Thursday, April 30, 2020

SPACE - S0 - 20200430 - Stellar Magnetic Volcano Trigger, Wobble Quake, Orion

SPACE - S0 - 20200430 - Stellar Magnetic Volcano Trigger, Wobble Quake, Orion

Good Morning, 0bservers!

   
    
Despite a significant rise in particle density, the solar winds continued a downward slope into the calm range, from yesterday's high of 390 KPS to a current 280 KPS. The density rise coincides with a sharp Phi Angle shift. The calm winds are reflected in the KP-Index, which stayed quite low, in the KP-1 to KP-0 range, so unless we get some increase in solar winds we should expect a Cosmic Ray Alert in the next 24-36 hours. The X-Ray Flux popped up into the mid A-range around midnight UTC, calming somewhat a bit after that. The large equatorial bright spot is well past the midpoint, but it still seems to be crackling a bit, which may explain part of the X-Ray spike, but no CMEs are showing on LASCO C3. We had a Mag 5.1 quake off Kokopo, Papua New Guinea, a Mag 5.2 about 75 miles ENE of Hachinohe Japan, and a Mag 5.3 off Indonesia.

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Another new video from Suspicious0bservers, "Solar Superstorms | Will It Happen This Cycle? [Part 3]" 
  
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Wednesday, April 29, 2020

SPACE - S0 - 20200429 - UFOs, Comet ATLAS, 1998 OR2, Magnon Repulsion

SPACE - S0 - 20200429 - UFOs, Comet ATLAS, 1998 OR2, Magnon Repulsion

Good Morning, 0bservers!

   
    
Solar wind speeds dropped steadily yesterday from a high of around 430 KPS to a current low of 350 KPS, with a similar drop-off in particle density and temperature. Looks like the Phi Angle has stabilized as well, which is reflected in the KP-Index mostly in the KP-1 range, with the last reading coming in at KP-0. The GOES X-Ray Flux had a minor jump to the middle of the A-Range overnight. From the solar videos, it looks like both of the equatorial bright spots had a minor flicker or discharge at about the same time, which may explain the jump. Still, it does not seem to have been anything of serious note. Again, another quiet day on the lithosphere, with only a Mag 5.0 along the Northern Mid-Atlantic Ridge, and a Mag 5.4 blot echo in the Northwest of Argentina, about 100 miles deep.

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Another new video from Suspicious0bservers, "Solar Superstorms | Superflare vs Micronova [Part 2]" 
  
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Tuesday, April 28, 2020

Defense - Pentagon releases request for proposals on Next Generation Interceptor

Pentagon releases request for proposals on Next Generation Interceptor


By Aaron Mehta, Defense News,  April 24, 2020

A ground-based interceptor is launched from Vandenberg Air Force Base, Calif., toward a ballistic missile target launched from Alaska during a test Dec. 5, 2008. (Courtesy of the U.S. Missile Defense Agency)


WASHINGTON — The fight to build America’s next missile interceptor has officially begun.
The Missile Defense Agency on Friday released its request for proposal for its Next-Generation Interceptor (NGI). The RFP aims to downselect to two companies who will then compete for the right to build the interceptor, which will form the core of America’s homeland missile defense going forward.
Proposals are due July 31, but the MDA notes that there may be some give in that schedule due to the ongoing COVID-19 coronavirus pandemic.
The agency requested $664.1 million in fiscal year 2021 for the NGI program, as part of a $4.9 billion five-year budget plan.
Mark Wright, a spokesman for MDA, called the RFP “a vital step forward in designing, developing, and fielding the finest capabilities of both the DoD and American industry for the extraordinarily important purpose of defending the American homeland.”
“Notably, the intention of awarding two contracts for simultaneous development of the NGI effort promotes a healthy competition between the two contractor teams to produce the best NGI possible in the shortest time feasible,” Wright added.
In August, the Pentagon made the surprise decision to cancel the Redesigned Kill Vehicle program, with DoD research and engineering head Mike Griffin saying he didn’t want to keep throwing money at a program with fundamental technical issues.
RKV would have upgraded the U.S. homeland defense system’s interceptors designed to go after ballistic missile defense threats. The Pentagon decided that no more ground-based interceptors for the Ground-based Midcourse Defense System (GMD) would be built and all future interceptors that are fielded as part of the GMD system will be the new interceptor – that is, the NGI program.
Critics of the decision to cancel RKV and start over with a new design have raised concerns over the timeline, which could extend past 2030. But speaking in March, MDA head Vice Adm. Jon Hill said that waiting that long for the new capability is “unacceptable from a war fighter view” and “unacceptable to me as a program manager.”
Hill said once bids are on the table, the agency will be able to take a harder look at schedule and once an award has been made, it will hold industry accountable to meet “all the wickets.” If that happens, the schedule can be pulled to the left.
Jen Judson in Washington contributed to this report.

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Superconductivity: It's hydrogen's fault

APRIL 27, 2020, by Florian Aigner, Vienna University of Technology
https://phys.org/news/2020-04-superconductivity-hydrogen-fault.html

When hydrogen is incorporated into the nickelate structure, it is not a superconductor. Credit: TU Wien Nickelate

Last summer, a new age for high-temperature superconductivity was proclaimed—the nickel age. It was discovered that there are promising superconductors in a special class of materials, the so-called nickelates, which can conduct electric current without any resistance even at high temperatures.

However, it soon became apparent that these initially spectacular results from Stanford could not be reproduced by other research groups. TU Wien (Vienna) has now found the reason for this: In some nickelates additional hydrogen atoms are incorporated into the material structure. This completely changes the electrical behaviour of the material. In the production of the new superconductors, this effect must now be taken into account.

The search for High-Temperature Superconductors

Some materials are only superconducting near absolute temperature zero—such superconductors are not suitable for technical applications. Therefore, for decades, people have been looking for materials that remain superconducting even at higher temperatures. In the 1980s, "high-temperature superconductors" were discovered. What is referred to as "high temperatures" in this context, however, is still very cold: even high-temperature superconductors must be cooled strongly in order to obtain their superconducting properties. Therefore, the search for new superconductors at even higher temperatures continues.

"For a long time, special attention was paid to so-called cuprates, i.e. compounds containing copper. This is why we also speak of the copper age", explains Prof. Karsten Held from the Institute of Solid State Physics at TU Wien. "With these cuprates, some important progress was made, even though there are still many open questions in the theory of high-temperature superconductivity today".

But for some time now, other possibilities have also been under consideration. There was already a so-called "iron age" based on iron-containing superconductors. In summer 2019, the research group of Harold Y. Hwang's research group from Stanford then succeeded in demonstrating high-temperature superconductivity in nickelates. "Based on our calculations, we already proposed nickelates as superconductors 10 years ago, but they were somewhat different from the ones that have now been discovered. They are related to cuprates, but contain nickel instead of copper atoms," says Karsten Held.

The Trouble with Hydrogen

After some initial enthusiasm, however, it has become apparent in recent months that nickelate superconductors are more difficult to produce than initially thought. Other research groups reported that their nickelates do not have superconducting properties. This apparent contradiction has now been clarified at TU Wien.

"We analysed the nickelates with the help of supercomputers and found that they are extremely receptive to hydrogen into the material," reports Liang Si (TU Vienna). In the synthesis of certain nickelates, hydrogen atoms can be incorporated, which completely changes the electronic properties of the material. "However, this does not happen with all nickelates," says Liang Si, "Our calculations show that for most of them, it is energetically more favourable to incorporate hydrogen, but not for the nickelates from Stanford. Even small changes in the synthesis conditions can make a difference." Last Friday the group around Ariando Ariando from the NUS Singapore could report that they also succeeded in producing superconducting nickelates. They let the hydrogen that is released in the production process escape immediately.

Calculating the Critical Temperature with Supercomputers
At TU Wien new computer calculation methods are being developed and used to understand and predict the properties of nickelates. "Since a large number of quantum-physical particles always play a role here at the same time, the calculations are extremely complex," says Liang Si, "But by combining different methods, we are now even able to estimate the critical temperature up to which the various materials are superconducting. Such reliable calculations have not been possible before."In particular, the team at TU Wien was able to calculate the allowed range of strontium concentration for which the nickelates are superconducting—and this prediction has now been confirmed in experiment.

"High-temperature superconductivity is an extremely complex and difficult field of research," says Karsten Held. "The new nickelate superconductors, together with our theoretical understanding and the predictive power of computer calculations, open up a whole new perspective on the great dream of solid state physics: a superconductor at ambient temperature that hence works without any cooling."

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SPACE - S0 - 20200428 - Solar Eruption, Storm Alert, Amazing Science - Dipole Universe

SPACE - S0 - 20200428 - Solar Eruption, Storm Alert, Amazing Science - Dipole Universe

Good Morning, 0bservers!

   
    
Solar winds were variable yesterday, but still in the medium to calm range. After a peak of nearly 460 KPS, the speed dropped as low as 370 KPS, then rose again to 480 KPS, then dropped again near 390 KPS, and currently sits close to 375 KPS. It appears to be due to magnetic instability more than any coronal streams. The KP Index was mostly calm yesterday, with one minor bump up to KP-3 after midnight, dropping back down to KP-1, all still in the green zone. The solar videos showed a high magnetic release from the low to high northern latitudes at 304Å, but the tracking of its movement will hopefully aim AWAY from Earth (it didn't show up on the LASCO C3 video so the release may have stayed within the solar atmosphere). The equatorial bright spot will cross the midpoint in a couple of hours, and they're still showing underlying sunspot complexity. Only one quake yesterday, a Mag 5.2 in the Samoa Islands region, with only three blot echoes in the Mag 4.2-4.3 range.

* * *

Another new video from Suspicious0bservers, "Solar Superstorms | Field Collapse Risk [Part 1]" 
  
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Monday, April 27, 2020

SPACE - S0 - 20200427 - Sunspots Growing, Weather Alerts, Solar Forcing

SPACE - S0 - 20200427 - Sunspots Growing, Weather Alerts, Solar Forcing

Good Morning, 0bservers!

   
    
Solar wind speeds rose again due to magnetic instability, peaking at around 450 KPS after midnight, but have calmed back down to the 370-400 KPS range. No rise in particle density, but there was a brief rise in the temperature of the stream. The KP Index stayed mostly at the KP-2 range, with a brief KP-3 right after midnight when the wind speed rose. The equatorial bright spot should cross the midpoint later today, as well as a few scattered coronal holes. The new bright spot on the Northeast surface doesn't appear to have much in magnetic complexity, we're seeing hints of a new bright spot in the low Southern latitudes at the Eastern lim, and a bright spot popped up just South of the equator right at center disk, visible at 171Å, 193Å, and 304Å. That one has underlying sunspots with adequate separation to suggest at least Beta-level complexity. There was a bit of a rise back to the "normal" range of earthquake activity, with a Mag 5.2 off Papua New Guinea and a Mag 5.4 following several hours later, and a somewhat shallow Mag 5.0 off the coast of Kushiro Japan.
   
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Sunday, April 26, 2020

SPACE - S0 - 20200426 - Sun controls Climate, Tech, Biology, Quakes, Catastrophe

SPACE - S0 - 20200426 - Sun controls Climate, Tech, Biology, Quakes, Catastrophe

Good Morning, 0bservers!

   
    
The Phi-Angle stabilized yesterday, and after a peak solar wind speed of 470 KPS, there was a calming to a current range of 380-400 KPS. The KP Index stayed in the KP-0 to KP-1 range most of yesterday, but did pop up to the KP-2 range a couple of hours ago. Some new coronal holes are developing, both at the equator and the mid-Southern latitudes. There's a new bright spot crossing the Northeastern lim, and the equatorial bright spot is about two days from the midpoint. Regarding the latter, we seem to be seeing some small magnetic instabilities that might drive flares. Will continue to watch closely to determine if those sunspots develop polarized complexity. The lithosphere was VERY quiet, with only three blot echos, all of them under Mag 5.0.
   
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Saturday, April 25, 2020

New high-energy-density physics research provides insights about the universe

APRIL 24, 2020, by University of Rochester
https://phys.org/news/2020-04-high-energy-density-physics-insights-universe.html


Credit: CC0 Public Domain


Atoms and molecules behave very differently at extreme temperatures and pressures. Although such extreme matter doesn't exist naturally on the earth, it exists in abundance in the universe, especially in the deep interiors of planets and stars. Understanding how atoms react under high-pressure conditions—a field known as high-energy-density physics (HEDP)—gives scientists valuable insights into the fields of planetary science, astrophysics, fusion energy, and national security.

One important question in the field of HED science is how matter under high-pressure conditions might emit or absorb radiation in ways that are different from our traditional understanding.

In a paper published in Nature Communications, Suxing Hu, a distinguished scientist and group leader of the HEDP Theory Group at the University of Rochester Laboratory for Laser Energetics (LLE), together with colleagues from the LLE and France, has applied physics theory and calculations to predict the presence of two new phenomena—interspecies radiative transition (IRT) and the breakdown of dipole selection rule—in the transport of radiation in atoms and molecules under HEDP conditions. The research enhances an understanding of HEDP and could lead to more information about how stars and other astrophysical objects evolve in the universe.

What Is Interspecies Radiative Transition (Irt)?

Radiative transition is a physics process happening inside atoms and molecules, in which their electron or electrons can "jump" from different energy levels by either radiating/emitting or absorbing a photon. Scientists find that, for matter in our everyday life, such radiative transitions mostly happen within each individual atom or molecule; the electron does its jumping between energy levels belonging to the single atom or molecule, and the jumping does not typically occur between different atoms and molecules.

However, Hu and his colleagues predict that when atoms and molecules are placed under HED conditions, and are squeezed so tightly that they become very close to each other, radiative transitions can involve neighboring atoms and molecules.

"Namely, the electrons can now jump from one atom's energy levels to those of other neighboring atoms," Hu says.

What Is The Dipole Selection Rule?

Electrons inside an atom have specific symmetries. For example, "s-wave electrons" are always spherically symmetric, meaning they look like a ball, with the nucleus located in the atomic center; "p-wave electrons," on the other hand, look like dumbbells. D-waves and other electron states have more complicated shapes. Radiative transitions will mostly occur when the electron jumping follows the so-called dipole selection rule, in which the jumping electron changes its shape from s-wave to p-wave, from p-wave to d-wave, etc.


Under normal, non-extreme conditions, Hu says, "one hardly sees electrons jumping among the same shapes, from s-wave to s-wave and from p-wave to p-wave, by emitting or absorbing photons."

However, as Hu and his colleagues found, when materials are squeezed so tightly into the exotic HED state, the dipole selection rule is often broken down.

"Under such extreme conditions found in the center of stars and classes of laboratory fusion experiments, non-dipole X-ray emissions and absorptions can occur, which was never imagined before," Hu says.

Using Supercomputers To Study Hedp

The researchers used supercomputers at both the University of Rochester's Center for Integrated Research Computing (CIRC) and at the LLE to conduct their calculations.

"Thanks to the tremendous advances in high-energy laser and pulsed-power technologies, 'bringing stars to the Earth' has become reality for the past decade or two," Hu says.

Hu and his colleagues performed their research using the density-functional theory (DFT) calculation, which offers a quantum mechanical description of the bonds between atoms and molecules in complex systems. The DFT method was first described in the 1960s, and was the subject of the 1998 Nobel Prize in Chemistry. DFT calculations have been continually improved since. One such improvement to enable DFT calculations to involve core electrons was made by Valentin Karasev, a scientist at the LLE and a co-author of the paper.

The results indicate there are new emission/absorption lines appearing in the X-ray spectra of these extreme matter systems, which are from the previously-unknown channels of IRT and the breakdown of dipole selection rule.

Hu and Philip Nilson, a senior scientist at the LLE and co-author of the paper, are currently planning future experiments that will involve testing these new theoretical predictions at the OMEGA laser facility at the LLE. The facility lets users create exotic HED conditions in nanosecond timescales, allowing scientists to probe the unique behaviors of matters at extreme conditions.

"If proved to be true by experiments, these new discoveries will profoundly change how radiation transport is currently treated in exotic HED materials," Hu says. "These DFT-predicted new emission and absorption channels have never been considered so far in textbooks."


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SPACE - S0 - 20200425 - Hiding in Plain Sight, Weather, Data Missing

SPACE - S0 - 20200425 - Hiding in Plain Sight, Weather, Data Missing

Good Morning, 0bservers!

   
    
We had an early afternoon (UTC) Phi-Angle shift in solar magnetism, which jumped the particle density of the solar winds. That caused a early morning rise and spike in solar wind speeds, going from yesterday's low of 325 KPS to a top-out of 460 KPS, then lowering to 380 KPS, and we're now in the 420-440 KPS range. The KP Index rose to KP-3 readings before and after midnight, but they're back down in KP-2 range. The 3-day SWPC forecast  shows nothing above KP-2 for the next 72 hours. Some equatorial coronal holes developing and disappearing in the last 24 hours, we'll have to wait and see how or if they have an effect on solar winds. The bright spot moves closer to the midpoint, but there are still no signs if underlying sunspots or magnetic complexity. Only one quake of note yesterday, but it was a biggie - a Mag 6.3 about 80 miles west of Panguna, Papua New Guinea. Only a handful of weaker blot echo activity as well.
   
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Friday, April 24, 2020

SPACE - S0 - 20200424 - Dark Energy Dusted, Solar Airline Risk, Moon Map

SPACE - S0 - 20200424 - Dark Energy Dusted, Solar Airline Risk, Moon Map

Good Morning, 0bservers!

   
    
Solar wind speeds continued their slowing into the lower end of the calm range, currently in the 350-380 KPS range. Particle density and temperature are likewise lowered. There was a bit of a magnetic perturbation before midnight UTC, which brought the KP Index off the floor briefly to a KP-3 reading just after midnight,with a return to KP-1 in the last two readings. A couple new equatorial coronal holes have developed and are crossing the midpoint today, but they're small and somewhat disorganized when compared to the holes at the poles. That bright spot just South of the equator continues to head inward, and while it has some rather large magnetic loops, and a bit of "sparking" at 304Å, but there are zero underlying sunspots. Still, as it gets closer to crossing the meridian, we'll be sure to keep a closer eye on it. As to earthquake activity, it was a bit calmer than yesterday's report, with a Mag 5.5 off the Southwest tip of Mexico, and Mag 5.4 in the "middle of nowhere" in the South Pacific ocean. 

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Another new video from Suspicious0bservers, "Millions Are Being Murdered | The Killer Cure" -- It's not solar weather, but it IS science, and you need to watch this...

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Thursday, April 23, 2020

Scientists uncover major cause of resistance in solid electrolytes

APRIL 22, 2020, by Savannah Mitchem, Argonne National Laboratory
https://phys.org/news/2020-04-scientists-uncover-major-resistance-solid.html
Seeing the invisible: An electron hologram of a grain boundary in a lightly doped solid electrolyte sample from which electric potential at the grain boundary can be recovered.
Credit: Argonne National Laboratory

Reducing resistance to the flow of ions in solid electrolytes can improve the efficiency of fuel cells and batteries, but first, scientists must understand the material properties responsible for the resistance.

Solid electrolyte materials consist of hundreds of thousands of small crystalline regions, called grains, with various orientations. The materials, used in fuel cells and batteries, transport ions, or charged atoms, from one electrode to the other electrode. Boundaries between the grains in the materials are known to impede the flow of ions through the electrolyte, but the exact properties that cause this resistance have remained elusive.

Scientists from the U.S. Department of Energy's (DOE) Argonne National Laboratory contributed to a recent study led by Northwestern University to investigate grain boundaries in a solid electrolyte material. The study involved two powerful techniques—electron holography and atom probe tomography—that allowed scientists to observe the boundaries at an unprecedentedly small scale. The resulting insights provide new avenues for tuning chemical properties in the material to improve performance.

"When scientists study the conductivity of these electrolytes, they typically measure the average performance of all of the grains and grain boundaries together," said Charudatta Phatak, a scientist in Argonne's Materials Science Division (MSD), "but strategically manipulating the material properties requires deep knowledge of the origins of the resistance at the level of individual grain boundaries."

To explore the grain boundaries, the scientists performed electron holography of a common solid electrolyte at Argonne's Center for Nanoscale Materials (CNM), a DOE Office of Science User Facility. In this process, a beam of electrons hits a thin sample of the material and experiences a phase shift due to the presence of a local electric field in and around it. An external electric field then causes a portion of the electrons passing through the sample to be deflected, creating an interference pattern.

The scientists analyzed these interference patterns, created on the same principles as holograms in optical physics, to determine the electric field inside the material at the grain boundaries. They measured the local electric fields at ten types of grain boundaries with different degrees of misorientation.

Before this study, scientists thought that resistance at grain boundaries arose due to internal thermodynamic effects alone, such as the limit on the buildup of charge in an area. However, the large and varied electric fields they observed indicated the existence of previously undetected impurities in the material that explain the resistance.

"If the resistance was only due to thermodynamic limits, we should have seen the same fields across different boundary types," said Phatak, "but since we saw differences of almost an order of magnitude, there had to be another explanation."


Atom probe tomography reconstruction at a grain boundary in lightly doped solid electrolyte showing the 3D distribution of impurities in the sample. Credit: Northwestern University


To further study the trace impurities, the scientists used the Northwestern University Center for Atom Probe Tomography (NUCAPT) to determine the chemical identity of individual atoms at the grain boundaries. The electrolyte material in the study, made of ceria and often used in solid oxide fuel cells, was thought to be almost completely pure, but the tomography revealed the existence of impurities including silicon and aluminum—produced during material synthesis.

"On the one hand, it shows that if you make your materials cleaner, you can lessen these interfacial problems with electrolytes," said Sossina Haile, Walter. P. Murphy Professor of Materials Science and Engineering at Northwestern's McCormick School of Engineering. "Realistically though, you can't make a sample at an industrial scale cleaner than what we had prepared."

These inherent impurities are configured at the grain boundaries in a way that causes the electric fields across the boundaries to resist the flow of ions. The footprints that the impurities leave on the overall resistance of the electrolyte closely resemble what scientists would expect from thermodynamic effects alone. Understanding the true cause of the resistance—the impurities—can help the scientists to correct for it.

"Based on our findings, we can intentionally insert elements into the material that negate the effects of the impurities, lowering the resistance at the grain boundaries," said Phatak.

Funding for the study, in part, came from a Northwestern-Argonne Early Career Investigator Award for Energy Research awarded to Phatak. The program, which was matched by funds from the Institute of Sustainable Energy at Northwestern, fostered a collaboration between Phatak and Haile and supported Northwestern graduate student Xin Xu, first author on the study.

The use of these two techniques enabled scientists to visualize the systems in 3-D and to resolve confusion surrounding the properties of grain boundaries and how they affect resistance in this electrolyte. The new information could help scientists to increase the efficiency of solid electrolytes in general, which could help to improve the performance of many types of sustainable and renewable energy sources.

"If ions can move across the interfaces of these solid-state electrolytes more effectively, batteries will become much more efficient," Haile said. "The same is true of fuel cells, which is closer to the material system we studied. There's a potential to really impact fuel efficiency by making it easier to operate at temperatures that aren't extremely high."

A study, titled "Variability and origins of grain boundary electric potential detected by electron holography and atom-probe tomography," was published on April 13 in Nature Materials.


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SPACE - S0 - 20200423 - Storms, Space Water, Superflares, Galactic Plane

SPACE - S0 - 20200423 - Storms, Space Water, Superflares, Galactic Plane

Good Morning, 0bservers!

   
    
The solar magnetic field stabilized yesterday, which helped to slowly calm the solar wind speeds from a peak of 500 KPS to the 370-400 KPS range this morning. The KP Index stayed in the KP-1 to KP-2 range. A few bright spots across the face of the sun, including that new equatorial one that just crossed the lim, but an examination of the surface shows no underlying sunspots or magnetic instabilities. The lithosphere was a lot busier yesterday, with a Mag 5.0 off Vanuatu, another Mag 5.0 off Yemen, a Mag 5.5 and Mag 5.1 off Tonga and a Mag 5.2 near Toyoshina Japan.

* * *

Another new video from Suspicious0bservers, "Solar Magnetic Field Flows"

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Wednesday, April 22, 2020

This Video of Bullets Hitting 'Unbreakable' Prince Rupert's Drops Will Blow Your Mind

FIONA MACDONALD, 22 APRIL 2020
https://www.sciencealert.com/this-high-speed-footage-of-bullets-hitting-unbreakable-prince-ruperts-drops-will-blow-your-mind

(Smarter Every Day/YouTube)

For those of you who aren't familiar with the Prince Rupert's drop, this weird, scientific enigma is a seemingly simple glass object created by dripping molten glass into very cold water.

That process creates all kinds of crazy physical properties, which we'll go into later, but the end result is a teardrop-shaped piece of glass that's practically unbreakable at its bulbous 'drop' end, but will shatter from the slightest pressure at the elongated tail end.

Physicists have been obsessed with these 'unbreakable' glass drops since the 1600s. But what happens if you shoot one with a bullet?

In a 2016 video, Destin from Smarter Every Day used the newest technology to find out, by documenting the entire thing at a glorious 150,000 frames per second.

https://youtu.be/24q80ReMyq0

Spoiler: Prince Rupert's drops are so strong, they actually cause the bullet to shatter.

So, what's going on here? As you can see in the video above, shooting the Prince Rupert's drop will typically make the glass object shatter too, but that's not because of breaking the glass at the thick end.

In glorious slow motion, you can watch as the bullet crumbles against the wide end of the drop, sending out shock waves that then rattle the rest of the structure and cause the thin end to break, resulting in the entire thing exploding.

To understand how this works, you first need to understand why a Prince Rupert's drop is so weird in the first place.

When the Prince Rupert's drop is made, molten glass is poured into extremely cold water, causing the outside of the drop to cool and solidify almost instantly, while the inside remains molten and cools more slowly.

Because of thermal expansion, glass wants to expand while it's hot, and contract while it's cool.

That means that as the molten inside of the glass gradually cools down, it wants to contract and pull the solid outer layer inwards. But because the outer layer is already solidified, this just makes the whole thing tighter, making that bulbous end of the Prince Rupert's drop pretty much indestructible, and, as it turns out, bullet-proof.

But because the outside of the glass is in extremely high compressive stress, and the inside is in extremely high tensile stress, if one link is ever broken, the whole thing explodes, feeding off its stored internal energy.

This is what happens when the fragile thin end at the back of the drop gets broken - it releases all that pent-up energy, and that's why the entire thing shatters.

To understand that properly, check out this incredible slow-mo video that Destin originally did on the Prince Rupert's drop a few years ago:

https://youtu.be/xe-f4gokRBs
Now we know that these incredible pieces of glass are even more fascinating, because they can also withstand a bullet from a .22 rifle when shot at the right angle.

In fact, if you watch to the end, you'll see the mark left on one of the Prince Rupert's drops which was only grazed by the bullet, and didn't even break. So epic.

A version of this article was originally published in 2016.


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SPACE - S0 - 20200422 - Magnetic Universe, Electric Weather, Earth Day Data

SPACE - S0 - 20200422 - Magnetic Universe, Electric Weather, Earth Day Data

Good Morning, 0bservers!

   
    
We had some wacky Phi-Angle shifting before noon UTC, and it was reflected in a rise in solar wind speeds. They spent most of yesterday ramping up, peaking above 500 KPS just after midnight, then dropping below 450 KPS a couple of hours later, with the current speed ranging from 450-475 KPS. The KP Index popped up into the yellow zone (KP-4) when the magnetic polarity started to go both do and lally, but has calmed back down into the green KP-2 to KP-3 range. The usual blot echo activity in the lithosphere, but there was a single quake of note on the charts, a Mag 5.3 in the Kuril Islands.
   
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Site of Hannibal's first great victory identified?

Battlefield that gave Hannibal his first great victory and paved the way for his march on Rome is discovered in Spain

  • Believed to be between the cities of Driebes and Illana on banks of Tagus river
  • Was found via historical records, geographical records and archaeological digs 
  • Dates back to 220BC - two years before Hannibal famously crossed the Alps 
  • This battle helped cement his reputation as one of the great strategists in the Carthaginian army  
The site of a Hannibal's first great battle has been discovered by scientists.
His army of 25,000 men and 40 war elephants defeated a 100,000-strong horde of Spanish tribesmen in a battle which cemented Hannibal's reputation as a warfare savant.   
The clash occurred on the banks of the Tagus river between Driebes and Illana in Guadalajara in 220BC, according to new research.
Academics say the battle occurred close to a settlement of the Carparthian tribe near Caraca, in central Spain.
Hannibal, the Carthaginian commander of folklore, is best known for marching 40 war elephants across the Alps on his blood-thirsty quest to defeat Rome. 
But two years before he famously traversed the mountain range during the Second Punic War, the military commander, aged just 27, was warring with Spanish tribes. 
His success in Iberia enhanced his standing in the military and allowed him to take command of the upcoming wars, culminating in the brazen march on the Roman Empire with his 40 elephants via the Alps. 
Earlier in 220BC he had successfully conquered Helmática – now Salamanca in the northwest of the country – after defeating the Vettones tribe. 
Still bathing in the success of his victory, he was ambushed upon his return to his winter headquarters in Qart Hadasht, now modern-day Cartagena, in southeast Spain.
It is the site of this particular skirmish that has been a hot topic among historians and archaeologists alike, with two centuries of bickering failing to discern its location. 
View of the Tagus River from the Caraca archeological site in Driebes, Guadalajara. This area was where Hannibal fought off 10,000 warring Spanish tribesmen, a study found
View of the Tagus River from the Caraca archeological site in Driebes, Guadalajara. This area was where Hannibal fought off 10,000 warring Spanish tribesmen, a study found 
The site of a famed battle between Hannibal and a 100,000-strong hoard of angry Spanish tribesmen has been discovered by archaeologists. It was discovered on the banks of the Tagus river between Driebes and Illana in Guadalajara province and is believed to be the site
The site of a famed battle between Hannibal and a 100,000-strong hoard of angry Spanish tribesmen has been discovered by archaeologists. It was discovered on the banks of the Tagus river between Driebes and Illana in Guadalajara province and is believed to be the site
Hannibal's legacy would last millennia, and to this day he is regarded as one of the most brilliant strategic wartime commanders of all-time.  
Scholars say it was his ability to process the rapidly unfolding events and formulate an effective response that led to his crushing victory.  
The terrain had several key features which Hannibal used to his advantage. His forces were outnumbered approximately four to one and he knew an all-out melee would result in a bloodbath for his troops.
Hannibal positioned his troops so the only way for them to be approached by the encroaching tribespeople was after crossing a ford in the river. 
This created a natural choke point as the 100,000 Spaniards were funnelled into small area in order to cross the Tagus river. 
This ensured his enemies, from the hostile local Carpetani, Vettone and Olcade tribes, could not attack in a mass wave, which may have overwhelmed the Carthaginians.  
After slowly making their way across the river via the fords, the natives were met by a waiting battalion of mounted troops, who butchered them in droves.   
As well as placing the cavalry at the fords, Hannibal also ordered the rapid construction of a palisade running parallel to the river. 
Here, the prized elephants and the infantry waited. 
The two defensive features meant the warring Spaniards had just two options to approach Hannibal's men — risk crossing the river which could reach almost 6ft deep with strong currents, or cross at the fords and take on the waiting cavalry. 
Many of the locals, fighting to avenge the destruction of their cities and crops, perished after being swept away by the river. Those that did survive the treacherous crossing were slain almost instantly.  
Hannibal, the Carthaginian commander of folklore, is best known for marching 40 war elephants across the Alps on his blood-thirsty quest to defeat Rome. Two years before he traversed the Alps, the military commander, aged just 27, was warring with various Spaniards
Hannibal, the Carthaginian commander of folklore, is best known for marching 40 war elephants across the Alps on his blood-thirsty quest to defeat Rome. Two years before he traversed the Alps, the military commander, aged just 27, was warring with various Spaniards 

How Hannibal rose to become one of the best military tacticians of all-time and took 40 war elephants across the Alps 

Hannibal, the Carthaginian commander of folklore, is best known for marching 40 war elephants across the alps on his blood-thirsty quest to defeat Rome
Hannibal, the Carthaginian commander of folklore, is best known for marching 40 war elephants across the alps on his blood-thirsty quest to defeat Rome
Hannibal, the Carthaginian commander of folklore, is best known for marching 40 war elephants across the alps on his blood-thirsty quest to defeat Rome.
He was the son of Hamilcar Barca, a Carthaginian commander during the First Punic War (264–241 BC).
His brothers and brothers-in-law were all also commanders in the army. 
During his lifetime, there was great tension in Europe as Rome asserted it dominance over Italy and it surrounding nations. 
Hannibal was central in the war against this expanding empire. 
In 222BC Hannibal was fighting battles against Spanish tribes and the general, in his mid-20s at his point, was establishing himself as one of the finest strategic minds in the Carthaginian army. 
In 218BC, the Second Punic War broke out following Hannibal's attack on Saguntum, an ally of Rome.
It was then that Hannibal marched his war elephants across the Alps, inscribing himself into legend.   
He occupied much of southern Italy for more than a decade, but the Romans were wary of his prowess and avoided direct confrontation when possible. 
A tumultuous post-war life led to his eventual betrayal to the Romans and he committed suicide by poison around the year 180BC. 
Hannibal's legacy would last millennia, and to this day is regarded as one of the most brilliant strategic wartime commanders of all-time. 
A raised area nearby, called El Jardín hill, may also have been useful for Hannibal.  
This spot, to the southeast of the main battle, would have provided a vantage point to the commander from which he could orchestrate his manoeuvres
It may also have been used to hide his escort and light cavalry, the researchers suggest. 
When the general saw his rivals floundering and the victory within reach, he counterattacked. 
Various sites for this battle have been suggested in the past, with most drawing on the accounts of Greek historian, Polybius and Roman author, Titus Livius. 
To track down the most likely location, the researchers — from Caraca-Driebes Archaeological Team, the National Museum of Roman Art and the Spanish Geological Mining Institute (IGME) — combined various sources of information. 
They assessed historical accounts and investigated geological data and archaeological studies to find the most  logical route Hannibal would have taken back to Qart Hadasht and which sites best fitted this description. 
The authors of the study believe Hannibal was using an ancient route which connected Complutum, now Alcalá de Henares in Madrid region, to Carthago Nova, now Cartagena in Murcia.
The route crossed the Tagus River close to Driebes, not far from Carpentani fortified settlement of Caraca. 
'The decision to attack Hannibal there was made by the Carpetani, as they knew the area well and it would also give them a leadership role within the coalition formed with the Vettones and Olcades,' explains Emilio Gamo, of the National Museum of Roman Art.
The report, titled Historical, Archaeological and Geological Data for the location of the Battle of Hannibal on the Tagus (220 B.C.), also found that it is likely the fords seen on the bend of the river today are likely in the same location as they were at the time of the battle. 
Archaeological evidence reported in the study also speaks of silver and ceramics at the site which may belong to Hannibal's warriors.