Zobrazeno 1 - 7
of 7
pro vyhledávání: '"H. V. Pinto"'
Publikováno v:
J Forensic Odontostomatol
Human identification using Forensic Dentistry occurs through comparative analysis of ante-mortem (AM) and post-mortem (PM) data. With the constant improvement of technology, photographs became a common source of AM data. When clinical dental records
Publikováno v:
Il Nuovo Cimento A. 105:1283-1290
The atmospheric diffusion of high-energy cosmic-ray hadrons induced by a single nucleus is calculated analytically under the assumption of three different types of cosmic-ray primary nuclei (proton, alpha and iron). We used the wounded model for nucl
Publikováno v:
Progress of Theoretical Physics. 88:53-62
pseudo·rapidity 5). It was found that for both parametrizations the inelasticity in pp collision decreases when energy increases and for proton· air nucleus the inelasticity has also a moderate decrease with the energy. However for proton· nucleus
Publikováno v:
Il Nuovo Cimento A. 104:1535-1544
In this work we use two differents procedures for mini-jet identification in cosmic-ray particle interaction with carbon target chamber (C-jets) observed by Brazil-Japan Collaboration. These events concern the overlapping energy region with CERN and
A photodensitometric method for determining the structure of cosmic ray showers in emulsion chambers
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms. 51:182-186
We describe a photodensitometric method for the study of the longitudinal and lateral development, as well as the energy determination, of high energy showers in an emulsion chamber. These showers are produced by the nuclear interaction of cosmic ray
Publikováno v:
Il Nuovo Cimento A. 99:619-624
Systematic analysis is made on cosmic-ray-induced atmospheric interactions detected by Brasil-Japan Collaboration on Chacaltaya Emulsion Chamber experiments to study the hadron multiple production. It is demonstrated that hadron-rich events are not c
Publikováno v:
Physical Review D. 40:2898-2902
Propagation of primary and secondary cosmic rays in the atmosphere is calculated analytically. Two different cases of primary-cosmic-ray composition are used: the first case assumes a mixed composition of very heavy, heavy, middle, and $\ensuremath{\