Survey and Comparison of Solar Activity and Energetic Particle Emission in 1970,

Author(s):  
H. W. Dodson-Prince ◽  
E. R. Hedeman ◽  
O. C. Mohler
1991 ◽  
Vol 39 (4) ◽  
pp. 557-562
Author(s):  
A. Geranios ◽  
S. Fischer ◽  
M. Vandas ◽  
K. Kudela

1999 ◽  
Author(s):  
R. G. Marsden ◽  
D. Lario ◽  
T. R. Sanderson ◽  
M. Maksimovic ◽  
A. Balogh ◽  
...  

1985 ◽  
Vol 156 (1-2) ◽  
pp. 42-46 ◽  
Author(s):  
J.L. Laville ◽  
C. Le Brun ◽  
J.F. Lecolley ◽  
F. Lefebvres ◽  
M. Louvel ◽  
...  

2000 ◽  
Vol 179 ◽  
pp. 251-254
Author(s):  
Vladislav Timofeev ◽  
Sergey Starodubtsev

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.


2019 ◽  
Vol 11 (4) ◽  
pp. 974
Author(s):  
Aleksandra Nina ◽  
Vladimir Srećković ◽  
Milan Radovanović

The atmosphere is a very sensitive medium to extraterrestrial forces, most importantly, solar electromagnetic radiation and energetic particle intrusion. This released intense solar activity can cause sudden disturbances in the Earth’s atmosphere and further create ground telecommunication interferences, blackouts, transportation problems, water supply problems, potential health effects, as well as natural disasters, such as forest fires. These extreme events can cause billions of dollars of damage and impact individuals, families, communities, and societies. For this reason, it is of crucial importance to investigate the connections between this extreme activity and natural disasters, and further develop ways to prevent, prepare against, and respond to them. The aim of this special issue is to engage a wide community of scientists to de-fragment broaden and improve our knowledge in this field. We invite researchers from all relevant fields to publish their recent investigations in this special issue.


1991 ◽  
Vol 15 (2) ◽  
pp. 145-148 ◽  
Author(s):  
A Badala ◽  
R Barbera ◽  
G Bizard ◽  
D Durand ◽  
J. L Laville ◽  
...  

2020 ◽  
Vol 63 (5) ◽  
Author(s):  
Jianping Huang ◽  
Xuhui Shen ◽  
Wenjing Li ◽  
Wei Chu

A megathrust earthquake with Mw 9.0 occurred in the North-western Pacific Ocean on March 11, 2011. From the energetic particle flux from WIND, CLUSTER and GOES in different L locations, some variation can be found around the earthquake. Among the three satellites, WIND is used to identify solar activity, and GOES is used to detect the changes from ground source. And during the same period, a magnetic storm with intensity -80nT occur. In order to validate the particle flux variation, multi-parameters relationship is compared. The results show that: (1) all energetic fluxes variation can reflect the solar activity. The far ones are connected with the F10.7 and the near ones are connected with Dst/Kp. (2) The energetic particle fluxes give a scarp change in all energy bands at the beginning coupling period and when the space recovers to be quite, the fluxes will have a long decreasing tail from high to low energy. (3) The coseismic and after effect have been detected in GOES and the pre-seismic emission should exist because the bigger decreasing fluxes in GOES are responding to the period with smaller Kp.


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