scholarly journals Comparisons of predictions from two intranuclear-cascade models with measured secondary proton spectra at several angles from 62- and 39-MeV protons on various elements

1974 ◽  
Author(s):  
H. W. Bertini ◽  
G. D. Harp ◽  
F. E. Bertrand
2015 ◽  
Vol 91 (3) ◽  
Author(s):  
Davide Mancusi ◽  
Alain Boudard ◽  
Jaume Carbonell ◽  
Joseph Cugnon ◽  
Jean-Christophe David ◽  
...  

1980 ◽  
Vol 58 (6) ◽  
pp. 891-899 ◽  
Author(s):  
H. Dautet ◽  
G. Bischoff ◽  
J. M. D'Auria ◽  
B. D. Pate

Absolute cross sections for short-lived alpha emitting, very neutron deficient nucleides resulting from the interaction of 480 MeV protons with several medium mass targets (Ho, Tm, Re, Ta, Au) have been measured at the TRIUMF facility (Vancouver, Canada). Activities were transported using a gas jet system and relative transport efficiencies for products of various Z were measured. Calculations for the production of such deep spallation products were performed using the empirical Silberberg–Tsao method and the more fundamental, intranuclear cascade – evaporation model, and compared against the observed values.


1986 ◽  
Vol 33 (3) ◽  
pp. 867-875 ◽  
Author(s):  
Joseph J. Molitoris ◽  
Horst Stöcker ◽  
Hans-ke Gustafsson ◽  
Joseph Cugnon ◽  
Denis L’Hte

2021 ◽  
Vol 73 (1) ◽  
Author(s):  
Mitsuo Oka ◽  
Takahiro Obara ◽  
Nariaki V. Nitta ◽  
Seiji Yashiro ◽  
Daikou Shiota ◽  
...  

AbstractIn gradual Solar Energetic Particle (SEP) events, shock waves driven by coronal mass ejections (CMEs) play a major role in accelerating particles, and the energetic particle flux enhances substantially when the shock front passes by the observer. Such enhancements are historically referred to as Energetic Storm Particle (ESP) events, but it remains unclear why ESP time profiles vary significantly from event to event. In some cases, energetic protons are not even clearly associated with shocks. Here, we report an unusual, short-duration proton event detected on 5 June 2011 in the compressed sheath region bounded by an interplanetary shock and the leading edge of the interplanetary CME (or ICME) that was driving the shock. While < 10 MeV protons were detected already at the shock front, the higher-energy (> 30 MeV) protons were detected about four hours after the shock arrival, apparently correlated with a turbulent magnetic cavity embedded in the ICME sheath region.


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