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  What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes?

Keppler, E. (1998). What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes? Annales Geophysicae, 16(12), 1552-1556.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-D9FA-0 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-D9FB-E
Genre: Journal Article

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 Creators:
Keppler, E.1, Author           
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1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: ULYSSES: EPAC
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 Dates: 1998
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: BibTex Citekey: Keppler:1998-109
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Title: Annales Geophysicae
Source Genre: Journal
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Pages: - Volume / Issue: 16 (12) Sequence Number: - Start / End Page: 1552 - 1556 Identifier: -