F2 occurs at about 10 lunar hours at moderate geomagnetic latitudes and at about 04 lunar hours near the geomagnetic equator1,2. Recent analyses of the lunar variations at Singapore, Ibadan and Bombay have indicated non-agreement in the phases of the variation at stations having the same geomagnetic latitudes.
Similar content being viewed by others
References
McNish, A. G., and Gautier, T. N., J. Geophys. Res., 54, 303 (1949).
Kotadia, K. M., and Ramanathan, K., Proc. Ind. Acad. Sci., 63, 394 (1956).
Osborne, B. W., Nature, 169, 661 (1952).
Brown, R. A., J. Atmos. Terr. Phys., 9, 144 (1956).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
RASTOGI, R. Lunar Tide in the F2 Layer of the Ionosphere near the Geomagnetic Equator. Nature 189, 214–215 (1961). https://doi.org/10.1038/189214a0
Issue Date:
DOI: https://doi.org/10.1038/189214a0
- Springer Nature Limited
This article is cited by
-
Seasonal variation of the lunar tidal effects in the F2 layer of the ionosphere over Indian stations
Proceedings of the Indian Academy of Sciences - Section A (1963)
-
Some effects of geomagnetic activity on the F2 region of the ionosphere over leopoldville (4·4°S, 15·3°E)
Proceedings of the Indian Academy of Sciences - Section A (1961)