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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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 |
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Directory of Open Access Journals: DOAJ Articles |
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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 |
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Annales Geophysicae |
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21 |
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4 |
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947 |
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953 |
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