Internal Structure of the Geomagnetic Neutral Sheet
Models for internal structure of geomagnetic tail neutral sheet deduced from Explorer 34 magnetic data
Engineering topics
Publications and source records attributed to Schindler, K..
Models for internal structure of geomagnetic tail neutral sheet deduced from Explorer 34 magnetic data
The rotational properties in the photospheric and solar wind plasma and magnetic fields are considered. In both the photosphere and the interplanetary medium near the earth, there is a tendency for the field patterns to rotate a few percent faster than the plasma patterns. The fields and plasmas show variability in their rotational properties on time scales of days or months, but averages over a few years tend to be less variable, as shown by the results for long-lived sunspots, and by the rotating solar magnetic dipole.
Laboratory models for solar wind and magnetosphere interactions with similarity laws of Vlasov theory as reference system