On the structure of the interplanetary magnetic field under non-stationary boundary conditions.

Details On the structure of the interplanetary magnetic field under non-stationary boundary conditions. On the structure of the interplanetary magnetic field under non-stationary boundary conditions.

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stgg...32..362t&link_type=abstract

Stud. Geophys. Geod., Vol. 32, No. 4, p. 362 - 367

Physics

1

Interplanetary Magnetic Field: Solar Wind, Interplanetary Magnetic Field: Structure

Scientific paper

The IMF is investigated theoretically in a kinematic approximation under frozen-in conditions in the solar wind and non-stationary boundary conditions. as an example, a time-dependent model of the IMF, created in the case of a change of the general magnetic field of the Sun represented by the dipole term, is analyzed. The results show the formation of zero IMF points of two types (O, X). Points of the O-type are formed and move radially in the equatorial plane. They are surrounded by magnetic clouds with loops of lines of force. Points of the X-type are formed and move radially above the poles.

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