Aurora effect on the planet
This experiment continues the row of forbidden experiments. It describes the experiment when a measuring instrument on the Earth's surface becomes involved in measurements. In that case, an observer likes to detect the Aurora Effect on the planetary surface. He uses two atomic clocks located at points A and B. Some distance AB separates those points. The direction of AB has a casual orientation on the planetary surface in a general case. A similar experiment on the Earth's surface can be conducted in any lab. The following figure shows that case.
Earth Aurora Experiment
The figure schematically shows the Earth with two atomic clocks located on its surface at points A and B. The measuring channel connecting both clocks is shown as a straight line between them. Point N shows the North Pole, and point S shows the South Pole. Ex shows the Absolute Velocity Vector (AVV).
In that case, the measuring instrument that comprises both clocks and the measuring channel between them rotates with the planet because it is located motionlessly on the planet's surface. As a result, the measuring instrument makes one revolution in 24 hours according to the direction of the Sun and 23 hours 56 minutes according to the direction of any fixed star (sidereal rotation of the Earth).
According to the figure, the measuring instrument changes its orientation contentiously. Moreover, all those changes can be reduced by rotating the measuring instrument with fixed point A. In that case, the measuring instrument forms a measuring cone A1-B1-B2.
The projection of AVV on that cone gives a cross-section of the Aurora Ellipsoid. The following figure shows that case.
a Cross-section of the Aurora Ellipsoid
Z-C1 shows again the distance between points of measurement. The planet takes some orientation in the medium. The measuring signal leaves the first point of measurement in medium A and reaches the last point of measurement, E1, in the medium. That point coincides with the point R in the observer-bound reference frame. The measuring signal bounces back and returns to the first measurement point. The first point of measurement comes to point B in the medium at the time when the signal comes back. Therefore, every point of the measuring instrument covers the distance in the medium equal to AB during the round-trip propagation of the measuring signal.
The planet changes its orientation slowly with the measuring instrument mounted on it. Therefore, the last point of measurement (point R in the observer-bound reference frame) also changes its location in the medium, following the path E1-E2-D1-E3.
That path forms an ellipse that appears as a cross-section of the Aurora Ellipsoid by the plain of the measuring cone, as mentioned above. Observation of the figure leads to the following conclusion.
Every one-way measurement shows its duration, which depends on the planet's orientation.
Deviation of the duration of forward propagation of the measuring signal becomes ever compensated by deviation of backward propagation regarding some mean duration of signal propagation.
The duration of a round-trip experiment conducted by a measuring device located on the Earth's surface remains constant regardless of the orientation of the Earth (as a result of statements 1 and 2).
The duration of forward propagation never coincides with the duration of backward propagation.
- Allan Zade
Therefore, such an experiment does not allow the observer to see a situation when the duration of forward propagation coincides with the duration of backward propagation.
Moreover, the duration of signal propagation in one direction remains ever greater than the duration of signal propagation in the opposite direction. That situation led to a significant side effect that appeared in view during the greatest experiment ever conducted by humankind. Allan means the CERN faster-than-light neutrino experiment.
