Abstract
In the period of the International Geophysical Year (IGY), almost the entire planet was covered for the first time by ground-based geophysical observations. Their analysis led to two fundamental results: the existence of the auroral oval and auroral (magnetospheric) substorm. At the final stage of the IGY, satellite explorations of the near-Earth space began. The auroral luminosity appeared to be related to the plasma structure of the magnetosphere. That opened new possibilities for parameters diagnostics of the Earth’s magnetosphere on the basis of ground-based aurora observations. The concepts of auroral oval and magnetospheric substorm became paradigms of the new science of solar-terrestrial physics.
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Dedicated to the memory of Genrikh Vladimirovich Starkov and many others who studied auroras during the IGY
Original Russian Text © Ya.I. Feldstein, V.G. Vorobjev, V.L. Zverev, 2010, published in Geomagnetizm i Aeronomiya, 2010, Vol. 50, No. 4, pp. 435–458.
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Feldstein, Y.I., Vorobjev, V.G. & Zverev, V.L. Planetary features of aurorae: Results of the IGY (a review). Geomagn. Aeron. 50, 413–435 (2010). https://doi.org/10.1134/S0016793210040018
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DOI: https://doi.org/10.1134/S0016793210040018