dot
Detailansicht
Katalogkarte GBA
Katalogkarte ISBD
Suche präzisieren
Drucken
Download RIS
Hier klicken, um den Treffer aus der Auswahl zu entfernen
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.