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- W2119189061 abstract "We generalize our previous discussion of the fluctuations in the cosmic ray intensity near earth by including non-field-aligned diffusion in the model. For frequencies of ≳ 5 × 10−6 Hz the fluctuations are interplanetary scintillations caused by the field-aligned anisotropy, as was previously discussed. For lower frequencies the effects of non-field-aligned diffusion dominate and give a power spectral density proportional to f−2. Observations are presented which support the model." @default.
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- W2119189061 date "1976-05-01" @default.
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- W2119189061 title "Cosmic ray scintillations, 4. The effects of non-field-aligned diffusion" @default.
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- W2119189061 doi "https://doi.org/10.1029/ja081i013p02094" @default.
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