Extraction of high-energy particle beams through the yoke of the synchrocyclotron magnet

Atomic Energy ◽  
1956 ◽  
Vol 1 (5) ◽  
pp. 667-671
Author(s):  
A. E. Ignatenko ◽  
V. V. Krivitsky ◽  
A. I. Mukhin ◽  
B. Pontecorvo ◽  
A. A. Reut ◽  
...  
Keyword(s):  
High Energy ◽  
High Energy Particle ◽  
Energy Particle ◽  
Particle Beams

scholarly journals Accelerators, Colliders and Their Application

2020 ◽  
pp. 1-14
Author(s):  
E. Wilson ◽  
B. J. Holzer
Keyword(s):  
High Precision ◽  
Broad Spectrum ◽  
Nuclear Physics ◽  
World Wide ◽  
High Energy ◽  
High Energy Particle ◽  
Medical Applications ◽  
Energy Particle ◽  
Particle Beams ◽  
Basic Physics

AbstractAccelerators are modern, high precision tools with applications in a broad spectrum that ranges from material treatment, isotope production for nuclear physics and medicine, probe analysis in industry and research, to the production of high energy particle beams in physics and astronomy. At present about 35,000 accelerators exist world-wide, the majority of them being used for industrial and medical applications. Originally however the design of accelerators arose from the request in basic physics research, namely to study the basic constituents of matter.

A lithium lens for axially symmetric focusing of high energy particle beams

1981 ◽  
Vol 190 (1) ◽  
pp. 9-14 ◽  
Author(s):  
B.F. Bayanov ◽  
J.N. Petrov ◽  
G.I. Sil'vestrov ◽  
J.A. Maclachlan ◽  
G.L. Nicholls
Keyword(s):  
High Energy ◽  
High Energy Particle ◽  
Axially Symmetric ◽  
Energy Particle ◽  
Particle Beams

scholarly journals Exploring the Origin of High-Energy Particle Beams in the Atmosphere

Eos ◽  
2014 ◽  
Vol 95 (46) ◽  
pp. 420-421
Author(s):  
Ashot A. Chilingarian
Keyword(s):  
High Energy ◽  
High Energy Particle ◽  
Energy Particle ◽  
Particle Beams

scholarly journals Sizes of flaring kernels in various parts of the Hα line profile

2008 ◽  
Vol 26 (10) ◽  
pp. 2991-2997 ◽  
Author(s):  
K. Radziszewski ◽  
P. Rudawy
Keyword(s):  
Line Profile ◽  
Solar Flares ◽  
Imaging System ◽  
High Energy ◽  
High Energy Particle ◽  
High Temporal Resolution ◽  
Energy Particle ◽  
Double Pass ◽  
Particle Beams ◽  
Very High

Abstract. In this paper we present new results of spectra-photometrical investigations of the flaring kernels' sizes and their intensities measured simultaneously in various parts of the Hα line profile. Our investigations were based on the very high temporal resolution spectral-imaging observations of the solar flares collected with Large Coronagraph (LC), Multi-channel Subtractive Double Pass Spectrograph and Solar Eclipse Coronal Imaging System (MSDP-SECIS) at Białkow Observatory (University of Wrocław, Poland). We have found that the areas of the investigated individual flaring kernels vary in time and in wavelengths, as well as the intensities and areas of the Hα flaring kernels decreased systematically when observed in consecutive wavelengths toward the wings of the Hα line. Our result could be explained as an effect of the cone-shaped lower parts of the magnetic loops channeling high energy particle beams exciting chromospheric plasma.

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