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Fig. 15 | Earth, Planets and Space

Fig. 15

From: Nighttime Pc3 pulsations: MM100 and MAGDAS observations

Fig. 15

Left empirical probability density function of the IMF magnetic field magnitude B for the intervals with the two types of night Pc3 pulsations: Pc3n\(_D\) (red) and Pc3n\(_L\) (blue), and for all the intervals analyzed (gray). Right empirical probability density function of \(\Delta f=f_B-f_c\) for the intervals with the two types of night Pc3 pulsations: Pc3n\(_D\) (red) and Pc3n\(_L\) (blue)

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