A Cloud-Chamber Study of Neutron Production by Sea-Level Cosmic Rays with Particular Reference toμ-Mesons Stopped in Lead

1953 ◽  
Vol 91 (2) ◽  
pp. 373-384 ◽  
Author(s):  
E. J. Althaus ◽  
R. D. Sard
Keyword(s):  
Cosmic Rays ◽  
Sea Level ◽  
Neutron Production ◽  
Cloud Chamber ◽  
Chamber Study

scholarly journals Cloud Chamber Observations of Cosmic Rays at 4300 Meters Elevation and Near Sea-Level

1936 ◽  
Vol 50 (4) ◽  
pp. 263-271 ◽  
Author(s):  
Carl D. Anderson ◽  
Seth H. Neddermeyer
Keyword(s):  
Cosmic Rays ◽  
Sea Level ◽  
Cloud Chamber

Neutron Production by Cosmic Rays at Sea Level

1949 ◽  
Vol 75 (5) ◽  
pp. 894-895 ◽  
Author(s):  
A. R. Tobey
Keyword(s):  
Cosmic Rays ◽  
Sea Level ◽  
Neutron Production

Neutron Production by Cosmic Rays at Sea Level

1951 ◽  
Vol 81 (4) ◽  
pp. 517-519 ◽  
Author(s):  
A. R. Tobey ◽  
C. G. Montgomery
Keyword(s):  
Cosmic Rays ◽  
Sea Level ◽  
Neutron Production

Cloud-Chamber Study of Cosmic Rays Underground

1950 ◽  
Vol 77 (6) ◽  
pp. 849-849 ◽  
Author(s):  
O. L. Tiffany ◽  
W. E. Hazen
Keyword(s):  
Cosmic Rays ◽  
Cloud Chamber ◽  
Chamber Study

Time and other Variations in the Intensity of Cosmic Ray Neutrons

1951 ◽  
Vol 6 (11) ◽  
pp. 592-598
Author(s):  
N. Adams ◽  
H. J. J. Braddick
Keyword(s):  
Cosmic Rays ◽  
Solar Flare ◽  
Diurnal Variation ◽  
Sea Level ◽  
Geomagnetic Latitude ◽  
Cosmic Ray ◽  
Temporal Variations ◽  
Neutron Production ◽  
Neutron Intensity

AbstractWe have measured the barometer coefficient of cosmic ray neutron production at sea level and find the value -9,25% ± 0,20/cmHg. We have shown that there is no diurnal variation of neutron production of amplitude greater than about 0,4 %. The effects of the large solar flare of November 19 th , 1949 on cosmic ray neutrons were much greater than on ionising cosmic rays at sea level; the maximum factor of increase was more than 5 and the intensity remained measurably above normal for about 12 hours. A small increase of neutron intensity is found, statistically, to be correlated with a number of recorded radio fade-outs. It is suggested that neutron measurements are particularly suitable for studying temporal variations of cosmic rays. The latitude increase of cosmic ray neutrons between geomagnetic latitude 54,5° and 56,5° was found to be about 2%. No certain increase was found between 56,5° and 59,5°.

scholarly journals Cloud-Chamber Study of Negative Strange Particles

1956 ◽  
Vol 104 (6) ◽  
pp. 1688-1694 ◽  
Author(s):  
G. H. Trilling ◽  
G. Neugebauer
Keyword(s):  
Cloud Chamber ◽  
Strange Particles ◽  
Chamber Study

Cloud-Chamber Study of Mesons Stopping in Aluminum Foils

1949 ◽  
Vol 75 (8) ◽  
pp. 1275-1276 ◽  
Author(s):  
R. L. Cool ◽  
E. C. Fowler ◽  
J. C. Street ◽  
W. B. Fowler ◽  
R. D. Sard
Keyword(s):  
Cloud Chamber ◽  
Chamber Study
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