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| Titel |
Demeter high resolution observations of the ionospheric thermal plasma response to magnetospheric energy input during the magnetic storm of November 2004 |
| VerfasserIn |
E. Seran, H. U. Frey, M. Fillingim, J.-J. Berthelier, R. Pottelette, G. Parks |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 25, no. 12 ; Nr. 25, no. 12 (2008-01-02), S.2503-2511 |
| Datensatznummer |
250015957
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| Publikation (Nr.) |
 copernicus.org/angeo-25-2503-2007.pdf |
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| Zusammenfassung |
High resolution Demeter plasma and wave observations were
available during one of the geomagnetic storms of November 2004 when the
ionospheric footprint of the plasmasphere was pushed below 64 degrees in the
midnight sector. We report here onboard observations of thermal/suprathermal
plasma and HF electric field variations with a temporal resolution of 0.4 s,
which corresponds to a spatial resolution of 3 km. Local perturbations of
the plasma parameters at the altitude of 730 km are analysed with respect to
the variation of the field-aligned currents, electron and proton
precipitation and large-scale electric fields, measured in-situ by Demeter
and by remote optical methods from the IMAGE/Polar satellites.
Flow monitoring in the 21:00 and 24:00 MLT sectors during storm conditions reveals
two distinct regions of O+ outflow, i.e. the region of the
field-aligned currents, which often comprises few layers of opposite
currents, and the region of velocity reversal toward dusk at sub-auroral
latitudes. Average upward O+ velocities are identical in both local
time sectors and vary between 200 and 450 m s−1, with an exception of a
few cases of higher speed (~1000 m s−1) outflow, observed in the
midnight sector. Each individual outflow event does not indicate any
heating process of the thermal O+ population. On the contrary, the
temperature of the O+, outflowing from auroral latitudes, is found to
be even colder than that of the ambient ion plasma. The only ion population
which is observed to be involved in the heating is the O+ with energies
a few times higher than the thermal energy. Such a population was detected at
sub-auroral latitudes in the region of duskward flow reversal. Its
temperature raises up to a few eV inside the layer of sheared velocity.
A deep decrease in the H+ density at heights and latitudes, where,
according to the IRI model, these ions are expected to comprise ~50% of the positive charge, indicates that the thermospheric balance
between atomic oxygen and hydrogen was re-established in favour of oxygen.
As a consequence, the charge exchange between oxygen and hydrogen does not
effectively limit the O+ production in the regions of the electron
precipitation. According to Demeter observations, the O+ concentration
is doubled inside the layers with upward currents (downward electrons). Such
a density excess creates the pressure gradient which drives the plasma away
from the overdense regions, i.e. first, from the layers of precipitating
electrons and then upward along the layers of downward current.
In addition, the downward currents are identified to be the source regions
of hiss emissions, i.e. electron acoustic mode excited via the Landau
resonance in the multi-component electron plasma. Such instabilities, which
are often observed in the auroral region at 2–5 Earth radii, but rarely at
ionospheric altitudes, are believed to be generated by an electron beam
which moves through the background plasma with a velocity higher than its
thermal velocity. |
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