Sanoisin että aika massiivista tehoa tyrkyllä:
Auroral Kilometric Radioionic Energy
A publication by the Center for Academic Publication in Tokyo, Japan, Magnetospheric
Plasma Physics, edited by Atsuhiro Nishida, brings together some prominent world
physicists for a very clear picture of their
Earth energy model, along with their complex mathematics for the model. The conducting ionosphere causes instability of this Earth energy model by short circuiting the ions in the
Earth electric field.
Auroral displays
result in a process called ‘ring currents,’ which occurs along magnetic field lines that connect the
magnetotail with the ionosphere. This is the primary supply of energy for the aurora.
The process studied releases a radiation that is being called “Auroral Kilometric radiation(AKR)”
from a round 50 to 500 KHz.
Auroral arcs are generated by convection currents formed in the plasma of the magneto tail. These arcs curve toward the Earth on the night side, enter and generate
the aurora field at around 68 degrees latitude between 22 and 24 hours local time. The AKR
has a frequency spectrum from around 30 to 500 KHz,
with a peak power at around 200 KHz. The total power is about
1,000 Megawatts. It originates
at a low altitude, less than three Earth radii, with a radiation power of about one per cent of
the energy dissipation of the auroral particles. It appears that the ionizing wave front
stimulates the ionosphere, thus allowing the influx of the powerful AKR energies. Very
strong electrostatic waves have been monitored, between 17.8 and 100 KHz.
with the greatest amplitude at around 31.1 KHz.
Some of these same frequencies have been observed by the
Voyager II when it passed the magnetospheres of Jupiter and Saturn.
linkissä:
http://www.radio-ionics.com/pdf/Ion%20Valves%20v1.3.pdf