![Hier klicken, um den Treffer aus der Auswahl zu entfernen](images/unchecked.gif) |
Titel |
The Propagation of Jovian Electrons in the Heliospheric Magnetic Field |
VerfasserIn |
O. Sternal, B. Heber, H. Fichtner, A. Burger |
Konferenz |
EGU General Assembly 2009
|
Medientyp |
Artikel
|
Sprache |
Englisch
|
Digitales Dokument |
PDF |
Erschienen |
In: GRA - Volume 11 (2009) |
Datensatznummer |
250023126
|
|
|
|
Zusammenfassung |
The propagation of energetic particles in the heliosphere is described
by the Parker transport equation including the physical processes of
diffusion, drift, convection and adiabatic energy changes. For the inner
heliosphere the Jovian magnetosphere appears to be the dominant source
of energetic electrons. Therefore the so-called Jovian electrons are
nearly perfect test particles to study transport theories. In this
contribution we present model calculations of the electron flux in
Parker- and Fisk-type heliospheric magnetic field configurations and
compare our results to spacecraft data. |
|
|
|
|
|