"Interplanetary Magnetic Field and the Auroral Zones:"
This is a brief summary of "Interplanetary Magnetic Field and the Auroral
Zones" by J. W. Dungey.
This paper was one of the references in C. T. Russell's "The
Structure of the Magnetopause," which I am attempting to
summarize.
This is one of the earliest papers discussing the role of reconnection in
creating and defining magnetospheric structure and behavior. This paper
was inspired by Pioneer V's discovery that the IMF is fairly steady in
behavior, allowing several predictions to be made based on IMF direction.
Dungey concerns himself primarily with southward IMF, which results in
reconnection in the equatorial plane.
When a steady flow around the earth is assumed (Dungey admits that this
may not be a reliable approximation), the electric field found from
the cross product of the flow vector and the earth's magnetic field
exhibits equipotentials which coincide with observed current lines.
The primary auroral acceleration, in this case, would take place at
the neutral points, the current lines being the auroral field lines.
Dungey predicts proton auroras before midnight and electron
auroras after midnight, in accordance with the model's electric field
directions.
In reading papers written way before my birth, I find it difficult to
place the discussion in the proper context. Dungey states that if the
IMF was northward, the topology of the magnetosphere-solar wind system
would not allow open field lines, and hence the IMF points southward.
So when did the physical community become aware that the IMF
fluctuates in direction? I found it interesting and exciting that a single
paper could contain such a large volume of relevant and vital information,
even though he failed to notice the potential for reconnection during
northward IMF. Indeed, the theory for northward IMF reconnection was
probably worked out 6-12 months after the discovery of a steady
northward IMF.
Return to "The Structure of the Magnetosphere" by
C. T. Russell.