scholarly journals The energy spectrum of Telescope Array’s Middle Drum detector and the direct comparison to the High Resolution Fly’s Eye experiment

2012 ◽  
Vol 39-40 ◽  
pp. 109-119 ◽  
Author(s):  
T. Abu-Zayyad ◽  
R. Aida ◽  
M. Allen ◽  
R. Anderson ◽  
R. Azuma ◽  
...  
2001 ◽  
Vol 27 (7) ◽  
pp. 1611-1623
Author(s):  
Lawrence Wiencke ◽  
the HiRes Collaboration

2001 ◽  
Vol 16 (supp01c) ◽  
pp. 1019-1021
Author(s):  
JOHN BELZ

The High-Resolution Fly's Eye cosmic ray observatory has been operating in monocular (stereo) mode for about three years (one year), during which time we have observed extensive airshowers with an integrated aperture of ~ 1500 km2-sr-yr (~ 400 km-sr-yr) at 5×1019 eV. We describe the HiRes experiment and the nitrogen fluorescence technique, and present data taken in both monocular and stereo modes including preliminary energy spectra.


2006 ◽  
Vol 25 (1) ◽  
pp. 74-83 ◽  
Author(s):  
R ABBASI ◽  
T ABUZAYYAD ◽  
J AMANN ◽  
G ARCHBOLD ◽  
K BELOV ◽  
...  

Author(s):  
B. R. Petersen ◽  
D. M. Heim ◽  
J. B. Ghandhi

High-resolution planar laser-induced fluorescence and particle image velocimetry (PIV) measurements were acquired during the intake stroke in a motored engine to investigate the mixing behavior of in-cylinder flows. The data were analyzed to determine the scalar energy and kinetic energy spectra, which were used to find the corresponding dissipation spectra. The results were compared with a model turbulent spectrum. The scalar energy and scalar dissipation spectra were shown to be resolved through the full dissipation range, enabling the determination of the Batchelor/Kolmogorov length scale and agreed well with the model turbulent spectrum at all but the highest wavenumbers where the effects of random noise were present. The 2% point in the scalar dissipation spectra was used to estimate the Batchelor scale, which was found to be approximately 32 μm. The PIV data, which had a 675 μm interrogation region, were used to calculate a one-dimensional kinetic energy spectrum. The kinetic energy spectrum agreed well with the scalar energy spectrum and the model spectrum up to wavenumbers corresponding to approximately two times the PIV interrogation region size. For the present measurements, this meant that the PIV data were not able to resolve the peak in the dissipation spectrum, i.e., the full high-wavenumber part of the inertial subrange.


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