EXPERIMENTAL EXPERIENCE IN STUDYING THE WEIGHT DYNAMICS OF ROTATING GYROSCOPES AND THEIR ROTATION FEATURES AT CRITICALLY LOW SPEEDS, INCLUDING AT SUNRISE AND DURING A LUNAR-SOLAR ECLIPSE
The cycle of experiments with free-rolling gyroscopes at different angular velocity intervals including those on scales with continuous-discrete weight registration was carried out. We concluded that the free-running time of gyroscopes in one interval of angular velocities can vary greatly (within hundreds of percent). Measuring the free running time of a gyroscope during a solar eclipse has shown a connection between registered fluctuations in the gyroscope behavior and the eclipse stroke. The data obtained during the periods of sunrise indicate that the gyroscope can react at the moment of the sunrise while recording the true ascent, as well as the ascent preceding the true one with a difference of 8 minutes. Statistical analysis of the graphs of weight changes of the disk at right and left-hand free rotation in the speed range from 5000 to 250 rpm showed that the abnormal weight changes recorded at certain “critical” frequencies with different directions of rotation reliably differ in amplitude characteristics.