"Magnetic Field Rotation Through the Magnetopause: ISEE 1 and 2 Observations:"

J. Berchem and C. T. Russell, J. Geophys. Res., 87, 8139-8148, 1982.

This is a brief summary of "Magnetic Field Rotation Through the Magnetopause: ISEE 1 and 2 Observations:" by J. Berchem and C. T. Russell. This paper was one of the references in C. T. Russell's "The Structure of the Magnetopause," which I am attempting to summarize.

Summary

The variability of the magnetopause prevents an immediate analysis of the polarization (magnetic field angle) of the magnetopause. The sense of the rotation through magnetopause crossings by the ISEE satellites can be compared with theoretical predictions for rotational discontinuities. However, most of the crossings (about 61%) did not exhibit a structure which had the coherence to be compared and analyzed, and very few (a few percent) of the crossings which did provide clear data actually agreed with the Lee and Kan[1982] model for a rotational discontinuity.

Very few (so few that statistically it could be a coincidence) of the crossings observed rotations which would confirm the electron whistler polarization given by the first-order orbit theory of rotational discontinuities. The authors conclude that the rotation of the magnetic field depends more on the relative polarizations of the magnetosheath and magnetospheric field than on the prescribed jump conditions.

Although the theory probably was too simplified for this analysis, it illustrates the effect of undertaking analysis with the intent of proving something. Berchem and Russell selected the events based on magnetic field signatures, and not on jump conditions, which may have affected the outcome of their results. Had they chosen to analyze the events which appeared to be likely candidates for rotational discontinuities, they probably would have had more evidence supporting the theory. "Evidence for Magnetic Field Reconnection at the Earth's Magnetopause" by Sonnerup et al., [1981] uses correlated data sets and provides more evidence for rotational discontinuities.

Return to "The Structure of the Magnetosphere" by C. T. Russell.