Polar and Cluster observations of a dayside inverted-V during conjunction
We investigate particle and fields data during a conjunction of the Polar and Cluster spacecraft. This conjunction occurs near the dayside cusp boundary layer when a dayside inverted-V was observed in the particle data of both satellites. Electron, ion, electric field, and magnetic field data fr...
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doaj-bc9c2b16fa954ef0a046fdb126b8d0492020-11-24T23:14:48ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762007-03-012554355510.5194/angeo-25-543-2007Polar and Cluster observations of a dayside inverted-V during conjunctionJ. D. Menietti0R. A. Frahm1A. Korth2F. S. Mozer3Y. Khotyaintsev4University of Iowa, Department of Physics and Astronomy, Iowa City, IA, USASouthwest Research Institute, 6220 Culebra Road, San Antonio, TX, USAMax-Planck-Institut fur Sonnensystemforschung, Katlenburg-Lindau, GermanySpace Science Lab, University of California, Berlekey, CA, USAInstitutet fur rymdfysik (IRFU), Uppsala, SwedenWe investigate particle and fields data during a conjunction of the Polar and Cluster spacecraft. This conjunction occurs near the dayside cusp boundary layer when a dayside inverted-V was observed in the particle data of both satellites. Electron, ion, electric field, and magnetic field data from each satellite confirm that the dayside inverted-V (DSIV) structure is present at the location of both satellites and the electric fields persist from the altitude of the Polar (lower) spacecraft to the altitude of the Cluster spacecraft. We observe accelerated, precipitating electrons and upward ions along the magnetic field. In addition, large amplitude electric fields perpendicular to the ambient magnetic field seen by Polar and by Cluster suggest significant parallel electric fields associated with these events. For similar DSIV events observed by the Polar spacecraft, plasma waves (identified as possible Alfvén waves) have been observed to propagate in both directions along the magnetic field line. Future conjunctions will be necessary to confirm that DSIVs are associated with reconnection sites.https://www.ann-geophys.net/25/543/2007/angeo-25-543-2007.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
J. D. Menietti R. A. Frahm A. Korth F. S. Mozer Y. Khotyaintsev |
spellingShingle |
J. D. Menietti R. A. Frahm A. Korth F. S. Mozer Y. Khotyaintsev Polar and Cluster observations of a dayside inverted-V during conjunction Annales Geophysicae |
author_facet |
J. D. Menietti R. A. Frahm A. Korth F. S. Mozer Y. Khotyaintsev |
author_sort |
J. D. Menietti |
title |
Polar and Cluster observations of a dayside inverted-V during conjunction |
title_short |
Polar and Cluster observations of a dayside inverted-V during conjunction |
title_full |
Polar and Cluster observations of a dayside inverted-V during conjunction |
title_fullStr |
Polar and Cluster observations of a dayside inverted-V during conjunction |
title_full_unstemmed |
Polar and Cluster observations of a dayside inverted-V during conjunction |
title_sort |
polar and cluster observations of a dayside inverted-v during conjunction |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2007-03-01 |
description |
We investigate particle and fields data during a conjunction of the Polar
and Cluster spacecraft. This conjunction occurs near the dayside cusp
boundary layer when a dayside inverted-V was observed in the particle data
of both satellites. Electron, ion, electric field, and magnetic field data
from each satellite confirm that the dayside inverted-V (DSIV) structure is
present at the location of both satellites and the electric fields persist
from the altitude of the Polar (lower) spacecraft to the altitude of the
Cluster spacecraft. We observe accelerated, precipitating electrons and
upward ions along the magnetic field. In addition, large amplitude electric
fields perpendicular to the ambient magnetic field seen by Polar and by
Cluster suggest significant parallel electric fields associated with these
events. For similar DSIV events observed by the Polar spacecraft, plasma
waves (identified as possible Alfvén waves) have been observed to
propagate in both directions along the magnetic field line. Future
conjunctions will be necessary to confirm that DSIVs are associated with
reconnection sites. |
url |
https://www.ann-geophys.net/25/543/2007/angeo-25-543-2007.pdf |
work_keys_str_mv |
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