The study of the Schumann Resonances is key in understanding the origin of the planets
In 2011, many researchers discovered that they could use the so-called “Electromagnetic Field Vector Instrument” of NASA that is mounted on modern satellites and aircraft, for the detection and monitoring of Schumann Resonances, so that it can be investigated in detail how the RS they affect the formation and configuration of the different planets of the Solar System.
Every second, various light beams travel the Earth's electromagnetic field. These flashes generate electromagnetic waves that surround the Earth, and have an impact on pulses located between the surface and the lower layers of the ionosphere. These pulses are known as Schumann Resonances, and are present in each and every one of the planets of our Solar System, and probably also in the planets satellites.
II.-New crucial discoveries for science that studies the origin of the cosmos: Schumann Resonances and Cosmogenesis.
In a study published in May 2012, in the Astrophysical Journal, researchers led by Fernando Simoes describe a new technique that could be used to understand the genesis of the Solar System. Certainly the Schumann Resonances play a key role in the formation of the planets of the Solar System. The key, says Simoes, is not only in the dependence of the RS on the size of the planets as previously thought, but on their composition and subsequent modifications in said composition. The reason, among others, is the presence of conductivity due to the exit of atoms and molecules of elements such as water, methane, oxygen and ammonium. The existence of these elements is related to the RS, once it has already been proven that the RS are present in the entire Solar system and not only on Earth as initially thought.
The novelty according to Simoes, implies the possibility of using these techniques of measurement of the RS to determine the atmosphere of all the planets of the Solar System in function of the detection of the Schumann resonances, something that could be done by incorporating these previously mentioned measuring devices into space probes and satellites.
Simoes suggests that the best way to determine it would be to activate these modules in the process of final entry of internment of satellites in the atmosphere of the planets, so that during the process prior to their destruction can be collected all the data corresponding to the RS of the atmosphere of these planets. In this way, the composition of the atmospheres could be known with great precision and not miss this opportunity in future space missions.
