The power spectrum of cosmic ray fluctuations and its role in discriminating the statistically significant fluctuations in detection data
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Los resultados de las observaciones de la intensidad de los rayos cósmicos con telescopios de centelleo, supermonitores de neutrones y telescopios de mesones son utilizados para calcular los espectros de potencia de las fluctuaciones de los rayos cósmicos en la superficie terrestre durante varios periodos de actividad solar y geomagnética. Se muestra que la confiabilidad de los cálculos de las estimaciones espectrales relativas, es mucho mayor cuando se hace con base en el espectro calculado.
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