Latitudinal and radial variation of >2 GeV/n protons and alpha-particles at solar maximum: ULYSSES COSPIN/KET and neutron monitor network observations

Belov, A. V.; Eroshenko, E. A.; Heber, B.; Yanke, V. G.; Raviart, A.; Müller-Mellin, R.; Kunow, H.

doi:https://doi.org/10.5194/angeo-21-1295-2003

Articles | Volume 21, issue 6

https://doi.org/10.5194/angeo-21-1295-2003

© Author(s) 2003. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue:

Ulysses and Beyond

https://doi.org/10.5194/angeo-21-1295-2003

© Author(s) 2003. This work is distributed under
the Creative Commons Attribution 3.0 License.

Articles | Volume 21, issue 6

30 Jun 2003

| 30 Jun 2003

Latitudinal and radial variation of >2 GeV/n protons and alpha-particles at solar maximum: ULYSSES COSPIN/KET and neutron monitor network observations

A. V. Belov, E. A. Eroshenko, B. Heber, V. G. Yanke, A. Raviart, R. Müller-Mellin, and H. Kunow

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Latest update: 24 Apr 2024

Latitudinal and radial variation of >2 GeV/n protons and alpha-particles at solar maximum: ULYSSES COSPIN/KET and neutron monitor network observations

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