The long-term variations of the ozone column density, observed in the Antarctic atmosphere in the period 1964-1985, are studied in connection with the trend of the geomagnetic activity. While the current view accounts for the ozone depletion entirely in terms of chemical and dynamical processes occurring in the atmosphere, we show that the present experimental evidences rely favourably on the contribution of geomagnetic phenomena such as aurorae, induced by solar related disturbances. -Authors

DE PETRIS, M., Gervasi, M., Masi, S., Olivo, B., Moreno, G., Storini, M., et al. (1990). ON THE ANTARCTIC OZONE DEPLETION DURING SOLAR-CYCLE 21. ANNALES GEOPHYSICAE, 8(7-8), 541-548.

ON THE ANTARCTIC OZONE DEPLETION DURING SOLAR-CYCLE 21

GERVASI, MASSIMO;
1990

Abstract

The long-term variations of the ozone column density, observed in the Antarctic atmosphere in the period 1964-1985, are studied in connection with the trend of the geomagnetic activity. While the current view accounts for the ozone depletion entirely in terms of chemical and dynamical processes occurring in the atmosphere, we show that the present experimental evidences rely favourably on the contribution of geomagnetic phenomena such as aurorae, induced by solar related disturbances. -Authors
No
Articolo in rivista - Articolo scientifico
Scientifica
Su-Earth relations, space weather
English
541
548
8
DE PETRIS, M., Gervasi, M., Masi, S., Olivo, B., Moreno, G., Storini, M., et al. (1990). ON THE ANTARCTIC OZONE DEPLETION DURING SOLAR-CYCLE 21. ANNALES GEOPHYSICAE, 8(7-8), 541-548.
DE PETRIS, M; Gervasi, M; Masi, S; Olivo, B; Moreno, G; Storini, M; Calisse, P
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/10281/34288
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