The characteristics of the magnetopause reconnection X-line deduced from low-altitude satellite observations of cusp ions
Journal Article
·
· Geophysical Research Letters
- Rutherford Appleton Lab., Oxon (United Kingdom)
- Univ. of New Hampshire, Durham, NH (United States)
- Goddard Space Flight Center, Greenbelt, MD (United States)
- Phillips Lab., Bedford, MA (United States)
The authors present an analysis of a {open_quotes}quasi-steady{close_quotes} cusp ion dispersion signature observed at low altitudes. They 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 they find the field-parallel magnetosheath flow at the X-line was only 20 {+-} 60 km s{sup {minus}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, they derive a wealth of information about the X-line, including: the density, flow, magnetic field and Alfven 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. The authors 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. 11 refs., 5 figs., 1 tab.
- OSTI ID:
- 86414
- Journal Information:
- Geophysical Research Letters, Journal Name: Geophysical Research Letters Journal Issue: 24 Vol. 21; ISSN GPRLAJ; ISSN 0094-8276
- Country of Publication:
- United States
- Language:
- English
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