Fig. 8From: Occurrence characteristics of electromagnetic ion cyclotron waves at sub-auroral Antarctic station Maitri during solar cycle 24Probability distribution functions of solar wind parameters: a density n, b dynamic pressure, and c velocity V, and d proton temperature \(T_i\) at the Earth’s bow-shock nose for the ascending (blue) and descending (red) phases of the solar cycle 24. Here, \(\sum pdf\) corresponds to 1, which means 100%Back to article page