Long-term neutron monitor observations and the 2009 cosmic ray maximum

Author:

Moraal H.1,Stoker P. H.1

Affiliation:

1. Unit for Space Physics, School for Physical and Chemical Sciences; North-West University; Potchefstroom South Africa

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference23 articles.

1. For how long will the current grand maximum of solar activity persist?;Abreu;Geophys. Res. Lett.,2008

2. Galactic cosmic-ray modulation: effects of the solar wind termination shock and the heliosheath;Caballero-Lopez;J. Geophys. Res.,2004

3. The heliospheric magnetic field from 850 to 2000 inferred from 10Be records;Caballero-Lopez;J. Geophys. Res.,2004

4. Cosmic ray survey to Antarctica and coupling functions for neutron component near solar minimum (1996-1997), 2. Determination of meteorological effects;Iucci;J. Geophys. Res.,2000

5. Krainev , M. M. Kalinin 2009 On the current phase of the solar cycle in the solar and heliospheric parameters and GCR intensity Proc. 31st Int. Cosmic-ray Conf. 1043

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