Abstract The quasitrapping region (QTR) at the night side of a disturbed magnetosphere in the majority of models is either absent completely or merges with the plasma sheet of the magnetosphere tail. At the same time these two regions are different both in the topology of the magnetic field and in the character of motion of charged particles. Moreover, it is the region of quasitrapping that is conjugate to the zone of auroral active forms; i.e., it can be called the auroral magnetosphere. Models of the magnetosphere in which the tail structures of the magnetic field are directly adjacent to the boundary of stable trapping (in particular, the “isotropic boundary” model) are based on erroneous assumptions. Our understanding of the processes of magnetosphere substorms and magnetic storms depends on a correct understanding of the magnetosphere structure.
Structure of the Disturbed Magnetosphere
Cosmic Research ; 42 , 5
2004
Article (Journal)
English
BKL: | 55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung | |
Local classification TIB: | 770/3520/8000 |
Structure of the Disturbed Magnetosphere
Springer Verlag | 2004
|Tail current sheet dynamics in the disturbed magnetosphere
Elsevier | 1993
|Cusp confinement zones on quiet and disturbed dayside magnetosphere
British Library Conference Proceedings | 2006
|Study of wave-particle interaction in the disturbed magnetosphere
Online Contents | 2005
|Cusp confinement zones on quiet and disturbed dayside magnetosphere
Elsevier | 2005
|