[PDF] Top 20 The future of the high energy cosmic ray detection: HERD
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The future of the high energy cosmic ray detection: HERD
... for high and low range IsCMOS cameras and the other one for the trigger ...maximum energy deposition in one crystal, calculated on simulation, is about 20 TeV which is created by a PeV hadronic ... See full document
7
Future Prospects for High Energy Polarimetry of Gamma‐Ray Bursts
... this energy range ...this energy band ...CdZnTe detection plane of the Swift BAT instrument [10] might make for a good polarimeter, but the packaging design of the detectors and the design of the ... See full document
6
Status of KM3NeT
... for high energy ...to high-energy neutrino ...larger detection area and better angular resolution, exploiting the optical characteristics of deep ...The detection of ... See full document
8
Abstract: The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to
... goals, detection techniques, wide cosmic-ray energy ranges, ...The high social and educational potential of the project gives confidence in its contributing to a progress in ... See full document
6
Performance of the SciBar cosmic ray telescope (SciCRT) toward the detection of high energy solar neutrons in solar cycle 24
... atmosphere, high- energy neutrons ( > 100 MeV) may be detected by ground- based ...at high-altitude moun- tains; several solar neutron events were observed (Sako et ...the energy of the ... See full document
8
Development of the radio astronomical method of cosmic particle detection for extremely high-energy cosmic ray physics and neutrino astronomy
... t,he zenith (corresponding to a declination around +55 ◦ ) and decreases in the other directions as Cos Z. Beginning from mid-2013 this radio telescope has been used for day by day monitoring, at 111 MHz, of the large ... See full document
6
Measurement of ultra-high energy cosmic rays: An experimental summary and prospects
... In order to exchange ideas and experiences for the next generation detector, it was agreed to form a new working group for future projects. The JEM/EUSO group also expressed an interest to join the working group. ... See full document
18
Proton-air and proton-proton cross sections
... cise cosmic ray data can be directly sensitive to hadronic cross ...improved detection resolu- tion in the current generation of cosmic ray experiments, at ultra-high energies, ... See full document
7
Measurements of the proton-air cross section with high energy cosmic ray experiments
... FD’s), future cross section results, using events from all three FDs will likely be ...with future versions of the high energy cosmic ray shower models is ... See full document
7
TAIGA - a hybrid array for high energy gamma astronomy and cosmic ray physics
... A detection of gamma rays is one of the most efficient ways of investigating of galactic and metagalactic sources of high-energy cosmic rays as well solving of many problems of astroparticle ... See full document
8
ATLAS and ultra high energy cosmic ray physics
... The ALFA detector (Absolute Luminosity For ATLAS) is designed to measure elastic proton (small-angle) scattering. Two tracking stations are placed on each side of the central ATLAS detector at distances of 238 m and 241 ... See full document
7
Detection of ultra-high energy cosmic ray air showers by Cosmic Ray Air Fluorescence Fresnel lens Telescope for next generation
... the future, ultra-high energy cosmic ray (UHECR) observatory will be expanded due to the small ...structure cosmic ray detector named as Cosmic Ray Air ... See full document
7
Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... limited energy resolution and other uncertainties connected to the detection of GeV neu- trinos will make such a detection strategy much more com- ...measured cosmic ray flux at Earth ... See full document
5
TeV Blazars as the Sources of Ultra High Energy Cosmic Rays
... to high energy gamma rays, and they show variability in flux at all wavelengths as well as spectral shape on time scales ranging from months to a few ...first detection of TeV gamma rays from Mkn 421 ... See full document
12
Constraints on high energy interaction models from LHC and cosmic ray data
... of high energy hadronic interactions is of considerable importance for experimental studies at the Large Hadron Collider (LHC) and, especially, in high energy cosmic ray (CR) ... See full document
10
Constraints on ultra-high-energy neutrino flux from radio observations of the Moon
... The next phase in the NuMoon experiment will be to use LOFAR, the Low Frequency Array (Falcke et al., 2006), that is under construction in the Netherlands and several other European countries. LOFAR is a network of ... See full document
5
Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... the cosmic ray energy spectrum at 3 PeV can be explained as a split between a radiation-dominated expansion and a matter-dominated expansion of an expanding heat ...that high energy ... See full document
5
Cosmic ray transport and anisotropies to high energies
... There is another source of information about a possible CR gradient, which would result in an anisotropy: the star forma- tion rate in the Galaxy strongly depends on radial distance from the Galactic Center (GC) (Smith ... See full document
6
Cosmic ray observations at high zenith angles
... for a compound telescope consisting of 30 sub-units h = 240 cmo For the given geometry of the high zenith angle telescope for a 30-fold increase of the high zenith angle count-rate the a[r] ... See full document
135
Highlights from HAWC
... The HAWC observatory is a second generation ground based instrument designed to characterize electromagnetic showers with high precision. This allows to obtain the best gamma / hadron rejection obtained so far for ... See full document
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