The characteristics of the magnetopause reconnection X-line deduced from low-altitude satellite observations of cusp ions

Lockwood, M. ORCID: https://orcid.org/0000-0002-7397-2172, Onsager, T. G., Davis, C. J. ORCID: https://orcid.org/0000-0001-6411-5649, Smith, M. F. and Denig, W. F. (1994) The characteristics of the magnetopause reconnection X-line deduced from low-altitude satellite observations of cusp ions. Geophysical Research Letters, 21 (24). pp. 2757-2760. ISSN 0094-8276 doi: 10.1029/94GL02696

Abstract/Summary

We present an analysis of a “quasi-steady” cusp ion dispersion signature observed at low altitudes. We reconstruct the field-parallel part of the Cowley-D ion distribution function, injected into the open LLBL in the vicinity of the reconnection X-line. From this we find the field-parallel magnetosheath flow at the X-line was only 20 ± 60 km s−1, placing the reconnection site close to the flow streamline which is perpendicular to the magnetosheath field. Using interplanetary data and assuming the subsolar magnetopause is in pressure balance, we derive a wealth of information about the X-line, including: the density, flow, magnetic field and Alfvén speed of the magnetosheath; the magnetic shear across the X-line; the de-Hoffman Teller speed with which field lines emerge from the X-line; the magnetospheric field; and the ion transmission factor across the magnetopause. The results indicate that some heating takes place near the X-line as the ions cross the magnetopause, and that sheath densities may be reduced in a plasma depletion layer. We also compute the reconnection rate. Despite its quasi-steady appearance on an ion spectrogram, this cusp is found to reveal a large pulse of enhanced reconnection rate.

Additional Information	First published online 2012
Item Type	Article
URI	https://reading-clone.eprints-hosting.org/id/eprint/38811
Identification Number/DOI	10.1029/94GL02696
Refereed	Yes
Divisions	No Reading authors. Back catalogue items Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
Additional Information	First published online 2012
Publisher	American Geophysical Union
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