scholarly journals Observation of charmed particles produced by high-energy photons in nuclear emulsions coupled with a magnetic spectrometer

1981 ◽  
Author(s):  
B. Conforto ◽  
A. S Conti ◽  
M. m. Chernyavski ◽  
M. G. Dagliana ◽  
M. Dameri ◽  
...  
Keyword(s):  
High Energy ◽  
Magnetic Spectrometer ◽  
Nuclear Emulsions

scholarly journals Observation of pairs of charmed particles produced by high-energy photons in nuclear emulsions coupled with a magnetic spectrometer

1981 ◽  
Vol 99 (3) ◽  
pp. 271-276 ◽  
Author(s):  
M.I. Adamivich ◽  
Y.A. Alexandrov ◽  
J.M. Bolta ◽  
L. Bravo ◽  
A.M. Cartacci ◽  
...  
Keyword(s):  
High Energy ◽  
Magnetic Spectrometer ◽  
Nuclear Emulsions

Solar neutron flux in the energy range 20–160 MeV

1970 ◽  
Vol 48 (18) ◽  
pp. 2155-2161 ◽  
Author(s):  
C. Y. Kim
Keyword(s):  
Neutron Flux ◽  
Energy Range ◽  
Sunspot Number ◽  
Solar Flares ◽  
Energy Region ◽  
High Energy ◽  
The Sun ◽  
Solar Neutron ◽  
Nuclear Emulsions ◽  
The Difference

An attempt to measure the flux of high-energy solar neutrons was made by measuring the difference in flux from the direction of the sun and from the symmetrical direction about the zenith, using oriented nuclear emulsions flown by balloon on July 30, 1966 from Fort Churchill, Manitoba.An excess of (2.2 ± 2.5) × 10−2 neutrons cm−2 s−1 was observed from the direction of the sun in the energy region of 20–160 MeV. On the day of the flight the sunspot number was 63, and no major solar flares were reported.

Astrophysics and Particle Physics in Space with the Alpha Magnetic Spectrometer

2003 ◽  
Vol 18 (28) ◽  
pp. 1951-1966 ◽  
Author(s):  
Giovanni Lamanna
Keyword(s):  
Particle Physics ◽  
Gamma Ray ◽  
Space Shuttle ◽  
Space Station ◽  
Cosmic Ray ◽  
High Energy ◽  
Magnetic Spectrometer ◽  
High Energy Particle ◽  
Physics Experiment ◽  
Alpha Magnetic Spectrometer

The Alpha Magnetic Spectrometer (AMS) is a high energy particle physics experiment in space scheduled to be installed on the International Space Station (ISS) by 2006 for a three-year mission. After a precursor flight of a prototype detector on board of the NASA Space Shuttle in June 1998, the construction of the detector in its final configuration is started and it will be completed by 2004. The purpose of this experiment is to provide a high statistics measurement of charged particles and nuclei in rigidity range 0.5 GV to few TV and to explore the high-energy (> 1 GeV ) gamma-ray sky. In this paper we describe the detector layout and present an overview of the main scientific goals both in the domain of astrophysics: cosmic-ray origin, age and propagation and the exploration of the most energetic gamma-ray sources; and in the domain of astroparticle: the anti-matter and the dark matter searches.

High Energy Cosmic-Ray Showers in Nuclear Emulsions

1951 ◽  
Vol 81 (2) ◽  
pp. 239-244 ◽  
Author(s):  
L. S. Osborne
Keyword(s):  
Cosmic Ray ◽  
High Energy ◽  
Nuclear Emulsions

About high energy interactions in nuclear emulsions

1958 ◽  
Vol 8 (1) ◽  
pp. 166-169 ◽  
Author(s):  
P. Ciok ◽  
T. Coghen ◽  
J. Gierula ◽  
E. Hołyński ◽  
A. Jurak ◽  
...  
Keyword(s):  
High Energy ◽  
Nuclear Emulsions
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