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Indications of Proton-Dominated Cosmic Ray Composition above 1.6 EeV
We report studies of ultra-high energy cosmic ray composition via analysis of depth of airshower maximum (Xmax), for airshower events collected by the High Resolution Fly's Eye (HiRes) observatory. Th...
View Book →Cosmic ray composition measurements and cosmic ray background free gamma-ray observations with Chere
Muon component of extensive air showers (EAS) initiated by cosmic ray particles carries information on the primary particle identity. We show that the muon content of EAS could be measured in a broad ...
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Haptics: Science, Technology, Applications
12th International Conference, EuroHaptics 2020, Leiden, The Netherlands, September 6–9, 2020, Proceedings...
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NASA Technical Reports Server (NTRS) 19930013000: Finite element analysis of a composite artificial
Ultra-light carbon fiber composite materials are being utilized in artificial limbs with increasing frequency in recent years. Dr. Arthur Copes, an orthotist from Baton Rouge, Louisiana, has developed...
View Book →A composition dependent energy scale and the determination of the cosmic ray primary mass in the ank
At present there are still several open questions about the origin of the ultra high energy cosmic rays. However, great progress in this area has been made in recent years due to the data collected by...
View Book →Evidence for a mixed mass composition at the `ankle' in the cosmic-ray spectrum
We report a first measurement for ultra-high energy cosmic rays of the correlation between the depth of shower maximum and the signal in the water Cherenkov stations of air-showers registered simultan...
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Vessel Health and Preservation: The Right Approach for Vascular Access
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View Book →Propagation and Chemical Composition of Ultra High Energy Cosmic Rays
Extragalactic cosmic ray protons with an injection spectrum of the type $E^{-2.7}$ show a spectrum on earth with a dip due to the Bethe-Heitler pair production against the photons of the cosmic microw...
View Book →CIA Reading Room cia-rdp83m00914r002900130016-4: DDCI QUESTION ON JACK ANDERSON COLUMN
Approved For Release 2007/06/14: CIA-RDP83M00914R002900130016-4 Approved For Release 2007/06/14: CIA-RDP83M00914R002900130016-4 Approved For Release 2007/06/14: CIA-RDP83M00914R002900130016-4 17 Febru...
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High Resolution Imaging in Microscopy and Ophthalmology
New Frontiers in Biomedical Optics...
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Optics in Our Time
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View Book →Cosmic ray spectral hardening due to dispersion in the source injection spectra
Recent cosmic ray (CR) experiments discovered that the CR spectra experience a remarkable hardening for rigidity above several hundred GV. We propose that this is caused by the superposition of the CR...
View Book →Cosmic ray spectral hardening due to dispersion of source injection spectra
The cosmic ray (CR) energy spectra measured with ATIC, CREAM and PAMELA showed that there is remarkable hardening for rigidity of several hundred GV. We propose that this hardening is due to the super...
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Pragmatic Philanthropy
Asian Charity Explained...
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Cardiovascular Biomechanics
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Melting Hadrons, Boiling Quarks - From Hagedorn Temperature to Ultra-Relativistic Heavy-Ion Collisio
With a Tribute to Rolf Hagedorn...
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Diseases of the Chest, Breast, Heart and Vessels 2019-2022
Diagnostic and Interventional Imaging...
View Book →The origin of cosmic rays at all energies
There is mounting evidence from observations of long duration gamma ray bursts (GRBs), supernova remnants (SNR) and the supernova (SN) explosion 1987A, that SN explosions eject highly relativistic bip...
View Book →What Would Be The Most Hardcore Strength & Con ( 4)
"What would be the most hardcore strength & conditioning routine imaginabLe? Answer Images Videos Sources The BEST Strength & Conditioning Workout The #1 Full Body Routine to Build Muscle and Lose Fat...
View Book →The foot in multistage ultra-marathon runners: experience in a cohort study of 22 participants of th
This article is from BMJ Open , volume 2 . Abstract Objectives: 67 runners participated in the Trans Europe FootRace 2009 (TEFR09), a 4487 km (2789 mi) multistage ultra-marathon covering the south o...
View Book →Cosmic Rays: The Second Knee and Beyond
We conduct a review of experimental results on Ultra-High Energy Cosmic Rays (UHECR's) including measurements of the features of the spectrum, the composition of the primary particle flux and the sear...
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Diseases of the Abdomen and Pelvis 2018-2021
Diagnostic Imaging - IDKD Book...
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Marginality
Addressing the Nexus of Poverty, Exclusion and Ecology...
View Book →Extragalactic Sources for Ultra High Energy Cosmic Ray Nuclei
In this article we examine the hypothesis that the highest energy cosmic rays are complex nuclei from extragalactic sources. Under reasonable physical assumptions, we show that the nearby metally rich...
View Book →Comparing the energy spectra of ultra-high energy cosmic rays measured with EAS arrays
The energy spectra of ultra-high energy cosmic rays (CRs) measured with giant extensive air shower (EAS) arrays exhibit discrepancies between the flux intensities and/or estimated CR energies exceedin...
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Magnetized Sources of Ultra-high Energy Nuclei and Extragalactic Origin of the Ankle
It has recently been suggested that ultra-high energy cosmic rays could have an extragalactic origin down to the "second knee" at ~4x10^{17}eV. In this case the "ankle" or "dip" at ~5x10^{18}eV would ...
View Book →A Soft Interaction Model at Ultra High Energies: Amplitudes, Cross Sections and Survival Probabiliti
In this paper we present a two channel model with the goal of reproducing the soft scattering data available in the ISR-Tevatron energy range, and extend the model results to LHC and Cosmic Rays energ...
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Modern Web Development on the JAMstack
Modern Techniques for Ultra Fast Sites and Web Applications...
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Medical Imaging Systems
An Introductory Guide...
View Book →Galactic gamma-ray bursters - an alternative source of cosmic rays at all energies
We propose a new hypothesis for the origin of the major part of non-solar hadronic cosmic rays (CRs) at all energies: highly relativistic, narrowly collimated jets from the birth or collapse of neutro...
View Book →Ultra High Energy Comic Rays in the Cosmic Microwave Background
We consider the propagation of ultra high energy cosmic rays (UHECR), for energies greater than E > 10^{14} eV but less than E < 10^{26} eV, in the cosmic medium of the Cosmic Microwave Background (CM...
View Book →Ultra-high energy cosmic rays from Quark Novae
We explore acceleration of ions in the Quark Nova (QN) scenario, where a neutron star experiences an explosive phase transition into a quark star (born in the propeller regime). In this picture, two c...
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