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  • 1
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    In:  Other Sources
    Publication Date: 2011-08-10
    Description: Cosmic ray produced iron 60 measurement in Odessa meteorite by counting daughter radionuclide cobalt 60, noting dating application
    Keywords: SPACE SCIENCES
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  • 2
    Publication Date: 2013-08-31
    Description: Parallel processing of real-time dynamic systems simulation on a multiprocessor system named OSCAR is presented. In the simulation of dynamic systems, generally, the same calculation are repeated every time step. However, we cannot apply to Do-all or the Do-across techniques for parallel processing of the simulation since there exist data dependencies from the end of an iteration to the beginning of the next iteration and furthermore data-input and data-output are required every sampling time period. Therefore, parallelism inside the calculation required for a single time step, or a large basic block which consists of arithmetic assignment statements, must be used. In the proposed method, near fine grain tasks, each of which consists of one or more floating point operations, are generated to extract the parallelism from the calculation and assigned to processors by using optimal static scheduling at compile time in order to reduce large run time overhead caused by the use of near fine grain tasks. The practicality of the scheme is demonstrated on OSCAR (Optimally SCheduled Advanced multiprocessoR) which has been developed to extract advantageous features of static scheduling algorithms to the maximum extent.
    Keywords: COMPUTER SYSTEMS
    Type: JPL, Proceedings of the 3rd Annual Conference on Aerospace Computational Control, Volume 1; p 170-183
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  • 3
    Publication Date: 2011-08-19
    Description: Measurements of concentrations of chlorofluoromethanes (CFMs), carbon dioxide and carbon isotope ratio in stratospheric and tropospheric air by grab-sampling systems are reported. The balloon-borne grab-sampling system has been launched from Sanriku Balloon Center three times since 1981. It consists of: (1) six sampling cylinders, (2) eight motor driven values, (3) control and monitor circuits, and (4) pressurized housing. Particular consideration is paid to the problem of contamination. Strict requirements are placed on the choice of materials and components, construction methods, cleaning techniques, vacuum integrity, and sampling procedures. An aluminum pressurized housing and a 4-m long inlet line are employed to prevent the sampling air from contamination by outgassing of sampling and control devices. The sampling is performed during the descent of the system. Vertical profiles of mixing ratios of CF2Cl2, CFCl3 and CH4 are given. Mixing ratios of CF2Cl2 and CFCl3 in the stratosphere do not show the discernible effect of the increase of those in the ground level background, and decrease with altitude. Decreasing rate of CFCl3 is larger than that of CF2Cl2. CH4 mixing ratio, on the other hand, shows diffusive equilibrium, as the photodissociation cross section of CH4 is small and concentrations of OH radical and 0(sup I D) are low.
    Keywords: GEOPHYSICS
    Type: International Council of Scientific Unions Handbook for MAP, Vol. 18; 7 p
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  • 4
    Publication Date: 2019-06-28
    Description: The data of optical Cerenkov light from extensive air shower observed at the core distance more than 1 Km at Akeno are reexamined. Applying the new simulated results, the shower development curves for the individual events were constructed. For the showers of 10 to 17th power eV the average depth at the shower maximum is determined to be 660 + or - 40 gcm/2. The shower curve of average development is found to be well described by a Gaisser-Hillas shower development function with above shower maximum depth.
    Keywords: SPACE RADIATION
    Type: HE-4.4-7 , 19th Intern. Cosmic Ray Conf - Vol. 7; p 171-174; NASA-CP-2376-VOL-7
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  • 5
    Publication Date: 2019-06-28
    Description: The cosmic ray propagation in the Galactic arm is simulated. The Galactic magnetic fields are known to go along with so called Galactic arms as a main structure with turbulences of the scale about 30pc. The distribution of cosmic ray in Galactic arm is studied. The escape time and the possible anisotropies caused by the arm structure are discussed.
    Keywords: SPACE RADIATION
    Type: OG-5.4-2 , 19th Intern. Cosmic Ray Conf - Vol. 2; p 276-279; NASA-CP-2376-VOL-2
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  • 6
    Publication Date: 2019-06-28
    Description: Anisotropy of cosmic rays is studied with extensive air showers (EAS) data by muon trigger. The present results support those obtained by electron trigger which suggest the significant anisotropy of second harmonics with phase around 100 deg in right ascension for showers of 10 to the 16th power - 10 to the 17th power eV, and predominant arrival direction of 230 deg in right ascension for muon-rich showers. It seems that the phase of the first harmonics in the energy range below 10 to the 11th power eV is about 300 deg in right ascension and the second harmonics near 6 x 10 to the 14th power eV is statistically significant with an amplitude of 0.39 + or - 0.13% in direction of 83 + or - 10 deg in right ascension.
    Keywords: SPACE RADIATION
    Type: OG-5.3-3 , 19th Intern. Cosmic Ray Conf - Vol. 2; p 242-245; NASA-CP-2376-VOL-2
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  • 7
    Publication Date: 2019-06-28
    Description: The properties of 10 to the 18th power - 10 to the 19th power eV EAS showers such as the electron lateral distribution, the muon lateral distribution ( 1Gev), the ratio of muon density to a electron density, the shower front structure and the transition effects in scintillator of 5cm thickness are investigated with the Akeno 4 sq km/20sq km array at far core distances between 500m and 3000m. The fluctuation of densities and arrival time increase rapidly at core distances greater than 2km.
    Keywords: SPACE RADIATION
    Type: HE-4.7-3 , 19th Intern. Cosmic Ray Conf - Vol. 7; p 320-323; NASA-CP-2376-VOL-7
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  • 8
    Publication Date: 2019-06-28
    Description: As the first stage of the future huge array, the Akeno air shower array was expanded to about 20 sq. km. by adding 19 scintillation detectors of 2.25 sq m area outside the present 1 sq. km. Akeno array with a new data collection system. These detectors are spaced about 1km from each other and connected by two optical fiber cables. This array has been in partial operation from 8th, Sep. 1984 and full operation from 20th, Dec. 1984. 20 sq m muon stations are planned to be set with 2km separation and one of them is now under construction. The origin of the highest energy cosmic rays is studied.
    Keywords: SPACE RADIATION
    Type: OG-9.4-8 , 19th Intern. Cosmic Ray Conf - Vol. 3; p 430-433; NASA-CP-2376-VOL-3
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  • 9
    Publication Date: 2019-06-28
    Description: The experimental data of extensive air showers observed at Akeno have been analyzed to detect the gamma ray signal from Cyg X-3. After muon poor air showers are selected, the correlation of data acquisition time with 4.8 hours X-ray period is studied, giving the data concentration near the phase 0.6, the time of X-ray maximum. The probability that uniform backgrounds create the distribution is 0.2%. The time averaged integral gamma ray flux is estimated as (1.1 + or - 0.4)x 10 to the -14th power cm(-2) sec(-1) for Eo 10 to the 15th power eV and (8.8 + or - 5.0)x 10 to the 14th power cm(-2) sec(-1) for Eo 6 x 10 to the 14th power eV.
    Keywords: SPACE RADIATION
    Type: OG-2.1-5 , 19th Intern. Cosmic Ray Conf - Vol. 1; p 67-70; NASA-CP-2376-VOL-1
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  • 10
    Publication Date: 2019-06-28
    Description: A search experiment for cosmic ray magnetic monopoles was performed by means of atomic induction mechanism by using He mixture gas proportional counters of the calorimeter (130 square meters sr) at the center of the Akeno air shower array. In 3,482 hours operation no monopole candidate was observed. The upper limit of the monopole flux is 1.44 x 10 to the minus 13th power cm-z, sec -1, sr-1 (90% C.L.) for the velocity faster than 7 x 0.0001 c.
    Keywords: SPACE RADIATION
    Type: HE-6.1-2 , 19th Intern. Cosmic Ray Conf - Vol. 8; p 218-221; NASA-CP-2376-VOL-8
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