The study presented the archived data of Coronal Mass Ejection (CME) together with its intrinsic properties and Smooth Sunspot Number (SSN) that both came from international science institutions which are the Solar Heliospheric Observatory and National Oceanic and Atmospheric Administration with the purpose of finding the relationship between the SSN and CME together with its properties. Also to determined the behavior of the two variables during solar maximum. With the data gathered the researcher will be able to conclude the relationship of the two.
The researcher used the descriptive method in this study, to determine the relationship of SSN and CME with its intrinsic properties such as width, frequency, initial and final velocity and acceleration. This method enabled the researcher to establish if this relationship exists. The research materials that were used in this study were the archived data from National Oceanic and Atmospheric Administration (NOAA) for Smooth Sunspot Data and for the CME Data came from Solar Heliospheric Observatory (SOHO). The archived data ranges from the year 1996-2012.
By: Princess B. Tucio
The researcher used the descriptive method in this study, to determine the relationship of SSN and CME with its intrinsic properties such as width, frequency, initial and final velocity and acceleration. This method enabled the researcher to establish if this relationship exists. The research materials that were used in this study were the archived data from National Oceanic and Atmospheric Administration (NOAA) for Smooth Sunspot Data and for the CME Data came from Solar Heliospheric Observatory (SOHO). The archived data ranges from the year 1996-2012.
By: Princess B. Tucio