Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics

We present a statistical study of four years of Cluster crossings of the mid-altitude cusp. In this first part of the study, we start by introducing the method we have used a) to define the cusp properties, b) to sort the interplanetary magnetic field (IMF) conditions or behaviors into classes,...

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Main Authors: F. Pitout, C. P. Escoubet, B. Klecker, H. Rème
Format: Article
Language:English
Published: Copernicus Publications 2006-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/24/3011/2006/angeo-24-3011-2006.pdf
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author F. Pitout
C. P. Escoubet
B. Klecker
H. Rème
author_facet F. Pitout
C. P. Escoubet
B. Klecker
H. Rème
author_sort F. Pitout
collection DOAJ
description We present a statistical study of four years of Cluster crossings of the mid-altitude cusp. In this first part of the study, we start by introducing the method we have used a) to define the cusp properties, b) to sort the interplanetary magnetic field (IMF) conditions or behaviors into classes, c) to determine the proper time delay between the solar wind monitors and Cluster. Out of the 920 passes that we have analyzed, only 261 fulfill our criteria and are considered as cusp crossings. We look at the size, location and dynamics of the mid-altitude cusp under various IMF orientations and solar wind conditions. For southward IMF, <i>B<sub>z</sub></i> rules the latitudinal dynamics, whereas <i>B<sub>y</sub></i> governs the zonal dynamics, confirming previous works. We show that when |<i>B<sub>y</sub></i>| is larger than |<i>B<sub>z</sub></i>|, the cusp widens and its location decorrelates from <i>B<sub>y</sub></i>. We interpret this feature in terms of component reconnection occurring under <i>B<sub>y</sub></i>-dominated IMF. For northward IMF, we demonstrate that the location of the cusp depends primarily upon the solar wind dynamic pressure and upon the Y-component of the IMF. Also, the multipoint capability of Cluster allows us to conclude that the cusp needs typically more than ~20 min to fully adjust its location and size in response to changes in external conditions, and its speed is correlated to variations in the amplitude of IMF-<i>B<sub>z</sub></i>. Indeed, the velocity in &deg;ILAT/min of the cusp appears to be proportional to the variation in <i>B<sub>z</sub></i> in nT: V<sub>cusp</sub>=0.024 &Delta;<i>B<sub>z</sub></i>. Finally, we observe differences in the behavior of the cusp in the two hemispheres. Those differences suggest that the cusp moves and widens more freely in the summer hemisphere.
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spelling doaj.art-a04229198fdb4d7181121c14935536812022-12-22T01:14:21ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762006-11-01243011302610.5194/angeo-24-3011-2006Cluster survey of the mid-altitude cusp: 1. size, location, and dynamicsF. Pitout0C. P. Escoubet1B. Klecker2H. Rème3Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85741 Garching, GermanyEuropean Space Agency, Keplerlaan 1, 2201 AZ, Noordwijk, The NetherlandsMax-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85741 Garching, GermanyCentre d'étude Spatiale des Rayonnements, 9, avenue du Colonel Roche, BP 4346, 31028 Toulouse Cedex 4, FranceWe present a statistical study of four years of Cluster crossings of the mid-altitude cusp. In this first part of the study, we start by introducing the method we have used a) to define the cusp properties, b) to sort the interplanetary magnetic field (IMF) conditions or behaviors into classes, c) to determine the proper time delay between the solar wind monitors and Cluster. Out of the 920 passes that we have analyzed, only 261 fulfill our criteria and are considered as cusp crossings. We look at the size, location and dynamics of the mid-altitude cusp under various IMF orientations and solar wind conditions. For southward IMF, <i>B<sub>z</sub></i> rules the latitudinal dynamics, whereas <i>B<sub>y</sub></i> governs the zonal dynamics, confirming previous works. We show that when |<i>B<sub>y</sub></i>| is larger than |<i>B<sub>z</sub></i>|, the cusp widens and its location decorrelates from <i>B<sub>y</sub></i>. We interpret this feature in terms of component reconnection occurring under <i>B<sub>y</sub></i>-dominated IMF. For northward IMF, we demonstrate that the location of the cusp depends primarily upon the solar wind dynamic pressure and upon the Y-component of the IMF. Also, the multipoint capability of Cluster allows us to conclude that the cusp needs typically more than ~20 min to fully adjust its location and size in response to changes in external conditions, and its speed is correlated to variations in the amplitude of IMF-<i>B<sub>z</sub></i>. Indeed, the velocity in &deg;ILAT/min of the cusp appears to be proportional to the variation in <i>B<sub>z</sub></i> in nT: V<sub>cusp</sub>=0.024 &Delta;<i>B<sub>z</sub></i>. Finally, we observe differences in the behavior of the cusp in the two hemispheres. Those differences suggest that the cusp moves and widens more freely in the summer hemisphere.https://www.ann-geophys.net/24/3011/2006/angeo-24-3011-2006.pdf
spellingShingle F. Pitout
C. P. Escoubet
B. Klecker
H. Rème
Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
Annales Geophysicae
title Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
title_full Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
title_fullStr Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
title_full_unstemmed Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
title_short Cluster survey of the mid-altitude cusp: 1. size, location, and dynamics
title_sort cluster survey of the mid altitude cusp 1 size location and dynamics
url https://www.ann-geophys.net/24/3011/2006/angeo-24-3011-2006.pdf
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AT hreme clustersurveyofthemidaltitudecusp1sizelocationanddynamics