Abstract The present conception of substorms is now under development within the scope of two basic models. In one of them (model 1) an active substorm phase is due to instability (plasma sheet reconnection) resulting from the accumulation of solar wind energy, transported to the magnetosphere, in the form of magnetotail energy. In model 2 the active phase requires no energy accumulation. In this paper a semi-empirical model is proposed where the active substorm phase comprises two periods. The first period (convection-type disturbances) corresponds to model 2, the second one (anticonvection-type disturbances) does not contradict model 1.
Magnetic storms, substorms and microsubstorms
Advances in Space Research ; 1 , 1 ; 145-150
1981-01-01
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
CHAPTER 7 -- STORMS AND SUBSTORMS - Tail Configuration During Storms
Online Contents | 2000
|CHAPTER 7 -- STORMS AND SUBSTORMS - Development of Substorms in the Near-Earth Tail
Online Contents | 2000
|The Interplanetary Causes of Magnetic Storms, Substorms and Geomagnetic Quiet
British Library Conference Proceedings | 2001
|Effect of magnetic storms and substorms on GPS slips at high latitudes
Springer Verlag | 2016
|Effect of magnetic storms and substorms on GPS slips at high latitudes
Online Contents | 2016
|