Characteristic Times of Gradual Solar Energetic Particle Events and Their Dependence on Associated Coronal Mass Ejection Properties

2005 ◽  
Vol 628 (2) ◽  
pp. 1014-1022 ◽  
Author(s):  
S. W. Kahler
Keyword(s):  
Coronal Mass Ejection ◽  
Energetic Particle ◽  
Solar Energetic Particle ◽  
Solar Energetic Particle Events ◽  
Mass Ejection

scholarly journals Strength of Coronal Mass Ejection‐driven Shocks near the Sun and Their Importance in Predicting Solar Energetic Particle Events

2007 ◽  
Vol 670 (1) ◽  
pp. 849-856 ◽  
Author(s):  
Chenglong Shen ◽  
Yuming Wang ◽  
Pinzhong Ye ◽  
X. P. Zhao ◽  
Bin Gui ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
Energetic Particle ◽  
Solar Energetic Particle ◽  
The Sun ◽  
Solar Energetic Particle Events ◽  
Mass Ejection

Solar Energetic Particle Events at the Rise Phase of the 23rd Solar Activity Cycle Registered aboard the Spacecraft “INTERBALL-2”

2000 ◽  
Vol 179 ◽  
pp. 251-254
Author(s):  
Vladislav Timofeev ◽  
Sergey Starodubtsev
Keyword(s):  
Solar Activity ◽  
Solar Flares ◽  
Energetic Particle ◽  
Solar Energetic Particle ◽  
Activity Cycle ◽  
Solar Activity Cycle ◽  
Solar Energetic Particle Events ◽  
Mass Ejection ◽  
Rise Phase ◽  
23Rd Solar Activity Cycle

AbstractThe experiment with 10K-80 aboard the INTER-BALL-2 (which detects protons with energies > 7, 27–41, 41–58, 58–88, 88–180 and 180–300 MeV) registered six events of the solar energetic particle (SEP) increase. These events are during the initial rise phase of the 23rd solar activity cycle. Solar flares with the SEP generation are accompanied by coronal mass ejection (CME). Here we analyze the dynamics of the differential energy spectrum at different phases of the SEP increase.

Sign in / Sign up

Export Citation Format

Share Document