Premium
Prediction of the occurrence and intensity of magnetospheric substorms
Author(s) -
Akasofu S.I.,
Chao J. K.
Publication year - 1979
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/gl006i011p00897
Subject(s) - solar wind , substorm , physics , earth radius , intensity (physics) , venus , geophysics , magnetosphere , computational physics , astrophysics , atmospheric sciences , plasma , astrobiology , optics , quantum mechanics
The solar wind and IMF data obtained by the Venus probe Mariner 5 (at a distance of 460 earth radii) and by the earthbound Explorer 34 satelliteon June 2425and 261967 were examined. It is demonstrated that the occurrence and intensity of magnetospheric substorms can be predicted about 1‐3 hours prior to their onsets by monitoring the energy coupling function at a distance of a few hundred earth radii upstream of the solar wind. It appears that the ‘ ∈ signal ’ propagates with different speedsperhaps depending on the propagation time of disturbances which increase ∈