Fig. 15From: Nighttime Pc3 pulsations: MM100 and MAGDAS observations 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)Back to article page