Geomagnetic storms forecast using IPS observations
Main Article Content
Abstract
IPS observations have shown to provide a very good track of the disturbances in the solar wind flowing out from coronal holes at the Sun and eventually hitting the Earth and causing geomagnetic and ionospheric perturbations. A continuous survey of IPS for 900 stellar radio sources, carried out from July 1978 to September 1979, showed that most of the sudden commencements of geomagnetic storms took place more than one day after the first IPS detection of the disturbance in the interplanetary medium, and some of them even four or five days later. This shows that IPS observations can also be a useful tool in the forecasting of geomagnetic perturbations and associated effects.
Article Details

This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License.
References
BORRINI, G., J. T. GOSLING, S. J. BAME and W. C. FELDMAN, 1982. An analysis of the shock wave disturbances observed at IAU from 1971 through 1978. J. Geophys. Res., 87, 4365-4373. DOI: https://doi.org/10.1029/JA087iA06p04365
CANE, H. V. and R. G. STONE, 1984. Type II solar radio burst, interplanetary shocks and energetic particle events. Astrophys. 1., 282, 339-344. DOI: https://doi.org/10.1086/162207
CANE, H. V., 1985. The evolution of interplanetary shocks. J. Geophys. Res., 90, 191-197. DOI: https://doi.org/10.1029/JA090iA01p00191
GAPPER, G. R., A. HEWISH, A. PURVIS and P. J. DUFFETT-SMITH, 1982. Observing interplanetary disturbances from the ground. Nature, 296, 633-636. DOI: https://doi.org/10.1038/296633a0
HEWISH, A., S. J. TAPPIN and G. R. GAPPER, 1985. Origin of strong interplanetary shocks. Nature, 314, 137-140. DOI: https://doi.org/10.1038/314137a0
HEWISH, A. and S. BRAVO, 1986a. The sources of large scale heliospheric disturbances. Solar Phys., 106, 185-200. DOI: https://doi.org/10.1007/BF00161362
HEWISH, A. and S. BRAVO, 1986b. Distribution of energetic particles near interplanetary shocks. Nature, 324, 44-46. DOI: https://doi.org/10.1038/324044a0
INTRILIGATOR, D. S., 1977. Pioneer 9 and Pioneer 10 observations of the solar wind associated with the August 1972 events. J. Geophys. Res., 82, 603-617. DOI: https://doi.org/10.1029/JA082i004p00603
INTRILIGATOR, D. S., 1980. Transient phenomena originating at the Sun-an interplanetary view, in solar and interplanetary dynamics, M. Dryer and E. Tandberg-Hanssen (Eds.), Reidel, Dordrecht, 357-374. DOI: https://doi.org/10.1007/978-94-009-9100-2_57
JOSELYN, J. A. and P. S. MciNTOSH, 1981. Disappearing solar filaments: a useful predictor of geomagnetic activity. J. Geophys. Res., 86, 4555-4564. DOI: https://doi.org/10.1029/JA086iA06p04555
LANZEROTTI, L. J., 1979. Solar System Plasma Physics Vol. 3, North-Holland, Amsterdam.
RUST, D. M., 1982. Solar flares, proton showers, and the space shuttle. Science, 216, 939-946. DOI: https://doi.org/10.1126/science.216.4549.939
STEINITZ, R. and M. EYNI, 1980. Global properties of the solar wind. 1. The invariance of the momentum flux density. Astrophys. J., 241, 417-424. DOI: https://doi.org/10.1086/158355
TAPPIN, S. J., A. HEWISH and G. R. GAPPER, 1983. Tracking a major interplanetary disturbance. Planet Space Sci., 31, 1171-1176. DOI: https://doi.org/10.1016/0032-0633(83)90106-X
TAPPIN, S. J., A. HEWISH and G. R. GAPPER, 1984. Tracking a high-latitude corotating stream for more than half a solar rotation. Planet. Space Sci., 32, 1273-1281. DOI: https://doi.org/10.1016/0032-0633(84)90070-9
WOLFE, J., D. S. INTRILIGATOR, J. MIHALOV, H. COLLARD, D. McKIBBIN, R. WHITTEN and A. BARNES, 1979. Initial observations of the Pioneer Venus Orbiter Solar Wind Plasma Experiment, Science, 203, 750-752. DOI: https://doi.org/10.1126/science.203.4382.750