International Journal of Science and Research (IJSR)

International Journal of Science and Research (IJSR)
Call for Papers | Fully Refereed | Open Access | Double Blind Peer Reviewed

ISSN: 2319-7064

ser



Downloads: 106 | Views: 209

Research Paper | Physics Science | India | Volume 5 Issue 4, April 2016 | Rating: 6.2 / 10


Statistical Study of Coronal Mass Ejections during Rising Phase of Solar Cycle 24

Nisha Patel [3] | Ajaysinh K. Jadeja [2]


Abstract: We have analyzed the data for more than 8000 CMEs which were obtained by Large Angle and Spectrometric Coronagraph Experiment on board Solar and Heliospheric Observatory during the rising phase of solar cycle 24. We found that the speed distribution for events with strong peak at v = 344 km/ s and a long tail (>1000 km/s) is to a good approximation they can be fitted with a single log-normal distribution. Based on SOHO/LASCO catalogue and solar geophysical data, we have also studied the geo-effectiveness, solar source and flare association of a set of 192 halo CMEs during the period of 2008 to 2013. CMEs with maximum rate of geo-effectiveness occurred in maximum phase of solar cycle. Maximum number of strong storms occurred towards western hemisphere. Front disk halos are faster. Most intense storms are due to front side limb halo. Severe storms (Dst < -200nT) not have been observed during the initial phase of solar cycle 24.


Keywords: Coronal Mass Ejection, Limb Halo, Disk Halo, SOHO, LASCO


Edition: Volume 5 Issue 4, April 2016,


Pages: 1342 - 1345


How to Download this Article?

Type Your Valid Email Address below to Receive the Article PDF Link


Verification Code will appear in 2 Seconds ... Wait

Top