Abstract: The heliosphere is the region around the Sun that is filled by the solar wind and its embedded magnetic field. The interaction of the supersonic solar wind with the local interstellar medium leads to a transition from supersonic to subsonic speeds at the heliospheric termination shock. The latter is regarded to be the source of the anomalous component of cosmic rays. Within the heliosphere “local” energetic particle sources, like the Sun and interplanetary shock waves contribute to the cosmic ray flux, too. At energies below a few GeV the observed galactic and anomalous cosmic ray intensities are modulated by the heliospheric magnetic field. In my contribution, both the current knowledge and hypotheses about modulation and the transport of cosmic rays in the heliosphere are reviewed.
Information on participating / attending:
Organisation: Prof. H. Fehske und Prof. L. Schweikhard
Kontakt: Institut für Physik, Felix-Hausdorff-Straße 6, 17487 Greifswald,
Telefon 03834 86-4700, info@physik.uni-greifswald.de
Date:
07/04/2013 17:00 - 07/04/2013 18:00
Event venue:
Hörsaal, Institut für Physik
Felix-Hausdorff-Straße 6
17489 Greifswald
Mecklenburg-Vorpommern
Germany
Target group:
Scientists and scholars, Students
Relevance:
regional
Subject areas:
Physics / astronomy
Types of events:
Presentation / colloquium / lecture
Entry:
04/17/2013
Sender/author:
Sabine Köditz
Department:
Presse- und Informationsstelle
Event is free:
yes
Language of the text:
German
URL of this event: http://idw-online.de/en/event43334
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