Solar Gamma Ray and neutron observations

Solar Gamma Ray and neutron observations PDF Author: E. L. Chupp
Publisher:
ISBN:
Category :
Languages : de
Pages : 23

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Book Description

Solar Gamma Ray and neutron observations

Solar Gamma Ray and neutron observations PDF Author: E. L. Chupp
Publisher:
ISBN:
Category :
Languages : de
Pages : 23

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Book Description


Solar Gamma Ray and Neutron Observations

Solar Gamma Ray and Neutron Observations PDF Author: E. L. Chupp
Publisher:
ISBN:
Category :
Languages : en
Pages : 23

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Book Description


Solar Neutrons and Related Phenomena

Solar Neutrons and Related Phenomena PDF Author: Lev Dorman
Publisher: Springer
ISBN: 9789048137565
Category : Science
Languages : en
Pages : 873

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Book Description
Short Historical Overview In the 1940s, two phenomena in the ?eld of cosmic rays (CR) forced scientists to think that the Sun is a powerful source of high-energy particles. One of these was discovered because of the daily solar variation of CR, which the maximum number of CR observed near noon (referring to the existence of continuous ?ux of CR from the direction of the Sun); this became the experimental basis of the theory that CR’s ́ originate from the Sun (or, for that matter, from within the solar system) (Alfven 1954). The second phenomenon was discovered when large ?uxes of high energy particles were detected from several solar ?ares, or solar CR. These are the - called ground level events (GLE), and were ?rst observed by ionization chambers shielded by 10 cm Pb (and detected mainly from the secondary muon-component CR that they caused) during the events of the 28th of February 1942, the 7th of March 1942, the 25th of July 1946, and the 19th of November 1949. The biggest such event was detected on the 23rd of February 1956 (see the detailed description in Chapters X and XI of Dorman, M1957). The ?rst phenomenon was investigated in detail in Dorman (M1957), by ?rst correcting experimental data on muon temperature effects and then by using coupling functions to determine the change in particle energy caused by the solar-diurnal CR variation.

X-ray and Gamma-ray Observations of Solar Flares

X-ray and Gamma-ray Observations of Solar Flares PDF Author: Paul Thomas Feffer
Publisher:
ISBN:
Category :
Languages : en
Pages : 332

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Remote Compositional Analysis

Remote Compositional Analysis PDF Author: Janice L. Bishop
Publisher: Cambridge University Press
ISBN: 110718620X
Category : Language Arts & Disciplines
Languages : en
Pages : 655

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Book Description
Comprehensive overview of the spectroscopic, mineralogical, and geochemical techniques used in planetary remote sensing.

Solar Gamma-, X-, and EUV Radiation

Solar Gamma-, X-, and EUV Radiation PDF Author: S.R. Kane
Publisher: Springer Science & Business Media
ISBN: 9401018022
Category : Science
Languages : en
Pages : 424

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Book Description
Proceedings of IAU Symposium No. 68 held in Buenos Aires, Argentina, 11-14 June 1974, organized by the IAU in co-operation with COSPAR

Evidence for Extended Neutron and Gamma-Ray Generation During Two Solar Flares

Evidence for Extended Neutron and Gamma-Ray Generation During Two Solar Flares PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 5

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Book Description
High energy solar gamma-rays and neutrons were observed by spacecraft experiments during the major solar flares on 24 May 1990 and 15 June 1991. Both these flares were also associated with relativistic solar protons measured by ground-based neutron monitors. The integrated analysis of intensity-time profiles of different radiations and particles during these events gives evidence for extended neutron and gamma-ray generation during these solar flares.

Solar Cosmic Rays

Solar Cosmic Rays PDF Author: L.I. Miroshnichenko
Publisher: Springer Science & Business Media
ISBN: 9401596468
Category : Science
Languages : en
Pages : 489

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Book Description
It turned out to be really a rare and happy occasion that we know exact1y when and how a new branch of space physics was born, namely, a physics of solar cosmic rays. It happened on February 28 and March 7, 1942 when the fIrst "cosmic ray bursts" were recorded on the Earth, and the Sun was unambiguously identifIed for the fIrst time as the source of high-velocity 10 particles with energies up to > 10 eV. Just due to such a high energy these relativistic particles have been called "solar cosmic rays" (SCR), in distinction from the "true" cosmic rays of galactic origin. Between 1942 and the beginning ofthe space era in 1957 only extremely high energy solar particle events could be occasionally recorded by cosmic ray ground-Ievel detectors and balloon borne sensors. Since then the detection techniques varied considerably and the study of SCR turned into essential part of solar and solar-terrestrial physics.

Gamma-ray Bursts

Gamma-ray Bursts PDF Author: Cheng Ho
Publisher: Cambridge University Press
ISBN: 9780521414494
Category : Nature
Languages : en
Pages : 532

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Book Description
Summarizes the current understanding of Astronomical gamma-ray bursts, short-lived flashes of high-energy radiation, which have eluded even a basic explanation for over twenty years, and describes directions for future research.

Nuclear Planetary Science: Planetary Science Based On Gamma-ray, Neutron And X-ray Spectroscopy

Nuclear Planetary Science: Planetary Science Based On Gamma-ray, Neutron And X-ray Spectroscopy PDF Author: Nobuyuki Hasebe
Publisher: World Scientific
ISBN: 9813209720
Category : Science
Languages : en
Pages : 181

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Book Description
Nuclear planetary science has come to play an important role in our understanding of the origin and evolution of the planetary bodies in our solar system. A newly established branch of planetary science, its study aids in humankind's exploration of the present states of the structures of various planetary bodies (including the Earth), their atmospheres and their satellites, as well as small celestial bodies (e.g. asteroids), through direct observation. Knowing the elemental composition of the planetary bodies is essential in order to understand the formation and evolution of planetary bodies — just as important as it is to know the mass, radius, density and orbit of the celestial body.Suitable for students and specialists interested in the much wider field of Earth and Planetary Science, topics related to the planets and asteroids in the solar system are dealt with in this book. Techniques related to nuclear planetary science's nuclear cosmochemical and geological methods are also covered in this book.