The dependence of cusp ion signatures on the reconnection rate

The interpretation of structure in cusp ion dispersions is important for helping to understand the temporal and spatial structure of magnetopause reconnection. "Stepped" and "sawtooth" signatures have been shown to be caused by temporal variations in the reconnection rate under t...

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Published in:Annales Geophysicae
Main Authors: S. K. Morley, M. Lockwood
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2003
Subjects:
Q
Online Access:https://doi.org/10.5194/angeo-21-947-2003
https://doaj.org/article/0f64072c38244effbccb1b00f35ba06c
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spelling ftdoajarticles:oai:doaj.org/article:0f64072c38244effbccb1b00f35ba06c 2023-05-15T17:08:31+02:00 The dependence of cusp ion signatures on the reconnection rate S. K. Morley M. Lockwood 2003-04-01T00:00:00Z https://doi.org/10.5194/angeo-21-947-2003 https://doaj.org/article/0f64072c38244effbccb1b00f35ba06c EN eng Copernicus Publications https://www.ann-geophys.net/21/947/2003/angeo-21-947-2003.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-21-947-2003 0992-7689 1432-0576 https://doaj.org/article/0f64072c38244effbccb1b00f35ba06c Annales Geophysicae, Vol 21, Pp 947-953 (2003) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 2003 ftdoajarticles https://doi.org/10.5194/angeo-21-947-2003 2022-12-30T22:31:47Z The interpretation of structure in cusp ion dispersions is important for helping to understand the temporal and spatial structure of magnetopause reconnection. "Stepped" and "sawtooth" signatures have been shown to be caused by temporal variations in the reconnection rate under the same physical conditions for different satellite trajectories. The present paper shows that even for a single satellite path, a change in the amplitude of any reconnection pulses can alter the observed signature and even turn sawtooth into stepped forms and vice versa. On 20 August 1998, the Defense Meteorological Satellite Program (DMSP) craft F-14 crossed the cusp just to the south of Longyearbyen, returning on the following orbit. The two passes by the DMSP F-14 satellites have very similar trajectories and the open-closed field line boundary (OCB) crossings, as estimated from the SSJ/4 precipitating particle data and Polar UVI images, imply a similarly-shaped polar cap, yet the cusp ion dispersion signatures differ substantially. The cusp crossing at 08:54 UT displays a stepped ion dispersion previously considered to be typical of a meridional pass, whereas the crossing at 10:38 UT is a sawtooth form ion dispersion, previously considered typical of a satellite travelling longitudinally with respect to the OCB. It is shown that this change in dispersed ion signature is likely to be due to a change in the amplitude of the pulses in the reconnection rate, causing the stepped signature. Modelling of the low-energy ion cutoff under different conditions has reproduced the forms of signature observed. Key words. Ionosphere (particle precipitation) Magnetospheric physics (energetic particles, precipitating, magnetopause, cusp and boundary layers) Article in Journal/Newspaper Longyearbyen Directory of Open Access Journals: DOAJ Articles Longyearbyen Annales Geophysicae 21 4 947 953
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
spellingShingle Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
S. K. Morley
M. Lockwood
The dependence of cusp ion signatures on the reconnection rate
topic_facet Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
description The interpretation of structure in cusp ion dispersions is important for helping to understand the temporal and spatial structure of magnetopause reconnection. "Stepped" and "sawtooth" signatures have been shown to be caused by temporal variations in the reconnection rate under the same physical conditions for different satellite trajectories. The present paper shows that even for a single satellite path, a change in the amplitude of any reconnection pulses can alter the observed signature and even turn sawtooth into stepped forms and vice versa. On 20 August 1998, the Defense Meteorological Satellite Program (DMSP) craft F-14 crossed the cusp just to the south of Longyearbyen, returning on the following orbit. The two passes by the DMSP F-14 satellites have very similar trajectories and the open-closed field line boundary (OCB) crossings, as estimated from the SSJ/4 precipitating particle data and Polar UVI images, imply a similarly-shaped polar cap, yet the cusp ion dispersion signatures differ substantially. The cusp crossing at 08:54 UT displays a stepped ion dispersion previously considered to be typical of a meridional pass, whereas the crossing at 10:38 UT is a sawtooth form ion dispersion, previously considered typical of a satellite travelling longitudinally with respect to the OCB. It is shown that this change in dispersed ion signature is likely to be due to a change in the amplitude of the pulses in the reconnection rate, causing the stepped signature. Modelling of the low-energy ion cutoff under different conditions has reproduced the forms of signature observed. Key words. Ionosphere (particle precipitation) Magnetospheric physics (energetic particles, precipitating, magnetopause, cusp and boundary layers)
format Article in Journal/Newspaper
author S. K. Morley
M. Lockwood
author_facet S. K. Morley
M. Lockwood
author_sort S. K. Morley
title The dependence of cusp ion signatures on the reconnection rate
title_short The dependence of cusp ion signatures on the reconnection rate
title_full The dependence of cusp ion signatures on the reconnection rate
title_fullStr The dependence of cusp ion signatures on the reconnection rate
title_full_unstemmed The dependence of cusp ion signatures on the reconnection rate
title_sort dependence of cusp ion signatures on the reconnection rate
publisher Copernicus Publications
publishDate 2003
url https://doi.org/10.5194/angeo-21-947-2003
https://doaj.org/article/0f64072c38244effbccb1b00f35ba06c
geographic Longyearbyen
geographic_facet Longyearbyen
genre Longyearbyen
genre_facet Longyearbyen
op_source Annales Geophysicae, Vol 21, Pp 947-953 (2003)
op_relation https://www.ann-geophys.net/21/947/2003/angeo-21-947-2003.pdf
https://doaj.org/toc/0992-7689
https://doaj.org/toc/1432-0576
doi:10.5194/angeo-21-947-2003
0992-7689
1432-0576
https://doaj.org/article/0f64072c38244effbccb1b00f35ba06c
op_doi https://doi.org/10.5194/angeo-21-947-2003
container_title Annales Geophysicae
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