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Studies of the Chemical Composition of Cosmic Rays with Z

Studies of the Chemical Composition of Cosmic Rays with Z PDF Author: William Rex Webber
Publisher:
ISBN:
Category : Cosmic rays
Languages : en
Pages : 80

Book Description


Studies of the Chemical Composition of Cosmic Rays with Z

Studies of the Chemical Composition of Cosmic Rays with Z PDF Author: William Rex Webber
Publisher:
ISBN:
Category : Cosmic rays
Languages : en
Pages : 80

Book Description


A Study of the Chemical Composition of Primary Cosmic Rays at 1015eV.

A Study of the Chemical Composition of Primary Cosmic Rays at 1015eV. PDF Author: Saul Alan Rappaport
Publisher:
ISBN:
Category :
Languages : en
Pages : 232

Book Description


Origin of Cosmic Rays

Origin of Cosmic Rays PDF Author: Vitaliĭ Lazarevich Ginzburg
Publisher:
ISBN:
Category :
Languages : en
Pages : 62

Book Description


Kosmische Strahlung II / Cosmic Rays II

Kosmische Strahlung II / Cosmic Rays II PDF Author: K. Sitte
Publisher: Springer Science & Business Media
ISBN: 3642460798
Category : Science
Languages : en
Pages : 662

Book Description


Nuclear Science Abstracts

Nuclear Science Abstracts PDF Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 1058

Book Description


The Advanced Composition Explorer Mission

The Advanced Composition Explorer Mission PDF Author: C.T. Russell
Publisher: Springer Science & Business Media
ISBN: 9401147620
Category : Science
Languages : en
Pages : 667

Book Description
NASA's Advanced Composition Explorer (ACE) was launched on August 25, 1997, carrying six high-resolution spectrometers that measure the abundances of the elements, isotopes, and ionic charge states of energetic nuclei in space. Data from these instruments is being used to measure and compare the composition of the solar corona, the nearby interstellar medium, and cosmic-ray sources in the Galaxy, and to study particle acceleration processes in a variety of environments. ACE also includes three instruments that monitor solar wind and energetic particle activity near the inner Lagrangian point, "1.5 million kilometers sunward of Earth, and provide continuous, real-time data to NOAA for use in forecasting space weather. Eleven of the articles in this volume review scientific progress and outline questions that ACE will address in solar, space-plasma, and cosmic-ray physics. Other articles describe the ACE spacecraft, the real-time solar-wind system, and the instruments used to measure energetic particle composition.

The Chemical Composition of Cosmic Rays

The Chemical Composition of Cosmic Rays PDF Author: Lawrence Hugh Aller
Publisher:
ISBN:
Category :
Languages : en
Pages : 7

Book Description


Composition and Origin of Cosmic Rays

Composition and Origin of Cosmic Rays PDF Author: M.M. Shapiro
Publisher: Springer Science & Business Media
ISBN: 9400971664
Category : Science
Languages : en
Pages : 419

Book Description
Proceedings of the NATO Advanced Study Institute, Ettore Majorana Centre, Erice, Sicily, Italy, June 20-30, 1982

Cosmic Rays in the Earth’s Atmosphere and Underground

Cosmic Rays in the Earth’s Atmosphere and Underground PDF Author: Lev Dorman
Publisher: Springer Science & Business Media
ISBN: 1402021135
Category : Science
Languages : en
Pages : 891

Book Description
The present monograph as well as the next one (Dorman, M2005) is a result of more than 50 years working in cosmic ray (CR) research. After graduation in December 1950 Moscow Lomonosov State University (Nuclear and Elementary Particle Physics Division, the Team of Theoretical Physics), my supervisor Professor D. I. Blokhintsev planned for me, as a winner of a Red Diploma, to continue my education as an aspirant (a graduate student) to prepare for Ph. D. in his very secret Object in the framework of what was in those time called the Atomic Problem. To my regret the KGB withheld permission, and I, together with other Jewish students who had graduated Nuclear Divisions of Moscow and Leningrad Universities and Institutes, were faced with a real prospect of being without any work. It was our good fortune that at that time there was being brought into being the new Cosmic Ray Project (what at that time was also very secret, but not as secret as the Atomic Problem), and after some time we were directed to work on this Project. It was organized and headed by Prof. S. N. Vernov (President of All-Union Section of Cosmic Rays) and Prof. N. V. Pushkov (Director of IZMIRAN); Prof. E. L. Feinberg headed the theoretical part of the Project.

Chemical Composition of Primary Cosmic Rays with IceCube

Chemical Composition of Primary Cosmic Rays with IceCube PDF Author: Chen Xu
Publisher:
ISBN: 9781267249647
Category : Cosmic rays
Languages : en
Pages :

Book Description
Ground detector arrays have been used to measure high energy cosmic rays for decades to overcome their very low rate. IceCube is a special case with its 3D deployment and unique location--the South Pole. Although all 86 strings and 81 stations of IceCube were completed in 2011, IceCube began to take data in 2006, after the completion of the first 9 strings. In this thesis, experimental data taken in 2009 with 59 strings are used for composition analysis albeit some techniques are illustrated with the 40-string data. Simulation is essential in the composition work. Simulated data must be compared against the experimental data to find the right mix of cosmic ray components. However, because of limited computing resources and complexities of cosmic rays, the simulation in IceCube is well behind the experiment. The lower and upper bounds of primary energy in simulation for events that go through IceTop and the deep arrays of IceCube are 10 14 e V and 1017 e V. However, since IceCube has a threshold energy about several hundred TeV, and an upper limit of 10 18 e V, the full energy range cannot be explored in this thesis. The approach taken to the composition problem in this thesis is a 2D Bayesian unfolding. It takes account of the measured IceTop and InIce energy spectrum and outputs the expected primary energy spectrum of different mass components. Studies of the uncertainties in the results are not complete because of limited simulation and understanding of the new detector and South Pole environment.