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| Titel |
Ionisation as indicator for cosmic ray acceleration |
| VerfasserIn |
F. Schuppan, C. Röken, N. Fedrau, J. Becker Tjus |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
2199-3955
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| Digitales Dokument |
URL |
| Erschienen |
In: ASTRA Proceedings ; 1, no. 1 ; Nr. 1, no. 1 (2014-06-02), S.13-17 |
| Datensatznummer |
250115104
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| Publikation (Nr.) |
 copernicus.org/ap-1-13-2014.pdf |
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| Zusammenfassung |
| Astrospheres and wind bubbles of massive stars are believed to be sources of
cosmic rays with energies E ≲ 1 TeV. These particles are not
directly detectable, but their impact on surrounding matter, in particular
ionisation of atomic and molecular hydrogen, can lead to observable
signatures. A correlation study of both gamma ray emission, induced by
proton-proton interactions of cosmic ray protons with kinetic energies
Ep ≥ 280 MeV with ambient hydrogen, and ionisation
induced by cosmic ray protons of kinetic energies Ep <
280 MeV can be performed in order to study potential sources of
(sub)TeV cosmic rays. |
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