scholarly journals Measurement Method of Ion-beam Relative Intensity Distribution Using γ-Ray Irradiation Response Function of Gafchromic Film HD-V2

RADIOISOTOPES ◽  
2017 ◽  
Vol 66 (7) ◽  
pp. 251-258
Author(s):  
Tomohisa Ishizaka ◽  
Yosuke Yuri ◽  
Takashi Agematsu ◽  
Takahiro Yuyama ◽  
Hajime Seito ◽  
...  
2015 ◽  
Vol 170 (7-8) ◽  
pp. 659-667
Author(s):  
Abha H. Oza ◽  
N.S. Dhoble ◽  
S.P. Lochab ◽  
S.J. Dhoble
Keyword(s):  
Ion Beam ◽  

Author(s):  
N. Piel ◽  
W.H. Schulte ◽  
M. Berheide ◽  
H.W. Becker ◽  
L. Borucki ◽  
...  

1995 ◽  
Vol 396 ◽  
Author(s):  
Seok-Keun Koh ◽  
Ki-Hwan Kim ◽  
Won-Kook Choi ◽  
Hong-Gui Jang ◽  
Young-Soo Yoon ◽  
...  

AbstractChanges of crystallinity and surface roughness are discussed in terms of the average energy per deposited atom in the partially ionized beam(PIB) deposition. The average energy per deposited atom can be controlled by adjusting the ionization potential, Vi and acceleration potential, Va. The ion beam consists of a Cu ion beam and residual gas ion beam and residual gases as well as Cu particles that were ionized and accelerated to provide the film with energy required for film-growth. The relative contribution of residual gas ions and Cu ions to total average energy per deposited atom was varied with the ionization potential. At fixed ionization potentials of Vi=400 V and Vi=450 V, the average energy per deposited atom was varied in the range of 0 to 120 eV with acceleration potential Va, of 0 to 4 kV. The relative intensity ratio, 1(111)/I(200), of the Cu films increased from 6 to 37 and the root mean square(Rms) surface roughness decreased with an increase in acceleration potential at Vi=400 V. The relative intensity ratio, I(lll)/I(200), of Cu films increased up to Va=2 kV at Vi=2 kV, above which a decrease occurred, and the surface roughness of Cu films increased as a funtion of acceleration potential. The degree of preferred orientation was closely related with the average energy per deposited atom. The change of Rms roughness might be affected by ion flux, particle energy and preferred orientation.


2020 ◽  
Vol 175 (5-6) ◽  
pp. 407-421 ◽  
Author(s):  
Chaitali M. Mehare ◽  
V. Chopra ◽  
Chandan Ghanty ◽  
N. S. Dhoble ◽  
S. J. Dhoble

1971 ◽  
Vol 49 (13) ◽  
pp. 1828-1832 ◽  
Author(s):  
A. M. Lopez ◽  
W. V. Prestwich ◽  
B. Arad

Radioactive 97Rh was produced via the 96Ru(p,γ)97Rh reaction. The two most intense lines in the γ-ray spectrum of 97Rh, at 190 and 421 keV, were observed to decay with half-lives of 40 ± 2 and 30 ± 2 min respectively. This result is interpreted as evidence for a 30 min isomeric state in 97Rh. The interpretation is further supported by the observation of the 19 keV Rh Kα X ray. With this interpretation it is possible to resolve a discrepancy in the observations of previous investigators as regards the relative intensity of the 190 and 421 keV transitions.


2005 ◽  
Vol 13 ◽  
pp. 18-23 ◽  
Author(s):  
A. Melatos

AbstractRecent calculations of the neutrino fluxes and spectra from pulsar magnetospheres and wind nebulae are reviewed. The neutrinos, produced in pp and pγ collisions via pion decays, are a signature of TeV ions accelerated electrostatically in the magnetosphere, in the wind termination shock (Fermi), or in the wind neutral sheet (wave surfing and/or reconnection). The fluxes and spectra are related to the energy and density of the accelerated ion beam and the densities of the target species, thereby constraining ion-loaded pulsar wind models originally developed to explain the variable wisps in pulsar-driven supernova remnants. The neutrino signal may be detectable by km2 telescopes (e.g. IceCube) and is correlated with TeV γ-ray emission. Related sources are also reviewed, such as early-phase post-supernova pulsar winds, pulsar-driven γ-ray-burst afterglows, and accreting neutron stars. The possibility of long baseline oscillation experiments, to search for fine splitting of neutrino mass eigenstates and non-radiative neutrino decays, is noted.


Luminescence ◽  
2015 ◽  
Vol 30 (7) ◽  
pp. 967-977 ◽  
Author(s):  
Abha H. Oza ◽  
N. S. Dhoble ◽  
S. P. Lochab ◽  
S. J. Dhoble

1972 ◽  
Vol 104 (2) ◽  
pp. 263-283 ◽  
Author(s):  
B.R. Erdal ◽  
G. Rudstam
Keyword(s):  

2012 ◽  
Vol 15 (4) ◽  
pp. 263-270
Author(s):  
Noritaka Chiyo ◽  
Yuji Komine ◽  
Yasuhiro Tanaka ◽  
Atsuhiro Nishikata ◽  
Takuichi Hirano ◽  
...  

Microscopy ◽  
2021 ◽  
Author(s):  
Ken Harada ◽  
Keiko Shimada ◽  
Yoshio Takahashi

Abstract We have developed an observation and measurement method for spatial electromagnetic fields by using scanning electron/ion microscopes, combined with electron holography reconstruction technique. A cross-grating was installed below the specimen, and the specimens were observed under the infocus condition, and the grating was simultaneously observed under the defocus condition. Electromagnetic fields around the specimen were estimated from grating-image distortions. This method is effective for low and middle magnification and resolution ranges; furthermore, this method can in principle be realizable in any electron/ion beam instruments because it is based on the Lorentz force model for charged particle beams. Mini Abstract We have developed a visualization technique for spatial electromagnetic fields by using scanning electron/ion microscopes, combined with electron holography reconstruction technique. A specimen and a cross-grating installed below the specimen were observed simultaneously. The distorted grating image caused by electromagnetic fields around the specimen were quantitatively measured and visualized.


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