Gravitomagnetic explanation of cosmic phenomena without using computers. II. Streaming of plasma along field lines after an impact - even without any energy supply

Title:

Gravitomagnetic explanation of cosmic phenomena without using computers. II. Streaming of plasma along field lines after an impact - even without any energy supply

Creator:

Woyk (Chvojková), E.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:1e3e0533-9893-4d61-ae8d-fc0e591114cf
uuid:1e3e0533-9893-4d61-ae8d-fc0e591114cf

Subject:

astronomy, gravitomagnetic explanation, and cosmic phenomena

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

A particle path formula has been derived for charged particles spiralling in extended magnetic and gravity fields, In part I (Book 1, 3CS 1), a stationary dipole- like magnetic field has been considered in which particles of the highest energies slowly but continuousely diffuse up and fill the tops of very extended field lineš, while underescape charged paťticles diffuse down and separate from its top-trapped highTenergy part, Below an impact which squeezes the magnetic tubes the field strength H decreases less thon before or even grows with altitude r, in this region. Consequently the pitch angle of all down spiralling particles increases less now and vice versa; The plasma shifts down, it streams down even without having gained any energy surplus, The bottom of the Van Allen belt shifts down there and rises os Soon as the impact has ceased, This explains the oocurrence and disappearence of aurorae, When the H(r)-variation changes so that H=const is passed, without gravity the mag¬ netic mirror would immediately switch from the bottom on the top, In the gravity field first a "hole effect" gradually reverses the path - between H=const and r“^’ Phenomena occurring now apparently violate some basic physical laws.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

243-247

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:70

Harvested from:

CDK

Metadata only:

false