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Fig. 3 | Earth, Planets and Space

Fig. 3

From: Investigation of the relationship between geomagnetic activity and solar wind parameters based on a novel neural network (potential learning)

Fig. 3

Results of the application of PL at r = 5. The five OMNI solar wind parameters (IMF-Bx, IMF-By, Vx, Np, and Bs) are chosen as the input data to PL. The horizontal and vertical axes give input potentiality and the numbers of input five solar wind parameters, respectively. The potentialities of the solar wind velocity and density are 1.0 and 0.1208, respectively

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