scholarly journals Solar Neutron Decay Protons Observed in November 7, 2004

2021 ◽  
Author(s):  
Yasushi Muraki
Keyword(s):  
1990 ◽  
Vol 73 ◽  
pp. 273 ◽  
Author(s):  
Paul Evenson ◽  
Richard Kroeger ◽  
Peter Meyer ◽  
Donald Reames

1990 ◽  
Vol 73 ◽  
pp. 272
Author(s):  
Paul Evenson ◽  
Richard Kroeger ◽  
Peter Meyer ◽  
Donald Reames

1970 ◽  
Vol 75 (7) ◽  
pp. 1257-1262 ◽  
Author(s):  
E. Scott Claflin ◽  
R. Stephen White

1991 ◽  
Vol 18 (5) ◽  
pp. 829-832 ◽  
Author(s):  
M. A. Shea ◽  
D. F. Smart ◽  
Margaret D. Wilson ◽  
E. O. Flückiger

1997 ◽  
Vol 49 (9) ◽  
pp. 1105-1113
Author(s):  
Takasuke Sakai ◽  
Masahito Kato ◽  
Yasusi Muraki

2020 ◽  
Author(s):  
Yasushi Muraki ◽  
Jose F Valdes Galicia ◽  
Ernesto Fragoso Ortiz ◽  
Yutaka Matsubara ◽  
Shoichi Shibata ◽  
...  

Abstract We have found an interesting event registered by the solar neutron telescopes installed at high mountains in Bolivia (5250m a.s.l.) and Mexico (4600m a.s.l.). The event was observed November 7th of 2004 in association with a large solar flare of magnitude X2.0. Some features in our registers and in two satellites (GOES11 and SOHO) reveal the presence of electrons and protons as possible products of neutron decay. Solar neutron decay protons (sndp) were recorded on board ISEE3 satellite in June 3rd, 1982. On October 19th, 1989, the ground level detectors installed in Goose Bay and Deep River revealed the registration of solar neutron decay protons (sndp). Therefore this is the second example that such an evidence is registered on the Earth´s surface.Key words: Solar neutron decay protons, Solar flare, Solar Energetic particles,Particle acceleration


1994 ◽  
Vol 144 ◽  
pp. 635-639
Author(s):  
J. Baláž ◽  
A. V. Dmitriev ◽  
M. A. Kovalevskaya ◽  
K. Kudela ◽  
S. N. Kuznetsov ◽  
...  

AbstractThe experiment SONG (SOlar Neutron and Gamma rays) for the low altitude satellite CORONAS-I is described. The instrument is capable to provide gamma-ray line and continuum detection in the energy range 0.1 – 100 MeV as well as detection of neutrons with energies above 30 MeV. As a by-product, the electrons in the range 11 – 108 MeV will be measured too. The pulse shape discrimination technique (PSD) is used.


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