Solar Intensity Variation due to Coronal Mass Ejection Over a Long Range Time Period

Uzmah Bilkees, Rajeev Kumar Singh

Abstract: Earth system processes (ESP) are interrelated collection of processes in which changes are characterized continuously through which material or energy flow occurs. While looking at the data retrieved from different repositories like Solar and Heliospheric Observatory (SOHO), we presume that due to variation of the physical and morphological properties of coronal mass ejections (CMEs) in the sun. There will be changes in the Earths atmosphere corresponding to the solar cycle of CME. The CME parameters like intensity, halo, mass, acceleration, angular and linear speed from the SOHO data can be very much useful to Sun-Earth connection to drive important and dynamic state of the Earth system. We could infer here that CMEs might have a un-deciphered importance in the earth system processes (ESP).

Keywords: Earth system processes ESP, Sun, thermodynamic equilibrium TE, Maximum entropy production MEP, Irradiance, coronal mass ejection

How to Cite?: Uzmah Bilkees, Rajeev Kumar Singh, "Solar Intensity Variation due to Coronal Mass Ejection Over a Long Range Time Period", Volume 7 Issue 11, November 2018, International Journal of Science and Research (IJSR), Pages: 1378-1381, https://www.ijsr.net/getabstract.php?paperid=ART20192654, DOI: https://dx.doi.org/10.21275/ART20192654