scholarly journals Very High Energy Particle Astronomy with All-Sky Survey High Resolution Air-Shower Detector (ASHRA)

2003 ◽  
Vol 151 ◽  
pp. 192-200 ◽  
Author(s):  
Makoto Sasaki
Keyword(s):  
High Resolution ◽  
High Energy ◽  
High Energy Particle ◽  
Energy Particle ◽  
Air Shower ◽  
Sky Survey ◽  
Very High Energy ◽  
Very High

Multiplicities in a QCD-motivated description of very high energy particle interactions

1986 ◽  
Vol 166 (2) ◽  
pp. 219-222 ◽  
Author(s):  
T.K. Gaisser ◽  
F. Halzen ◽  
A.D. Martin ◽  
C.J. Maxwell
Keyword(s):  
High Energy ◽  
High Energy Particle ◽  
Particle Interactions ◽  
Energy Particle ◽  
Very High Energy ◽  
Very High

Multiplicity in Very High-Energy Particle-Nucleus Collisions

1971 ◽  
Vol 3 (1) ◽  
pp. 238-242 ◽  
Author(s):  
Paul M. Fishbane ◽  
J. S. Trefil
Keyword(s):  
High Energy ◽  
High Energy Particle ◽  
Energy Particle ◽  
Very High Energy ◽  
Very High

scholarly journals Very-high-energy particle acceleration powered by the jets of the microquasar SS 433

Nature ◽  
2018 ◽  
Vol 562 (7725) ◽  
pp. 82-85 ◽  
Author(s):  
A. U. Abeysekara ◽  
A. Albert ◽  
R. Alfaro ◽  
C. Alvarez ◽  
J. D. Álvarez ◽  
...  
Keyword(s):  
Particle Acceleration ◽  
High Energy ◽  
High Energy Particle ◽  
Energy Particle ◽  
Ss 433 ◽  
Very High Energy ◽  
Very High

scholarly journals Publisher Correction: Very-high-energy particle acceleration powered by the jets of the microquasar SS 433

Nature ◽  
2018 ◽  
Vol 564 (7736) ◽  
pp. E38-E38
Author(s):  
A. U. Abeysekara ◽  
A. Albert ◽  
R. Alfaro ◽  
C. Alvarez ◽  
J. D. Álvarez ◽  
...  
Keyword(s):  
Particle Acceleration ◽  
High Energy ◽  
High Energy Particle ◽  
Energy Particle ◽  
Ss 433 ◽  
Very High Energy ◽  
Very High

scholarly journals High Energy γ-Rays from the Direction of the Crab Pulsar

1981 ◽  
Vol 94 ◽  
pp. 327-328
Author(s):  
T. Dzikowski ◽  
B. Grochalska ◽  
J. Gawin ◽  
J. Wdowczyk
Keyword(s):  
High Energy ◽  
Crab Pulsar ◽  
Muon Detector ◽  
Extensive Air Shower ◽  
Air Shower ◽  
Very High Energy ◽  
Γ Rays ◽  
Shower Array ◽  
Very High ◽  
Air Shower Array

A search has been made for very high energy photons from the direction of the Crab Pulsar using the Lodz extensive air shower array. This device is particularly suitable for such a study because it consists of a large muon detector which can be used to search for the characteristic muon poor showers.

Air shower Cerenkov radiation as an instrument for very high energy?-astronomy (I)

1993 ◽  
Vol 209 (1) ◽  
pp. 19-38 ◽  
Author(s):  
A. M. Anokhina ◽  
V. I. Galkin ◽  
K. V. Mandritskaya ◽  
T. M. Roganova
Keyword(s):  
High Energy ◽  
Cerenkov Radiation ◽  
Air Shower ◽  
Very High Energy ◽  
Very High

VERY HIGH ENERGY PARTICLE ASTRONOMY WITH ALL-SKY SURVER HIGH RESOLUTION AIR-SHOWER DETECTOR

2004 ◽  
Vol 19 (13n16) ◽  
pp. 1107-1115
Author(s):  
◽  
MOKOTO SASAKI
Keyword(s):  
Image Intensifier ◽  
High Energy ◽  
Image Sensor ◽  
High Energy Particle ◽  
Air Shower ◽  
Effective Aperture ◽  
Observational Station ◽  
Very High Energy ◽  
Air Fluorescence ◽  
Tev Gamma Rays

The Ashra detector consists of 3 observational stations installed on the grid of 30-40km distance on the mountains on the Hawaii Big Island, which ensures a large target mass for neutrinos and a large effective aperture for UHECR. An observational station is composed of 12 wide-angle high-precision telescopes, which can completely cover allsky view. In realizing the telescope design, we newly apply the following techniques matured in the other fields: 1) Baker-Nunn optics optimized to keep better than 1 arcmin. resolution in 50° field of view, 2) Electro-static lens image-intensifier tube (IIT) with the resolution matched with that of the above optics, 3) Gated IIT with a fast image shutter, and 4) CMOS image sensor which reads triggered images out of the above IIT. These novel techniques allow us an excellent opportunity for simultaneous observation of air fluorescence and Cerenkov lights with 1 arcmin. resolution in entirely all sky. This will open an interesting field, "Observational Particle Astronomy" by continuously observing TeV gamma-rays, VHE-neutrinos, Knee-CR, and EHECR with the energies from TeV to ZeV in all sky.

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