An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics

We present an analysis of the accuracy of the method introduced by Lockwood <i>et al</i>. (1994) for the determination of the magnetopause reconnection rate from the dispersion of precipitating ions in the ionospheric cusp region. Tests are made by applying the method to synthesised...

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Main Authors: M. Lockwood, C. J. Davis
Format: Article
Language:English
Published: Copernicus Publications 1996-02-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/14/149/1996/angeo-14-149-1996.pdf
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spelling doaj-1bdce9291fbf40a395871dc0a4ab09ad2020-11-24T23:55:13ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05761996-02-011414916110.1007/s00585-996-0149-9An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristicsM. LockwoodC. J. DavisWe present an analysis of the accuracy of the method introduced by Lockwood <i>et al</i>. (1994) for the determination of the magnetopause reconnection rate from the dispersion of precipitating ions in the ionospheric cusp region. Tests are made by applying the method to synthesised data. The simulated cusp ion precipitation data are produced by an analytic model of the evolution of newly-opened field lines, along which magnetosheath ions are firstly injected across the magnetopause and then dispersed as they propagate into the ionosphere. The rate at which these newly opened field lines are generated by reconnection can be varied. The derived reconnection rate estimates are then compared with the input variation to the model and the accuracy of the method assessed. Results are presented for steady-state reconnection, for continuous reconnection showing a sine-wave variation in rate and for reconnection which only occurs in square wave pulses. It is found that the method always yields the total flux reconnected (per unit length of the open-closed field-line boundary) to within an accuracy of better than 5%, but that pulses tend to be smoothed so that the peak reconnection rate within the pulse is underestimated and the pulse length is overestimated. This smoothing is reduced if the separation between energy channels of the instrument is reduced; however this also acts to increase the experimental uncertainty in the estimates, an effect which can be countered by improving the time resolution of the observations. The limited time resolution of the data is shown to set a minimum reconnection rate below which the method gives spurious short-period oscillations about the true value. Various examples of reconnection rate variations derived from cusp observations are discussed in the light of this analysis.https://www.ann-geophys.net/14/149/1996/angeo-14-149-1996.pdf
collection DOAJ
language English
format Article
sources DOAJ
author M. Lockwood
C. J. Davis
spellingShingle M. Lockwood
C. J. Davis
An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
Annales Geophysicae
author_facet M. Lockwood
C. J. Davis
author_sort M. Lockwood
title An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
title_short An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
title_full An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
title_fullStr An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
title_full_unstemmed An analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
title_sort analysis of the accuracy of magnetopause reconnection rate variations deduced from cusp ion dispersion characteristics
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 1996-02-01
description We present an analysis of the accuracy of the method introduced by Lockwood <i>et al</i>. (1994) for the determination of the magnetopause reconnection rate from the dispersion of precipitating ions in the ionospheric cusp region. Tests are made by applying the method to synthesised data. The simulated cusp ion precipitation data are produced by an analytic model of the evolution of newly-opened field lines, along which magnetosheath ions are firstly injected across the magnetopause and then dispersed as they propagate into the ionosphere. The rate at which these newly opened field lines are generated by reconnection can be varied. The derived reconnection rate estimates are then compared with the input variation to the model and the accuracy of the method assessed. Results are presented for steady-state reconnection, for continuous reconnection showing a sine-wave variation in rate and for reconnection which only occurs in square wave pulses. It is found that the method always yields the total flux reconnected (per unit length of the open-closed field-line boundary) to within an accuracy of better than 5%, but that pulses tend to be smoothed so that the peak reconnection rate within the pulse is underestimated and the pulse length is overestimated. This smoothing is reduced if the separation between energy channels of the instrument is reduced; however this also acts to increase the experimental uncertainty in the estimates, an effect which can be countered by improving the time resolution of the observations. The limited time resolution of the data is shown to set a minimum reconnection rate below which the method gives spurious short-period oscillations about the true value. Various examples of reconnection rate variations derived from cusp observations are discussed in the light of this analysis.
url https://www.ann-geophys.net/14/149/1996/angeo-14-149-1996.pdf
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