Science Reveals the Vibrational Nature of the Sun | Tracking Waves from Sunspots Gives New Solar Insight

(Stillness in the Storm Editor) The ancients have long said that vibration is a fundamental principle of the universe. Traditional physics cannot explain the mystery of why the Sun is hotter on the outside than it is on the inside because of the supposition that our stellar parent is a kind of internal combustion engine—using fusion and fission to burn up hydrogen and other lighter elements to produce energy and heat.

But Electric Universe theorists, along with many in the hidden fields of science operating under cover of government secrecy, suppose that the Sun is more akin to a sonoluminescent focal point. Like a hurricane, the Sun’s corona—the hottest part of our star—is the most turbulent and energetic, thus producing a significant amount of heat and ejecta.

But as one dives into the Sun’s heart, it cools and becomes less active—much like the eye of a hurricane has a point of relative stillness at the core of swirling outward flowing activity.

Ben Davidson is a solar watcher who ascribes to electric universe theories and says that the following article is a staggering shift from the mainstream view described above. And given the principle of correspondence expressed in natural law, it would stand to reason that the same type of energy dynamics we see on Earth also appears elsewhere in the cosmos—in this case on our sun.

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Sunspots are like earth-spots in that they act as a region of energetic flux organized by rotating, and therefore vibrational systems of motion. And the connections between solar activity, such as flares, coronal mass ejections, and coronal hole streams, play an intimate role in managing the Earth system, the daughter of our stellar father, Sol.

Science seems to be slowly realizing a much more coherent understanding with what the ancient world described as a universe made from a primal sound or vibration.

Related The Energetic Evolution of The Solar System | At the Earth’s Core: The Geophysics of Planetary Evolution

Source – Phys Org

by Phys Org Staff Writer, October 20th 2016

While it often seems unvarying from our viewpoint on Earth, the sun is constantly changing. Material courses through not only the star itself, but throughout its expansive atmosphere. Understanding the dance of this charged gas is a key part of better understanding our sun – how it heats up its atmosphere, how it creates a steady flow of solar wind streaming outward in all directions, and how magnetic fields twist and turn to create regions that can explode in giant eruptions. Now, for the first time, researchers have tracked a particular kind of solar wave as it swept upward from the sun’s surface through its atmosphere, adding to our understanding of how solar material travels throughout the sun.

Tracking solar waves like this provides a novel tool for scientists to study the atmosphere of the sun. The imagery of the journey also confirms existing ideas, helping to nail down the existence of a mechanism that moves energy – and therefore heat – into the sun’s mysteriously-hot upper atmosphere, called the corona. A study on these results was published Oct. 11, 2016, in The Astrophysical Journal Letters.

“We see certain kinds of solar seismic waves channeling upwards into the lower atmosphere, called the chromosphere, and from there, into the corona,” said Junwei Zhao, a solar scientist at Stanford University in Stanford, California, and lead author on the study. “This research gives us a new viewpoint to look at waves that can contribute to the energy of the atmosphere.”

The study makes use of the wealth of data captured by NASA’s Solar Dynamics Observatory, NASA’s Interface Region Imaging Spectrograph, and the Big Bear Solar Observatory in Big Bear Lake, California. Together, these observatories watch the sun in 16 wavelengths of light that show the sun’s surface and lower atmosphere. SDO alone captures 11 of these.

“SDO takes images of the sun in many different wavelengths at a high time resolution,” said Dean Pesnell, SDO project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “That lets you see the frequencies of these waves – if you didn’t have such rapid-fire images, you’d lose track of the waves from one image to the next.”

Though scientists have long suspected that the waves they spot in the sun’s surface, called the photosphere, are linked to those seen in the lowest reaches of the sun’s atmosphere, called the chromosphere, this new analysis is the first time that scientists have managed to actually watch the wave travel up through the various layers into the sun’s atmosphere.

When material is heated to high temperatures, it releases energy in the form of light. The type, or wavelength, of that light is determined by what the material is, as well as its temperature. That means different wavelengths from the sun can be mapped to different temperatures of solar material. Since we know how the sun’s temperature changes throughout the layers of its atmosphere, we can then order these wavelengths according to their height above the surface – and essentially watch solar waves as they travel upwards.

The implications of this study are twofold – first, this technique for watching the waves itself gives scientists a new tool to understand the sun’s lower atmosphere.