A HYDROMAGNETIC THEORY OF GEOMAGNETIC STORMS AND AURORAS
A theory of geomagnetic storms, auroras and associated effects is further developed. It depends on motions in the Earth's exosphere or magnetosphere initiated by a combination of pressure and frictional drag of the solar wind and modified and extended by electric fields and currents in the ionosphere. Motion may be non-divergent, streamline flow opposed only by Lorentz forces in the ionosphere and not propagating to Earth, or divergent, non- streamline motion opposed by Lorentz forces in the Earth. The two types of motion are coupled in the E region where the former is identified with free flow of Hall current and the generation of non-streamline motion. The latter is identified with blockage of Hall current, the creation of a polarization field, and hence the generation of streamline motion. A theory of all components of a geomagnetic storm is given in terms of combination of these motions, and their distant, ionospheric and earth currents. This includes a new theory of the preliminary reverse part of the DS field and the transition from the sudden commencement to the main phase of the DS field. It is expected to introduce briefly a theory of auroras based mainly on ionospheric drifts caused by the magnetospheric motions. (auth)
- Research Organization:
- Commonwealth Scientific and Industrial Research Organization, Sydney
- NSA Number:
- NSA-17-012473
- OSTI ID:
- 4706492
- Journal Information:
- Planetary Space Sci., Journal Name: Planetary Space Sci. Vol. Vol: 9
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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