The Statistical Analysis of Coronal Mass Ejection During the Ascending Phase of Solar Cycle 24 and 25

We analysed the angular width and linear speed of all kinds of CMEs, including intermediate (20 ^º <W<200 ^º ), wide (W≥ 200 ^º ), and linear speed 500 km/s, during the ascending phase of solar cycles 24 and 25.Solar cycle 24 has intermediate CME 434 which is 4.5 times more than solar cycle 25. On the other hand, there was no noticeable difference in the number of large CMEs during solar cycles 24 and 25 (405 and 406, respectively). The striking finding is that the angular distributions for the ascending phase of solar cycles are quite similar. The maximum speed observed during ascending phase of solar cycle 24 is 2658 km/s (wide) and the maximum speed in ascending phase of solar cycle 25 is 2669 km/s (wide). The maximum number of wide Coronal Mass Ejections are occurred in the year of 2023.It was noticed that the maximum speed of solar cycle 24 is higher than the solar cycle 24.