A comparison of the probability distribution of observed substorm magnitude with that predicted by a minimal substorm model
A multispacecraft analysis of a small-scale transient entrained by solar wind streams
- Rouillard, A. P., Savani, N. P., Simunac, K. D. C., Luhmann, J. G., Galvin, A. B., Crothers, S. R., Davis, C. J., Harrison, R. A., Lockwood, M., Eyles, C. J., Bewsher, D., Brown, D. S., Davies, J. A., Lavraud, B., Forsyth, R. J., Morley, S. K., Opitz, A., Sheeley, N. R., Burlaga, L. F., Sauvaud, J-A.
A numerical model of the ionospheric signatures of time-varying magnetic reconnection: III. Quasi-instantaneous convection responses in the Cowley-Lockwood paradigm
Modeling the observed proton aurora and ionospheric convection responses to changes in the IMF clock angle: 1. persistance of cusp proton aurora
On the triggering of auroral substorms by northward turnings of the interplanetary magnetic field
Are you sure you would like to clear your session, including search history and login status?