 |
| Titel |
Spatial spreading of magnetospherically reflected chorus elements in the inner magnetosphere |
| VerfasserIn |
H. Breuillard, Y. Zaliznyak, O. Agapitov, A. Artemyev, V. Krasnoselskikh, G. Rolland |
| Medientyp |
Artikel
|
| Sprache |
Englisch
|
| ISSN |
0992-7689
|
| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 31, no. 8 ; Nr. 31, no. 8 (2013-08-26), S.1429-1435 |
| Datensatznummer |
250086095
|
| Publikation (Nr.) |
 copernicus.org/angeo-31-1429-2013.pdf |
|
|
|
|
|
| Zusammenfassung |
| Chorus-type whistler waves are known to be generated in the
vicinity of the magnetic equator, in the low-density plasma trough region.
These wave packets propagate towards the magnetic poles, deviating from the
magnetic field lines, before being eventually reflected at higher latitudes.
Magnetospheric reflection of whistler waves results in bounce oscillations of
these waves through the equator. Our study is devoted to the problem of
geometrical spreading of these whistler-mode waves after their first
magnetospheric reflection, which is crucial to determine where wave–particle
interactions occur. Recently, experimental studies stated that the relative
intensity of the reflected signal was generally between 0.005 and 0.05 of
the source signal. We model such wave packets by means of ray tracing
technique, using a warm plasma dispersion function along their trajectory and
a realistic model of the inner magnetosphere. We reproduce the topology of
the reflected energy distribution in the equatorial plane by modeling
discrete chorus elements generated at the equator. Our calculations show that
the spatial spreading is large and strongly dependent upon initial wave
parameters, especially the chorus wave frequency. Thus, the divergence of
each element ray trajectories can result in the filling of a large region
(about 4 Earth radii around the source) of the magnetosphere and a reflected
intensity of 0.005–0.06 of the source signal in the equatorial plane. These
results are in good agreement with previous Cluster and THEMIS observations. |
| |
|
| Teil von |
|
|
|
|
|
|
|
|