The flux of the helium component of the primary cosmic radiation at geomagnetic latitude 41‡ N

1956 ◽  
Vol 3 (5) ◽  
pp. 1150-1152 ◽  
Author(s):  
A. De Marco ◽  
A. Milone ◽  
M. Reinharz
Keyword(s):  
Cosmic Radiation ◽  
Geomagnetic Latitude ◽  
Primary Cosmic Radiation

THE HYDROGEN COMPONENT IN THE PRIMARY COSMIC RADIATION

1962 ◽  
Vol 40 (9) ◽  
pp. 1049-1055 ◽  
Author(s):  
H. H. Aly
Keyword(s):  
High Altitude ◽  
Cosmic Radiation ◽  
Nuclear Emulsion ◽  
Geomagnetic Latitude ◽  
The Other ◽  
Primary Cosmic Radiation ◽  
Good Agreement

Two values for the flux of the hydrogen component in the primary cosmic radiation have been measured. The first one was over Guam in the Marianas Islands, geomagnetic latitude λ = 0°. The value of the flux was found to be (123 ± 12) hydrogen nuclei/m2 sterad sec. The second measurement was made over Texas, λ = 41 °N., and the value found was (530 ± 53) hydrogen nuclei/m2 sterad sec. The detectors in both cases were stacks of nuclear emulsion exposed at high altitude. The results obtained in this experiment are in good agreement with the values obtained by the other authors using electronic counters flown at the same geomagnetic latitudes.

Untersuchungen über die schweren Kerne in der primären kosmischen Strahlung

1958 ◽  
Vol 13 (10) ◽  
pp. 801-808 ◽  
Author(s):  
Wolfgang Püschel
Keyword(s):  
Cosmic Radiation ◽  
Geomagnetic Latitude ◽  
Geometrical Model ◽  
Northern Italy ◽  
Incident Particle ◽  
Heavy Nuclei ◽  
Nuclear Radius ◽  
Primary Cosmic Radiation ◽  
Good Agreement

Fragmentation probabilities and interaction mean free paths for the interaction of heavy nuclei (Z > 2) of the primary cosmic radiation with target nuclei of emulsions (Ilford G 5) have been obtained. The experiment has been carried out in Northern Italy, at a geomagnetic latitude of 46° N. The values are in good agreement with those reported previously by Fowler, Hillier, Waddington and Rajopadhye, Waddingto and Cester, Debenedetti, Garelli, Quassiati, Tallone, Vigone.Values are derived for the fragmentation probabilities in air by a geometrical model introduced by Noon and Kaplon.Assigning both to the incident particle and to the target nuclei a radius R = R0 · A⅓, one obtains an effective nuclear radius R0=1,2·10-13 cm.Using our values for the fragmentation probabilities instead of the lower values found in an experiment by KAPLON et al., their ratio for the fluxes of L-nuclei to M-nuclei at the top of the atmosphere is increased from 0.46 to about 0.80.

The Penumbra at Geomagnetic Latitude 20° and the Energy Spectrum of Primary Cosmic Radiation

1939 ◽  
Vol 55 (7) ◽  
pp. 614-620 ◽  
Author(s):  
R. Albagli Hutner
Keyword(s):  
Energy Spectrum ◽  
Cosmic Radiation ◽  
Geomagnetic Latitude ◽  
Primary Cosmic Radiation

Energy Spectrum of Heavy Nuclei of the Primary Cosmic Radiation during Solar Maximum

1963 ◽  
Vol 130 (1) ◽  
pp. 362-368 ◽  
Author(s):  
K. A. Neelakantan ◽  
P. G. Shukla
Keyword(s):  
Energy Spectrum ◽  
Cosmic Radiation ◽  
Solar Maximum ◽  
Heavy Nuclei ◽  
Primary Cosmic Radiation

scholarly journals The search of the anisotropy of the primary cosmic radiation by the difference method

2017 ◽  
Vol 145 ◽  
pp. 03003
Author(s):  
Victor Pavlyuchenko ◽  
Romen Martirosov ◽  
Natalia Nikolskaya ◽  
Anatoly Erlykin
Keyword(s):  
Difference Method ◽  
Cosmic Radiation ◽  
Primary Cosmic Radiation ◽  
The Difference

The Determination of the Sign and the Energy Spectrum of Primary Cosmic Radiation

1947 ◽  
Vol 71 (7) ◽  
pp. 393-398 ◽  
Author(s):  
M. S. Vallarta ◽  
M. L. Perusquía ◽  
J. de Oyarzábal
Keyword(s):  
Energy Spectrum ◽  
Cosmic Radiation ◽  
Primary Cosmic Radiation
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