Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data
To investigate the physical mechanism responsible for substorm triggering, we performed a superposed-epoch analysis using plasma and magnetic-field data from THEMIS probes. Substorm onset timing was determined based on auroral breakups detected by all-sky imagers at the THEMIS ground-based obser...
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doaj-e266f0da163741e5a07aaf96d50f48652020-11-25T00:59:43ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762014-02-01329911110.5194/angeo-32-99-2014Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS dataS. Machida0Y. Miyashita1A. Ieda2M. Nosé3V. Angelopoulos4J. P. McFadden5Solar Terrestrial Environment Laboratory, Nagoya University, Aichi, JapanSolar Terrestrial Environment Laboratory, Nagoya University, Aichi, JapanSolar Terrestrial Environment Laboratory, Nagoya University, Aichi, JapanWorld Data Center for Geomagnetism, Kyoto University, Kyoto, JapanInstitute of Geophysics and Planetary Physics/Department of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USASpace Sciences Laboratory, University of California, Berkeley, CA, USATo investigate the physical mechanism responsible for substorm triggering, we performed a superposed-epoch analysis using plasma and magnetic-field data from THEMIS probes. Substorm onset timing was determined based on auroral breakups detected by all-sky imagers at the THEMIS ground-based observatories. We found earthward flows associated with north–south auroral streamers during the substorm growth phase. At around <i>X</i> = −12 Earth radii (<i>R</i><sub>E</sub>), the northward magnetic field and its elevation angle decreased markedly approximately 4 min before substorm onset. Moreover, a northward magnetic-field increase associated with pre-onset earthward flows was found at around <i>X</i> = −17 <i>R</i><sub>E</sub>. This variation indicates that local dipolarization occurs. Interestingly, in the region earthwards of <i>X</i> = −18 <i>R</i><sub>E</sub>, earthward flows in the central plasma sheet (CPS) reduced significantly approximately 3 min before substorm onset, which was followed by a weakening of dawn-/duskward plasma-sheet boundary-layer flows (subject to a 1 min time lag). Subsequently, approximately 1 min before substorm onset, earthward flows in the CPS were enhanced again and at the onset, tailward flows started at around <i>X</i> = −20 <i>R</i><sub>E</sub>. Following substorm onset, an increase in the northward magnetic field caused by dipolarization was found in the near-Earth region. Synthesizing these results, we confirm our previous results based on GEOTAIL data, which implied that significant variations start earlier than both current disruption and magnetic reconnection, at approximately 4 min before substorm onset roughly halfway between the two regions of interest; i.e. in the catapult current sheet.https://www.ann-geophys.net/32/99/2014/angeo-32-99-2014.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
S. Machida Y. Miyashita A. Ieda M. Nosé V. Angelopoulos J. P. McFadden |
spellingShingle |
S. Machida Y. Miyashita A. Ieda M. Nosé V. Angelopoulos J. P. McFadden Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data Annales Geophysicae |
author_facet |
S. Machida Y. Miyashita A. Ieda M. Nosé V. Angelopoulos J. P. McFadden |
author_sort |
S. Machida |
title |
Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data |
title_short |
Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data |
title_full |
Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data |
title_fullStr |
Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data |
title_full_unstemmed |
Statistical visualization of the Earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of THEMIS data |
title_sort |
statistical visualization of the earth's magnetotail and the implied mechanism of substorm triggering based on superposed-epoch analysis of themis data |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2014-02-01 |
description |
To investigate the physical mechanism responsible for
substorm triggering, we performed a superposed-epoch analysis using plasma
and magnetic-field data from THEMIS probes. Substorm onset timing was
determined based on auroral breakups detected by all-sky imagers at the
THEMIS ground-based observatories. We found earthward flows associated with
north–south auroral streamers during the substorm growth phase. At around
<i>X</i> = −12 Earth radii (<i>R</i><sub>E</sub>), the northward magnetic field and its
elevation angle decreased markedly approximately 4 min before substorm
onset. Moreover, a northward magnetic-field increase associated with
pre-onset earthward flows was found at around <i>X</i> = −17 <i>R</i><sub>E</sub>. This
variation indicates that local dipolarization occurs. Interestingly, in the
region earthwards of <i>X</i> = −18 <i>R</i><sub>E</sub>, earthward flows in the central plasma
sheet (CPS) reduced significantly approximately 3 min before substorm onset,
which was followed by a weakening of dawn-/duskward plasma-sheet
boundary-layer flows (subject to a 1 min time lag). Subsequently,
approximately 1 min before substorm onset, earthward flows in the CPS were
enhanced again and at the onset, tailward flows started at around <i>X</i> = −20
<i>R</i><sub>E</sub>. Following substorm onset, an increase in the northward magnetic
field caused by dipolarization was found in the near-Earth region.
Synthesizing these results, we confirm our previous results based on GEOTAIL
data, which implied that significant variations start earlier than both
current disruption and magnetic reconnection, at approximately 4 min before
substorm onset roughly halfway between the two regions of interest; i.e. in
the catapult current sheet. |
url |
https://www.ann-geophys.net/32/99/2014/angeo-32-99-2014.pdf |
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