posted on 2017-01-09, 16:15authored byJ. A. Davies, T. K. Yeoman, I. J. Rae, S. E. Milan, M. Lester, M. Lockwood, A. McWilliams
Observations from the EISCAT VHF incoherent scatter radar system in northern Norway, during a run of the common programme CP-4, reveal a series of poleward-propagating F-region electron density enhancements in the pre-noon sector on 23 November 1999. These plasma density features, which are observed under conditions of a strongly southward interplanetary magnetic field, exhibit a recurrence rate of under 10 min and appear to emanate from the vicinity of the open/closed field-line boundary from where they travel into the polar cap; this is suggestive of their being an ionospheric response to transient reconnection at the day-side magnetopause (flux transfer events). Simultaneous with the density structures detected by the VHF radar, poleward-moving radar auroral forms (PMRAFs) are observed by the Finland HF coherent scatter radar. It is thought that PM-RAFs, which are commonly observed near local noon by HF radars, are also related to flux transfer events, although the specific mechanism for the generation of the field-aligned irregularities within such features is not well understood. The HF observations suggest, that for much of their existence, the PMRAFs trace fossil signatures of transient reconnection rather than revealing the footprint of active reconnection itself; this is evidenced not least by the fact that the PMRAFs become narrower in spectral width as they evolve away from the region of more classical, broad cusp scatter in which they originate. Interpretation of the HF observations with reference to the plasma parameters diagnosed by the incoherent scatter radar suggests that as the PMRAFs migrate away from the reconnection site and across the polar cap, entrained in the ambient antisunward flow, the irregularities therein are generated by the presence of gradients in the electron density, with these gradients having been formed through structuring of the ionosphere in the cusp region in response to transient reconnection.
Funding
The authors are indebted to the director and
staff of EISCAT for operating the facility and supplying the data
and to the EISCAT group at the Rutherford Appleton Laboratory
for maintenance of the analysis software and assistance therewith.
EISCAT is an international facility funded collaboratively by
the research councils of Finland (SA), France (CNRS), the Federal
Republic of Germany (MPG), Japan (NIPR), Norway (NAVF),
Sweden (NFR) and the United Kingdom (PPARC). CUTLASS is
funded jointly by PPARC (Grant number PPA/R/R/1997/00256),
the Swedish Institute for Space Physics, Uppsala, and the Finnish
Meteorological Institute, Helsinki. The authors acknowledge the
principal investigators R. Lepping and N. Ness for enabling use of
the Wind and ACE MFI key parameter data, respectively. Thanks
are also due to the Canadian Space Agency for providing the
CANOPUS magnetometer data. J. A. Davies and S. E. Milan are
supported on PPARC grant number PPA/G/O/1999/00181. I. J. Rae
is supported by the Natural Sciences and Engineering Council of
Canada (NSERC). K. A. McWilliams is funded by the Association
of Commonwealth Universities of the British Council.
History
Citation
Annales Geophysicae, 20, 781-794, 2002
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Annales Geophysicae
Publisher
European Geosciences Union (EGU), Copernicus Publications, Springer Verlag (Germany)