Large-scale cosmic ray fluctuations inferred from the ground-based neutron and ionizing component observations and their relevance to cosmic ray anisotropy
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Se estudia el comportamiento del espectro de potencia de las fluctuaciones en la intensidad de los rayos cósmicos para frecuencias menores de 10-4Hz, determinado a partir de las observaciones en superficie de las componentes nucleónica y de ionización. Se hace un intento de describir el espectro de fluctuaciones, usando cambios en el valor de la anisotropía de rayos cósmicos y del espectro de inhomogeneidades del campo magnético interplanetario.
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