๐”– Bobbio Scriptorium
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Electromagnetic acceleration of particles to cosmic ray energies

โœ Scribed by W.F.G. Swann


Publisher
Elsevier Science
Year
1956
Tongue
English
Weight
266 KB
Volume
261
Category
Article
ISSN
0016-0032

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๐Ÿ“œ SIMILAR VOLUMES


Processes involved in electromagnetic ac
โœ W.F.G. Swann ๐Ÿ“‚ Article ๐Ÿ“… 1960 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 419 KB

The paper extends ideas, put forward by the writer sonm twenty-five years ago, according to which charged particles could be accelerated to cosmic-ray energies through electromagnetic induction resulting from magnetic fields like those encountered in sunspots. The paper confines itself, for simplic

Acceleration of particles to cosmic ray
โœ W.F. Swann ๐Ÿ“‚ Article ๐Ÿ“… 1957 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 744 KB

It is clear that the.particle, starting from rest, will move initially so as to make an acute angle with the electric field, that is, with the vector -(l/c)(XJ/%). As long as it continues to move so as to make an \*A paper presented at the Symposium on Electromagnetic Phenomena in Cosmical Physics

Acceleration to cosmic ray energies by b
โœ W.F.G. Swann ๐Ÿ“‚ Article ๐Ÿ“… 1954 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 57 KB

In 1933, W. F. G. Swann suggested a mechanism according to which charged particles could acquire cosmic ray energies by what is now called "betatron action" in the stars. The original paper was based on rather abstract dynamical considerations, and while the validity of the conclusions is generally

A general approach to the electromagneti
โœ W.F.G. Swann ๐Ÿ“‚ Article ๐Ÿ“… 1962 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 233 KB

No piece of matter can, under ordinary circumstances, contain, in any form, enough energy to provide cosmic ray energies for its particles. However, by evolving a magnetic field, matter can provide a means by which a small amount of ionized matter shot from the region of the magnetic field can, by c