scholarly journals High‐altitude polar NM with the new DAQ system as a tool to study details of the cosmic‐ray induced nucleonic cascade

Author(s):  
Markus Similä ◽  
Ilya Usoskin ◽  
Stepan Poluianov ◽  
Alexander Mishev ◽  
Gennady A. Kovaltsov ◽  
...  
Keyword(s):  

Cosmic ray measurements on mountains are limited in general to altitudes below about 4000 meters. Above this height Regener has made successful use of small balloons carrying self-recording apparatus, and occasional flights have been made with manned balloons by Piccard, Cosyns, and by American workers. Balloon experiments are, however, hardly practicable in this country, so we decided to investigate cosmic rays, and in particular the production of showers, using an aeroplane. Facilities for flying to a height of about 10 km. Were generously provided by the Air Ministry. Apparatus Two independent sets of three tube counters were used in conjunction with the usual coincidence counting circuits. The counters could be arranged in a vertical line to record vertical penetrating particles, or in a triangle to record showers. The triple coincidences were recorded by telephone counters which were photographed at intervals together with a clock and aneroid barometer. The detailed design of the apparatus required some consideration since the aeroplane available (the Vickers Vespa machine used for high altitude experiments at the Royal Aircraft Establishment) had an open observer’s cockpit in which the counting set had to be installed.


1933 ◽  
Vol 44 (4) ◽  
pp. 246-252 ◽  
Author(s):  
I. S. Bowen ◽  
R. A. Millikan ◽  
H. V. Neher

2019 ◽  
Vol 208 ◽  
pp. 14001
Author(s):  
H. León Vargas

The HAWC (High Altitude Water Cherenkov) observatory, located on the slopes of the Sierra Negra volcano in the state of Puebla, Mexico, was designed with the goal of detecting gamma-rays in the Teraelectron- volt energy range. However, most of the air showers that are detected with the observatory, with a rate of ≈ 27 kHz, are of hadronic origin. This makes that, after three years of operations, HAWC has accumulated a very large data set that allows to perform cosmic-ray analysis of high precision. The details of the observatory operation, as well as a selection of recent results in cosmic-ray physics are discussed in this work.


2013 ◽  
Vol 60 (4) ◽  
pp. 2418-2426 ◽  
Author(s):  
G. Hubert ◽  
R. Velazco ◽  
C. Federico ◽  
A. Cheminet ◽  
C. Silva-Cardenas ◽  
...  
Keyword(s):  

2017 ◽  
Vol 32 (32) ◽  
pp. 1730027
Author(s):  
Yifang Wang

Particle and astroparticle physics activities in China can be classified into four major categories: accelerator-based experiments, underground experiments, cosmic-ray physics at high altitude, and space experiments. An overview of these experiments and their future perspectives are presented.


2012 ◽  
Vol 10 ◽  
pp. 147-158 ◽  
Author(s):  
◽  
MIN ZHA

The ARGO-YBJ detector, a RPC carpet array at the high altitude of 4300 m has been stably operated since 2007. As a multi-purpose experiment the physics topics of ARGO-YBJ covers the VHE gamma-ray astronomy, cosmic ray physics and solar physics. Results of these experimental studies are reviewed. And as a future extension project, the Large High Altitude Air Shower Observatory (LHAASO) is introduced, some research and development of detectors are described.


Radiocarbon ◽  
1992 ◽  
Vol 34 (3) ◽  
pp. 737-744 ◽  
Author(s):  
A. J. T. Jull ◽  
Amy E. Wilson ◽  
George S. Burr ◽  
Laurence J. Toolin ◽  
Douglas J. Donahue

The production of radioisotopes at the Earth's surface by cosmic-ray effects has been discussed for many years. Only in the past few years, with the higher sensitivity provided by accelerator mass spectrometry (AMS) in detecting 10Be, 26A1 and 36Cl, have the radioisotopes produced in this way been measured. We report here our measurements of cosmogenic 14C in terrestrial rocks at high altitude, and comparisons to other exposure-dating methods.


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