ALMA Discovered a Titanic Galactic Wind

Researchers using the Atacama Large Millimeter/submillimeter Array (ALMA) discovered a titanic galactic wind driven by a supermassive black hole 13.1 billion years ago. This is the earliest example yet observed of such a wind to date and is a telltale sign that huge black holes have a profound effect on the growth of galaxies from the very early history of the universe.

At the center of many large galaxies hides a supermassive black hole that is millions to billions of times more massive than the Sun. Interestingly, the mass of the black hole is roughly proportional to the mass of the central region (bulge) of the galaxy in the nearby universe. At first glance, this may seem obvious, but it is actually very strange.

The reason is that the sizes of galaxies and black holes differ by about 10 orders of magnitude. Based on this proportional relationship between the masses of two objects that are so different in size, astronomers believe that galaxies and black holes grew and evolved together (coevolution) through some kind of physical interaction.

Stay Tuned For More Latest Research and Development

Solar Eclipse and Earth Changing Events

Research suggests the sudden temperature fluctuation during the period of a solar eclipse can set in motion a chain of events from Earth’s atmosphere to her ocean bottoms. As the moon cast its shadow along the eclipse path, it presents a sudden and rapid shift in jet stream temperature which in-turn has a direct affect on ocean currents.

Although temperature flux may be subtle, if tectonics are at their tipping point, it would not take much to set them off. Additionally, the rapid temperature change can cause an expansion and contraction of Earth’s lithosphere, even if ever so slight, can set off a chain reaction of tectonic slippage resulting in significant earthquakes and volcanic activity.

GREAT VIDEO – CLICK HERE (time lapsed)

Remember, the majority of volcanoes are submarine (ocean bottom); hence the rapid shift in ocean temperatures is also prone to set off a rippling effect which is often unpredictable due to the spider webbing tentacles which connect a system of mantle plumes and volcanoes.

Watch for significant events to occur over the next ten days. Pay special attention to geographical areas along the path of June 10th 2021 annular eclipse related to Earth Changing Events. (see graphic above)

Stay Tuned For More Latest Research and Development

Envisioning Safer Cities with Artificial Intelligence

Over the past several decades, artificial intelligence has advanced tremendously, and today it promises new opportunities for more accurate healthcare, enhanced national security and more effective education, researchers say. But what about civil engineering and city planning? How do increased computing power and machine learning help create safer, more sustainable and resilient infrastructure?

U.S. National Science Foundation-funded researchers at the Computational Modeling and Simulation Center, or SimCenter, have developed a suite of tools called BRAILS — short for Building Recognition using AI at Large-Scale — that can automatically identify characteristics of buildings in a city and detect the risks a city’s structures would face in the event of an earthquake, hurricane or tsunami.

SimCenter is part of the NSF-funded Natural Hazards Engineering Research Infrastructure program and serves as a computational modeling and simulation center for natural hazards engineering researchers at the University of California, Berkeley.

Charles Wang, the lead developer of BRAILS, says the project grew out of a need to “quickly and reliably characterize the structures in a city. We want to simulate the impact of hazards on all the buildings in a region, but we don’t have a description of the building attributes.”

For example, he says, “in the San Francisco Bay area, there are millions of buildings. Using AI, we are able to get the needed information. We can train neural network models to infer building information from images and other sources of data.”

To train the BRAILS modules and run the simulations, the researchers used supercomputers at the Texas Advanced Computing Center — notably Frontera, the fastest academic supercomputer in the world, and Maverick 2, a GPU-based system designed for deep learning.

“Frontera is a leadership computing resource that serves science and engineering research for the nation,” says Manish Parashar, director of NSF’s Office of Advanced Cyberinfrastructure. “We are excited about the new computational methods and techniques Frontera is enabling to transform how engineering discoveries are being made to make our lives safer.”

The SimCenter recently released BRAILS version 2.0, which includes modules to predict a larger spectrum of building characteristics. These include occupancy class, roof type, foundation elevation, year built, number of floors, and whether a building has a “soft-story” — a civil engineering term for structures that include ground floors with large openings like storefronts that may be more prone to collapse during an earthquake.

“Given the importance of regional simulations and the need for large inventory data to execute these, machine learning is really the only option for making progress,” says SimCenter co-director Sanjay Govindjee. “It is exciting to see civil engineers learning these new technologies and applying them to real-world problems.”

Stay Tuned For More Latest Research and Development


BREAKING NEWS: Recording of Largest Gamma-Ray Burst to Date

A specialized observatory in Namibia has recorded the most energetic radiation and longest gamma-ray afterglow of a so-called gamma-ray burst (GRB) to date.

The observations with the High Energy Stereoscopic System (H.E.S.S.) challenge the established idea of how gamma-rays are produced in these colossal stellar explosions which are the birth cries of black holes, as the international team reports in the journal Science.

“Gamma-ray bursts are bright X-ray and gamma-ray flashes observed in the sky, emitted by distant extragalactic sources,” explains DESY scientist Sylvia Zhu, one of the authors of the paper. “They are the biggest explosions in the universe and associated with the collapse of a rapidly rotating massive star to a black hole.

A fraction of the liberated gravitational energy feeds the production of an ultrarelativistic blast wave. Their emission is divided into two distinct phases: an initial chaotic prompt phase lasting tens of seconds, followed by a long-lasting, smoothly fading afterglow phase.”

Stay tuned for reports of ongoing events….

UPDATE: Galactic Cosmic Rays Continue to Rise and Human Effect

Yes, it’s me. Happy to be presenting the latest news and research as it occurs. It does appear published findings are reflective of my 2012 Equation.  Cheers, Mitch

Radiation is a form of energy that is emitted in the form of rays, electromagnetic waves, and/or particles. In some cases, radiation can be seen (visible light) or felt (infrared radiation), while other forms – like x-rays and gamma rays – are not visible and can only be observed with special equipment.

Galactic Cosmic Ray collisions in the body can be harmful because they can damage the DNA in cells. Remember, a single cosmic ray has a large amount of energy. If it collides with DNA, it will destroy part of that DNA strand. DNA contains instructions for the cell to function properly. When the DNA is damaged, the cell will malfunction. Usually the cell will then die, but sometimes it can reproduce itself. If that happens on a large enough scale, the person may develop cancer.

Galactic Cosmic radiation is a well-known cause of single-event upsets (SEU) on disruption to electrical circuits in electronic devices. It most commonly occurs with devices such as laptop computers, cell phones, and personal digital assistants. Research presented by the Heart Rhythm Society, indicate some patients with Implantable Cardioverter-Defibrillators (ICDs) who experienced ionizing radiation strikes that discharged elements in the Defib during air travel, may be attributed to exposure of Galactic Cosmic Radiation while on commercial airline flights. These cases highlight the significant impact of SEUs on ICD patients clinical and the need for further recognition and study of this problem.

NASA’s Cosmic Ray Telescope for the Effects of Radiation (CRaTER), studies radiation environment and its biological impacts by measuring galactic and solar cosmic ray radiation behind a “human tissue-equivalent” plastic.


CRaTER investigation goals are to measure and characterize the deep space radiation environment in terms of Linear Energy Transfer (LET) spectra of galactic and solar cosmic rays (particularly above 10 MeV) in Low Earth Orbit (LEO). It will also investigate the effects of shielding by measuring LET spectra behind tissue-equivalent plastic. Test models of radiation effects and shielding by verifying/validating model predictions of LET spectra with LRO measurements.

Stay Tuned For Ongoing News and Events


An Overlooked Piece Of The Solar Dynamo Puzzle


A previously unobserved mechanism is at work in the Sun’s rotating plasma: a magnetic instability, which scientists had thought was physically impossible under these conditions. The effect might even play a crucial role in the formation of the Sun’s magnetic field, say researchers from Helmholtz-Zentrum Dresden-Rossendorf (HZDR), the University of Leeds and the Leibniz Institute for Astrophysics Potsdam (AIP) in the journal Physical Review Fluids.

Just like an enormous dynamo, the sun’s magnetic field is generated by electric currents. In order to better understand this self-reinforcing mechanism, researchers must elucidate the processes and flows in the solar plasma. Differing rotation speeds in different regions and complex flows in the sun’s interior combine to generate the magnetic field. In the process, unusual magnetic effects can occur — like this newly discovered magnetic instability.

Researchers have coined the term “Super HMRI” for this recently observed special case of magnetorotational instability (MRI). It is a magnetic mechanism that causes the rotating, electroconductive fluids and gases in a magnetic field to become unstable. What is special about this case is that the Super HMRI requires exactly the same conditions that prevail in the plasma close to the solar equator — the place where astrophysicists observe the most sunspots and, thus, the Sun’s greatest magnetic activity. So far, however, this instability in the Sun had gone completely unnoticed and is not yet integrated in models of the solar dynamo.

It is, nonetheless, known that magnetic instabilities are crucially involved in many processes in the universe. Stars and planets, for example, are generated by large rotating disks of dust and gas. In the absence of a magnetic field, this process would be inexplicable. Magnetic instabilities cause turbulence in the flows within the disks and thus enable the mass to agglomerate into a central object. Like a rubber band, the magnetic field connects neighboring layers that rotate at different speeds. It accelerates the slow particles of matter at the edges and slows down the fast ones on the inside. There the centrifugal force is not strong enough and the matter collapses into the center. Near the solar equator it behaves precisely the other way around. The inner layers move more slowly than the outer ones. Up to now, experts had considered this kind of flow profile to be physically extremely stable.

The researchers at HZDR, the University of Leeds and AIP still decided to investigate it more thoroughly. In the case of a circular magnetic field, they had already calculated that even when fluids and gases were rotating faster on the outside, magnetic instability could occur. However, only under unrealistic conditions: the rotational speed would have to increase too strongly towards the outer edge.

Trying another approach, they now based their investigations on a helical magnetic field. “We didn’t have any great expectations, but then we were in for a genuine surprise,” HZDR’s Dr. Frank Stefani remembers — because the magnetic instability can already occur when the speed between the rotating layers of plasma only increases slightly — which happens in the region of the Sun closest to the equator.

“This new instability could play an important role in generating the sun’s magnetic field,” Stefani estimates. “But in order to confirm it we first need to do further numerically complicated calculations.” Prof. Günther Rüdiger of AIP adds, “Astrophysicists and climate researchers still hope to better understand the cycle of sunspots. Perhaps the ‘Super HMRI’ we have now found will take us a decisive step forward. We’ll check it out.”

With its various specialisms in magnetohydrodynamics and astrophysics, the interdisciplinary research team has been investigating magnetic instabilities — in the lab, on paper and with the aid of sophisticated simulations — for more than 15 years. The scientists want to improve physical models, understand cosmic magnetic fields and develop innovative liquid metal batteries. Thanks to close cooperation, in 2006, they managed to experimentally prove the theory of magnetorotational instability for the first time. They are now planning the test for the special form they have predicted in theory: In a large-scale experiment that is currently being set up in the DRESDYN project at HZDR, they want to study this magnetic instability in the lab.

2019 Nobel Prize In Physics: Evolution Of The Universe And Discovery Of Exoplanet Orbiting Solar-Type Star


The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics 2019 “for contributions to our understanding of the evolution of the universe and Earth’s place in the cosmos” with one half to James Peebles of Princeton University, USA, “for theoretical discoveries in physical cosmology” and the other half jointly to Michel Mayor of the University of Geneva, Switzerland, and Didier Queloz of the University of Geneva, Switzerland, and the University of Cambridge, UK, “for the discovery of an exoplanet orbiting a solar-type star.”

New perspectives on our place in the universe

This year’s Nobel Prize in Physics rewards new understanding of the universe’s structure and history, and the first discovery of a planet orbiting a solar-type star outside our solar system.

James Peebles’ insights into physical cosmology have enriched the entire field of research and laid a foundation for the transformation of cosmology over the last fifty years, from speculation to science. His theoretical framework, developed since the mid-1960s, is the basis of our contemporary ideas about the universe.

The Big Bang model describes the universe from its very first moments, almost 14 billion years ago, when it was extremely hot and dense. Since then, the universe has been expanding, becoming larger and colder. Barely 400,000 years after the Big Bang, the universe became transparent and light rays were able to travel through space. Even today, this ancient radiation is all around us and, coded into it, many of the universe’s secrets are hiding. Using his theoretical tools and calculations, James Peebles was able to interpret these traces from the infancy of the universe and discover new physical processes.

The results showed us a universe in which just five per cent of its content is known, the matter which constitutes stars, planets, trees — and us. The rest, 95 per cent, is unknown dark matter and dark energy. This is a mystery and a challenge to modern physics.

In October 1995, Michel Mayor and Didier Queloz announced the first discovery of a planet outside our solar system, an exoplanet, orbiting a solar-type star in our home galaxy, the Milky Way. At the Haute-Provence Observatory in southern France, using custom-made instruments, they were able to see planet 51 Pegasi b, a gaseous ball comparable with the solar system’s biggest gas giant, Jupiter.

This discovery started a revolution in astronomy and over 4,000 exoplanets have since been found in the Milky Way. Strange new worlds are still being discovered, with an incredible wealth of sizes, forms and orbits. They challenge our preconceived ideas about planetary systems and are forcing scientists to revise their theories of the physical processes behind the origins of planets. With numerous projects planned to start searching for exoplanets, we may eventually find an answer to the eternal question of whether other life is out there.

This year’s Laureates have transformed our ideas about the cosmos. While James Peebles’ theoretical discoveries contributed to our understanding of how the universe evolved after the Big Bang, Michel Mayor and Didier Queloz explored our cosmic neighbourhoods on the hunt for unknown planets. Their discoveries have forever changed our conceptions of the world.

James Peebles, born 1935 in Winnipeg, Canada. Ph.D. 1962 from Princeton University, USA. Albert Einstein Professor of Science at Princeton University, USA.

Michel Mayor, born 1942 in Lausanne, Switzerland. Ph.D. 1971 from University of Geneva, Switzerland. Professor at University of Geneva, Switzerland.

Didier Queloz, born 1966. Ph.D. 1995 from University of Geneva, Switzerland. Professor at University of Geneva, Switzerland and University of Cambridge, UK.

Prize amount: 9 million Swedish krona, with one half to James Peebles and the other half jointly to Michel Mayor and Didier Queloz