scholarly journals Application of Desensitized Nuclear Emulsion films for Chemical Composition Study of Cosmic-ray Nuclei in GRAINE 2018 balloon-borne experiment

2021 ◽  
Author(s):  
Atsushi Iyono
1991 ◽  
Vol 126 ◽  
pp. 433-436
Author(s):  
Kunitomo Sakurai

AbstractThe chemical composition of galactic cosmic rays in their sources is similar to that of interstellar clouds or grains which are relatively enriched in refractory and siderophile elements as compared with the chemical composition of the solar atmosphere. Taking into account this fact, it is shown that the cosmic ray source matter can be identified as the dust or grains observed in the envelopes of red supergiant stars or the matter originally ejected from supernova explosions.


1981 ◽  
Vol 94 ◽  
pp. 33-34
Author(s):  
C. J. Waddington ◽  
P. S. Freier ◽  
R. K. Fickle ◽  
N. R. Brewster

We are reporting here on the results obtained from a balloon exposure of a cosmic ray detector flown in 1977. This detector, described elsewhere, Gilman and Waddington (1975), Young (1979), measures elemental charge from scintillation and Cherenkov signals and mass from Cherenkov and total energy determined from a measure of residual range in nuclear emulsion. The charge resolution obtained ranged from 0.19 to 0.21 charge units between neon and nickel. This resolution was sufficient to ensure that all but a few percent of the nuclei were correctly identified, even for those elements of low abundance that have neighbors with high abundances, such as Cl or Al. The mass resolution obtained for those nuclei that stopped in the emulsions ranged from 0.40 to 0.70 amu for A between 20 and 60 amu. This was not adequate to uniquely resolve neighboring mass peaks in many cases, but was adequate to draw a number of conclusions regarding many of the more abundant elements.


Open Physics ◽  
2019 ◽  
Vol 17 (1) ◽  
pp. 233-240 ◽  
Author(s):  
M.C. Montesi ◽  
A. Lauria ◽  
A. Alexandrov ◽  
L. Alunni Solestizi ◽  
Ambrosi Giovanni ◽  
...  

Abstract In hadron therapy, the accelerated ions, interacting with the body of the patient, cause the fragmentation of both projectile and target nuclei. The fragments interact with the human tissues depositing energy both in the entrance channel and in the volume surrounding the tumor. The knowledge of the fragments features is crucial to determine the energy amount deposited in the human body, and - hence - the damage to the organs and to the tissues around the tumor target. The FOOT (FragmentatiOn Of Target) experiment aims at studying the fragmentation induced by the interaction of a proton beam (150-250 MeV/n) inside the human body. The FOOT detector includes an electronic setup for the identification of Z ≥ 3 fragments integrated with an emulsion spectrometer to measure Z ≤ 3 fragments. Charge identification by nuclear emulsions is based on the development of techniques of controlled fading of the particle tracks inside the nuclear emulsion, that extend the dynamical range of the films developed for the tracking of minimum ionising particles. The controlled fading strongly depends on temperature, relative humidity and treatment duration. In this study the performances in terms of charge separation of proton, helium and carbon particles, obtained on a batch of new emulsion films produced in Japan are reported.


1954 ◽  
Vol 32 (8) ◽  
pp. 538-554 ◽  
Author(s):  
Pierre Demers

The preparation of a silver bromide emulsion in the form of baseless sheets and their use in thick homogeneous stacks are described. In these sheets, a suitable development brings out minimum ionization tracks with a grain diameter 0.1 to 0.2 μ, and a linear grain density of 15 per 100 μ. The sequence of observations which led to the positive identification of minimum tracks is discussed. Short recoils and delta rays are visible, and excellent discrimination is available at all ionizing powers. The influence of grain size on fog is analyzed.Several cosmic ray phenomena containing minimum tracks are presented: single tracks, hard showers, πμe events, and an electron pair. Distortion is very small, and it is shown that the small grain size renders feasible better scattering measurements on higher energy particles. With this emulsion, nearly every possible measurement should become feasible with greater accuracy.


2000 ◽  
Vol 35 (3) ◽  
pp. 617-628 ◽  
Author(s):  
Dario TERRIBILINI ◽  
Otto EUGSTER ◽  
David W. MITTLEFEHLDT ◽  
Larryn W. DIAMOND ◽  
Stephan VOGT ◽  
...  

2007 ◽  
Author(s):  
Z. I. Goryaynova ◽  
M. V. Frontasyeva ◽  
D. F. Pavlov ◽  
S. Pankratova ◽  
Carlos Granja ◽  
...  

2009 ◽  
Vol 5 (S265) ◽  
pp. 376-377
Author(s):  
Edita Stonkutė ◽  
Birgitta Nordström ◽  
Gražina Tautvaišienė

AbstractFrom high resolution spectra taken with the spectrograph FIES on the Nordic Optical Telescope, La Palma, we measure abundances of oxygen and α-elements in order to characterize stars which from their dynamical properties are suspected to have originated in disrupted satellites. We find that the chemical composition of investigated stars is homogeneous and distinct from Galactic disk dwarfs, which is providing further evidence of their extragalactic origin.


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