Format:
1 Online-Ressource (xxii, 154 Seiten, 34525 KB)
,
Illustrationen, Diagramme
Content:
The Earth's inner magnetosphere is a very dynamic system, mostly driven by the external solar wind forcing exerted upon the magnetic field of our planet. Disturbances in the solar wind, such as coronal mass ejections and co-rotating interaction regions, cause geomagnetic storms, which lead to prominent changes in charged particle populations of the inner magnetosphere - the plasmasphere, ring current, and radiation belts. Satellites operating in the regions of elevated energetic and relativistic electron fluxes can be damaged by deep dielectric or surface charging during severe space weather events. Predicting the dynamics of the charged particles and mitigating their effects on the infrastructure is of particular importance, due to our increasing reliance on space technologies. The dynamics of particles in the plasmasphere, ring current, and radiation belts are strongly coupled by means of collisions and collisionless interactions with electromagnetic fields induced by the motion of charged particles. Multidimensional numerical ...
Note:
kumulative Dissertation
,
Dissertation Universität Potsdam 2020
Additional Edition:
Erscheint auch als Druck-Ausgabe Aseev, Nikita Modeling and understanding dynamics of charged particles in the Earth's inner magnetosphere Potsdam, 2020
Language:
English
Keywords:
Magnetosphäre
;
Hochschulschrift
DOI:
10.25932/publishup-47921
URN:
urn:nbn:de:kobv:517-opus4-479211
URL:
https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-479211
URL:
https://d-nb.info/1220355364/34
Author information:
Pikovskij, Arkadij 1956-
Bookmarklink