Thursday, August 5, 2021

Google’s ‘time crystals’ could be the greatest scientific achievement of our lifetimes

Tristan Greene


Eureka! A research team featuring dozens of scientists working in partnership with Google‘s quantum computing labs may have created the world’s first time crystal inside a quantum computer.

This is the kind of news that makes me want to jump up and do a happy dance.

These scientists may have produced an entirely new phase of matter. I’m going to do my best to explain what that means and why I personally believe this is the most important scientific breakthrough in our lifetimes.

However, for the sake of clarity, there’s two points I need to make first:
Time crystals are a wickedly difficult concept to understand and even harder to explain.
The Google team might have created time crystals. This is pre-print research and has yet to receive full peer-review. Until the rest of the scientific community has time to review and replicate the work, we can’t say for sure it’s legitimate.
What’s a time crystal?

In colloquial terms, it’s a big screw you to Sir Isaac Newton.

Time crystals are a new phase of matter. For the sake of simplicity, let’s imagine a cube of ice.

When you put a cube of ice in glass of water, you’re introducing two separate entities (the ice cube and the liquid water) to each other at two different temperatures.

Everyone knows that the water will get colder (that’s why we put the ice in there) and, over time, the ice will get warmer and turn into water. Eventually you’ll just have a glass of room-temperature water.

We call this process “thermal equilibrium.”

Most people are familiar with Newton’s first law of motion, it’s the one that says “an object at rest tends to stay at rest and an object in motion tends to stay in motion.”

An important side-effect of this law of physics is that it means a perpetual motion machine is classically impossible.

According to classical physics, the universe is always moving towards entropy. In other words: if we isolate an ice cube and a room-temperature glass of water from all other external forces, the water will always melt the ice cube.

The entropy (the movement towards change) of any system will always remain the same if there are no processes, and it will always increase if there are processes.

Since our universe has stars exploding, black holes sucking, and people lighting things on fire – chemical processes – entropy is always increasing.

Except when it comes to time crystals. Time crystals don’t give a damn what Newton or anyone else thinks. They’re lawbreakers and heart takers. They can, theoretically, maintain entropy even when they’re used in a process.
What’s that mean

Think about a crystal you’re familiar with, such as a snowflake. Snowflakes aren’t just beautiful because each one is unique, they’re also fascinating formations that nearly break the laws of physics themselves.

Crystalline structures form in the physical world because, for whatever fundamental scientific reason, the atoms within them “want” to exist in certain exact points.

“Want” is a really weird word to use when we’re talking about atoms – I’m certainly not implying they’re sentient – but it’s hard to describe the tendency toward crystalline structures in abstracts such as “why.”

A time crystal is a new phase of matter that, simplified, would be like having a snowflake that constantly cycled back and forth between two different configurations. It’s a seven-pointed lattice one moment and a ten-pointed lattice the next, or whatever.

What’s amazing about time crystals is that when they cycle back and forth between two different configurations, they don’t lose or use any energy.

Time crystals can survive energy processes without falling victim to entropy. The reason they’re called time crystals is because they can have their cake and eat it too.

They can be in a state of having eaten the whole cake, and then cycle right back to a state of still having the cake – and they can, theoretically, do this forever and ever.

Most importantly, they can do this inside of an isolated system. That means they can consume the cake and then magically make it reappear over and over again forever, without using any fuel or energy.
Who cares? What’s this going to mean for me?

Literally everyone should care. As I wrote back in 2018, time crystals could be the miracle quantum computing needs.

Nearly every far-future tech humans can imagine, from teleportation to warp drives and from artificial food synthesizers to perpetual motion reactors capable of powering the world without burning fuels or harnessing energy, will require quantum computing systems.

Quantum computers can solve really hard problems. Unfortunately, they’re brittle. It’s hard to build them, hard to maintain them, hard to get them to do anything, and even harder to interpret the results they give. This is because of something called “decoherence,” which works a lot like entropy.

Computer bits in the quantum world, qubits, share a funky feature of quantum mechanics that makes them act differently when observed than when they’re left alone. That sort of makes any direct measurements of qubit states (reading the computer’s output) difficult.

But time crystals want to be coherent. So putting them inside a quantum computer, and using them to conduct computer processes could potentially serve an incredibly important function: ensuring quantum coherence.

So Google solved quantum computing?

No. No, no, no, no no. Don’t get me wrong. This is baby steps. This is infancy research. This is Antony van Leeuwenhoek becoming the first person to use a microscope to look at a drop of water under magnification.

What Google‘s done, potentially, is prove that humans can manufacture time crystals. In the words of the researchers themselves:

"These results establish a scalable approach to study non-equilibrium phases of matter on current quantum processors."

Basically they believe they’ve proven the concept, so now it’s time to see what can be done with it.
Then why is this so exciting?

Time crystals have always been theoretical. And by “always,” I mean: since 2012 when they were first hypothesized.

If Google‘s actually created time-crystals, it could accelerate the timeline for quantum computing breakthroughs from “maybe never” to “maybe within a few decades.”

At the far-fetched, super-optimistic end of things – we could see the creation of a working warp drive in our lifetimes. Imagine taking a trip to Mars or the edge of our solar system, and being back home on Earth in time to catch the evening news.

And, even on the conservative end with more realistic expectations, it’s not hard to imagine quantum computing-based chemical and drug discovery leading to universally-effective cancer treatments.

This could be the big eureka we’ve all been waiting for. I can’t wait to see what happens in peer-review.

If you want to know more, you can read Google’s paper here. And if you’re looking for a technical deep-dive into the scientific specifics of what the researchers accomplished in the lab, this piece on Quanta Magazine by Natalie Wolchover is the bee’s knees.


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Observatories Assemble: NASA’s Juno Spacecraft Joins Japan’s Hisaki Satellite and W. M. Keck Observatory to Solve “Energy Crisis” on Jupiter

Aug 4, 2021, Bill Steigerwald, Editor: Bill Steigerwald
https://www.nasa.gov/feature/goddard/2021/juno-jupiter-auroral-heating


Jupiter is shown in visible light for context underneath an artistic impression of the Jovian upper atmosphere's infrared glow. 
The brightness of this upper atmosphere layer corresponds to temperatures, from hot to cold, in this order: white, yellow, bright red and lastly, dark red. The aurorae are the hottest regions and the image shows how heat may be carried by winds away from the aurora and cause planet-wide heating.
Credits: J. O'Donoghue (JAXA)/Hubble/NASA/ESA/A. Simon/J. Schmidt

Sitting more than five times the distance from the Sun as Earth, Jupiter is not expected to be particularly warm. Based on the amount of sunlight received, the average temperature in the planet’s upper atmosphere should be about minus 100 degrees Fahrenheit or a chilly minus 73 Celsius. Instead, the measured value soars to around 800 degrees Fahrenheit or 426 Celsius. The source of this extra heat has remained elusive for 50 years, causing scientists to refer to the discrepancy as an “energy crisis” for the planet.

Recently an international team assembled observations from a trio of observatories -- NASA’s Juno spacecraft, the Hisaki satellite from the Japan Aerospace Exploration Agency (JAXA) and Keck Observatory on Maunakea in HawaiĘ»i. -- to discover the likely source of Jupiter’s thermal boost.

“We found that Jupiter’s intense aurora, the most powerful in the solar system, is responsible for heating the entire planet’s upper atmosphere to surprisingly high temperatures,” said James O’Donoghue of the JAXA Institute of Space and Astronautical Science, Sagamihara, Japan. O’Donoghue began the research while at NASA’s Goddard Space Flight Center in Greenbelt, Maryland and is lead author of a paper about this research appearing in Nature August 4.

https://youtu.be/pXTpL3DA6yY
Jupiter is first shown in visible light for context before an artistic impression of the Jovian upper atmosphere's infrared glow is overlain. The brightness of this upper atmosphere layer corresponds to temperatures, from hot to cold, in this order: white, yellow, bright red and lastly, dark red. The aurorae are the hottest regions and the animation shows how heat may be carried by winds away from the aurora and cause planet-wide heating. At the end, real data is added with a temperature scale, indicating the observed global temperatures measured in the study.
Credits: J. O'Donoghue (JAXA)/Hubble/NASA/ESA/A. Simon/J. Schmidt


Auroras occur when electrically charged particles are caught in a planet’s magnetic field. These spiral along invisible lines of force in the magnetic field towards the planet’s magnetic poles, striking atoms and molecules in the atmosphere to release light and energy. On Earth, this leads to the colorful light show that forms the aurora Borealis and Australis, also known as the northern and southern lights. At Jupiter, material erupting from its volcanic moon, Io, leads to the most powerful aurora in the Solar System and enormous heating in upper atmosphere over the polar regions of the planet.

The idea that the aurora could be the source of Jupiter’s mysterious energy had been proposed previously but observations have been unable to confirm or deny this until now.

Global models of Jupiter’s upper atmosphere suggested that winds heated by the aurora and headed to the equator would be overwhelmed and redirected by westward winds driven by the planet’s rapid rotation. This would prevent the auroral energy from escaping the polar regions and heating the whole atmosphere. However, this new observational result suggests that such trapping is not occurring, and that the westward winds may be relatively weaker than expected compared with equatorward winds.

High-resolution temperature maps from Keck II, combined with magnetic field data from Hisaki and Juno, allowed the team to catch the aurora in the act of sending what appears to be a pulse of heat toward Jupiter’s equator.

The team observed Jupiter with the Keck II telescope for five hours on two separate nights in April 2016 and January 2017. Using the Near-Infrared Spectrometer (NIRSPEC) on Keck II, heat from electrically charged hydrogen molecules (H3+ ions) in Jupiter’s atmosphere was traced from the planet’s poles down to the equator.

Previous maps of the upper atmospheric temperature were formed using images consisting of only several pixels. That’s not enough resolution to see how the temperature might be changing across the planet, providing few clues as to the origin of the extra heat. To improve the situation, the team utilized the power of Keck II to take many more temperature measurements across the face of the planet and only included measurements with uncertainty in the recorded value of less than five percent. This took years of careful work and yielded temperature maps with over ten thousand individual data points, the highest resolution to date.

Instead of high temperatures only in the polar regions near the aurora, which would be expected if the heat was trapped there, these detailed maps showed that the heat in the upper atmosphere was more widely distributed, with a gradual decrease in temperature closer to the equator.

“We also revealed a strange localized region of heating well away from the aurora - a long bar of heating unlike anything we've seen before,” said Tom Stallard, a co-author of the paper at the University of Leicester, Leicester, United Kingdom. “Though we can't be sure what this feature is, I am convinced it’s a rolling wave of heat flowing equatorward from the aurora.”

Additionally, observations from JAXA’s Hisaki satellite showed that conditions at the time of the Keck II temperature observations could generate a strong aurora on Jupiter. From orbit around Earth, Hisaki has observed the aurora-generating magnetic field around Jupiter since the mission’s launch in 2013. This long-term monitoring has revealed that Jupiter’s magnetic field is strongly influenced by the solar wind; a stream of high-energy particles that emanates from the Sun. The solar wind carries its own magnetic field and when this meets Jupiter’s planetary field, the latter is compressed. At the time of the Keck II observations, Hisaki showed that pressure from the solar wind was particularly high at Jupiter and the field compression is likely to have created an enhanced aurora.

Jupiter is shown in visible light for context with an artistic impression of the Jovian upper atmosphere's infrared glow overlain, along with magnetic field lines (blue lines). The aurorae are the hottest regions and the image shows how heat may be carried by winds away from the aurora and cause planet-wide heating.
Credits: J. O'Donoghue (JAXA)/Hubble/NASA/ESA/A. Simon/J. Schmidt

Finally, observations from Juno in orbit around Jupiter provided the precise location of the aurora on the planet. “Juno’s magnetic field data provided us with a ‘ground truth’ as to where the aurora was: this information isn't readily available from heat maps, as heat leaks away in many directions,” said O’Donoghue. “Picture this like a beach: if the hot atmosphere is water, the magnetic field mapped by Juno is shoreline, and the aurora is ocean, we found that water left the ocean and flooded the land, and Juno revealed where that shoreline was to help us understand the degree of flooding.”

"It was pure luck that we captured this potential heat-shedding event,” adds O’Donoghue. “If we’d observed Jupiter on a different night, when the solar wind pressure had not recently been high, we would have missed it!”

More about the observatories and partners:

The research was funded by NASA through the Solar System Observations Program and the Solar System Workings Program as well as JAXA’s International Top Young Fellowship program. Juno is part of NASA's New Frontiers Program, which is managed at NASA's Marshall Space Flight Center in Huntsville, Alabama, for the agency's Science Mission Directorate in Washington. NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of the Southwest Research Institute, San Antonio, Texas. NASA Goddard built and runs Juno’s magnetometer instrument. The W. M. Keck Observatory is operated as a scientific partnership among the California Institute of Technology, the University of California and NASA. The Observatory was made possible by the financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community; the authors are fortunate to have the opportunity to conduct observations from this mountain.


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SPACE - S0 - 20210805 - Major Climate Bombshell, The Other Nova, Journal Shame

SPACE - S0 - 20210805 - Major Climate Bombshell, The Other Nova, Journal Shame

Good Morning, 0bservers!

    
     
Pretty quiet again up on ol' Sol yesterday, with solar winds remaining calm. They peaked just under 350 KPS around 0800 UTC yesterday and moved steadily downward, hitting a nadir of 280 KPS just before 0900 UTC before hopping back up to around 300 KPS. Particle Density also trended downward yesterday, but since midnight UTC it has made a very slow rise. Temperatures took a significant drop by almost a thousand degrees Kelvin around 1800, dropping below 4000°K, then fluctuating between there and 4400°K, but it dropped to a low of about 3700°K twice (2300 UTC and 0500 UTC) before climbing back to a current 4300°K. Bt/Bz polarities stayed quite close, clashing several times, which caused some early (and minor) Phi Angle instability, but that seemed to calm down around 1300 UTC and has stayed relatively stable since then. The KP-Index looks like a downward staircase, with three KP-2s, then three KP-1s, and finishing out the chart with five KP-0s. NOAA is forecasting a possible minor geomagnetic storm (KP-4) in the early morning hours of Friday, but that's incoming the coronal stream. Might even see a KP-6 over the weekend. The Magnetometer's sine wave pattern is nominal, but slightly higher than yesterday's rather shallow readings. The Proton Flux is also nominal, but the Electron Flux levels did briefly cross the Alert Threshold around 1700 UTC, and it may do that again today if the current trend line continues. No major spikes on the X-Ray Flux chart, just a few short bumps into or slightly above Class B, with a slightly lower background radiation level. The second portion of that Southern coronal hole system is crossing the midpoint right now, and its latitudinal structure suggests it'll be doing that for at least another day. Seeing a lot of glow along the Eastern lim, both North and South, and there's also a bright spot about 20° South of the equator that's incoming as well. LASCO C3 is showing no active ejections, but the Western lim is showing a continuing bright area at the equator and around 50° South, both pointing ahead of Earth's orbit. The Magnetogram is showing Beta complexity at a minimum on that new sunspot group, and the departing Southern group approaching the Western lim appears to be destabilizing (but is still magnetically complex, so it might have a nasty surprise once it crosses to the "dark" side of the Sun).
* * *
A new video from Suspicious0bservers, "THE SIGNS | The Disaster Timeline".
 
Enjoy!
  
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Wednesday, August 4, 2021

CubeSat becomes first craft to fly with ESA's standardized "space brain"

By David Szondy, August 01, 2021


The OPS-SAT running the new "space brain" software
ESA
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ESA has flown a CubeSat with the agency's standardized "brain" that will be used on all future European space missions. On June 26, the OPS-SAT space lab went into Earth orbit with a computer running the European Ground System – Common Core (EGS-CC) software that will be common to all European space missions from 2025.


In the early days of the 1960s, each spacecraft, unless it was part of a series with a high failure rate, was essentially a one-off. This meant that space engineers were essentially reinventing the wheel in terms of not only the spacecraft itself, but also its avionics, computers, and the software to control it. This resulted in a lot of remarkable innovations, but the process was also slow, expensive, inflexible, and resulted in spacecraft that could only be controlled by one ground control system.

Since then, there's been much more of a push to create standard buses, standard components, and generally finding ways to assemble spacecraft with off-the-shelf parts. This led to cheaper, more flexible designs that can be developed in a more timely manner.

Based on years of development by ESA, European national space agencies, and space industries, the EGS-CC is being tested using a CubeSat about the size of a loaf of bread to avoid risking the new operational software on a proper space mission. During the recent test, the OPS-SAT received routine commands and sent back data to mission control at the ESOC Operations Centre in Darmstadt, Germany.

Animated rendering of a future debris capture mission
ESA

The new software will be used across the board on missions ranging from monitoring the Earth's environment to deep-space missions to running constellations of satellites dedicated to clearing space debris. The EGS-CC will not only handle conventional spacecraft, but also future designs that incorporate artificial intelligence.

The idea is not only to openly provide European operators with a common core software that can be easily tailored to specific spacecraft and missions, but also to allow for greater collaboration between the various agencies. In addition to the craft themselves, this also applies to control systems, which means that a mission can be operated by different agencies, passing control from one to another as needed, resulting in a "European Network of Centers."

This will be particularly important for removing space debris, which will involve a number of spacecraft provided by different agencies that will need to work together under unpredictable conditions.

"At its heart, this new software marks an important step in bringing to life the space technologies of the future," says Rolf Densing, Head of ESA’s ESOC Operations Centre. "Close cooperation between space agencies and industry has made this possible, opening up opportunities for all space entities in Europe to fly exciting, innovative and important missions through space."

Source: ESA




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Posted by Charles Edward


SPACE - S0 - 20210804 - New Solar Forecast, 4 Paths to the Micronova

SPACE - S0 - 20210804 - New Solar Forecast, 4 Paths to the Micronova

Good Morning, 0bservers!

    
     
Solar wind speeds continued their downward trends all through yesterday, until just prior to midnight UTC. At that point, it jumped from 300 KPS to just over 440 KPS before coming right back down. At that point, we lost readings from both the DSCOVR and ACE satellites for a few hours. Current speed readings are in the 320-340 KPS range, Particle Density is elevated but doesn't appear to be critical, the Temperature is in the 4700°K-5100°K range (dropping somewhat yesterday's peak of 5300°K). The Phi Angle is mostly steady despite a few polarity collisions on the Bt/Bz chart. It does not appear that such a collision was the cause of those near-midnight UTC spikes, however. Not exactly sure what caused that, hopefully Ben will have some insights in the video. The KP-Index is far calmer than late Monday night, so we're back in KP-1 to KP-2 range. The Magnetometer has returned to a more shallow sine wave, and we're also getting nominal readings from the Proton Flux and Electron Flux charts. That said, those charts are also showing an outage around the same time as the other satellites, so this wasn't a "glitch" or a software issue, something must've hit them pretty hard. The X-Ray Flux chart is showing a pretty solid flare into upper Class B range around 0400 UTC, but since then the background radiation has moved back down to upper Class A. The second Southern coronal hole should be coming into range for Earth in the next 18-24 hours, and there's still a good portion of the Northern polar hole which may have a lesser effect. The other video loops did show a release in the new sunspot group in the Southwest around the time as the X-Ray spike, but it was not what you'd call spectacular. No really bright flaring at any of the wavelengths.
  
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Tuesday, August 3, 2021

First additively-manufacture thermal protection shield is going to space

AUGUST 2, 2021, by Oak Ridge National Laboratory

Northrop Grumman’s Cygnus spacecraft atop the company’s Antares rocket lifts off Feb. 20, 2021, to deliver important science and cargo to the International Space Station on the company’s 15th commercial resupply services mission for NASA. 
Credits: NASA

A research team at Oak Ridge National Laboratory have 3D printed a thermal protection shield, or TPS, for a capsule that will launch with the Cygnus cargo spacecraft as part of the supply mission to the International Space Station. The launch will mark the first time an additively manufactured TPS has been sent to space.

Scientists worked with NASA to develop materials designed to withstand extreme temperatures encountered when objects reenter the atmosphere. The TPS protects a basketball-sized capsule that was developed by the University of Kentucky as a testbed for entry system technologies.

"This is an opportunity to gain flight experience on new materials," ORNL's Greg Larsen said. "Additive manufacturing enables automated, rapid production and opens up new design opportunities for using lightweight materials in spacecraft."

Equipped with sensors that record and transmit data to monitor performance, the capsule is anticipated to return to earth before the end of 2021.

A 3D printed thermal protection shield, produced by ORNL researchers for NASA, is part of a cargo spacecraft bound for the International Space Station. The shield was printed at the Department of Energy’s Manufacturing Demonstration Facility at ORNL. 
Credit: ORNL, U.S. Dept. of Energy
(screen shot of 1 sec. vid CC)


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SPACE - S0 - 20210803 - Solar Storm, Major Field Variations

SPACE - S0 - 20210803 - Solar Storm, Major Field Variations

Good Morning, 0bservers!

    
     
Solar winds remained relatively low but somewhat variable throughout yesterday, staying in the 360-420 KPS range throughout. It started to lower significantly around 0230 UTC, dropping to below 340 KPS but bumped back up to 380 at 0900 UTC. This is a bit odd considering the Particle Density chart, which rose significantly starting at 0900 UTC before a significant yet brief drop around 1600-1900 UTC before yet another even higher climb with another longer drop starting just before midnight UTC. Temperatures had been riding near the 5000°K before dropping nearly 800°K around 0900, and actually hitting 4000°K at 2000 UTC before a significant rise after 0200 UTC to nearly 5300°K. The Bt/Bz gaps were quite large during the afternoon and early evening before they started colliding around 2300 UTC, then gapping again for a couple of hours before a series of sustained polarity clashes for nearly 90 minutes. Naturally the Phi Angle was pretty scrambled during that period, but since the collisions have stopped the Phi Angle polarity has stabilized to the 50°-60° range. Those Particle Density elevations finally showed up on the KP-Index, where we had a KP-4 (minor geomagnetic storm) reading at 1800, followed by a KP-5 (level 1 storm), and then two more KP-4s directly afterward. By the bye, yesterday's forecast from NOAA completely missed that. We're back in the green now with a KP-2 and KP-3 as the last two readings. The Magnetometer did a pretty high spike to nearly 150 nT before dropping below 60 nT about 12 hours later (the latter number still well above the alert threshold of 40 nT). The Proton Flux and Electron Flux charts were nominal, but the latter chart did show an elevation in readings that was getting pretty close to the threshold line around 1400-1500 UTC before going back down.  The X-Ray Flux showed a very small spike just above the Class B flare line around 1700. Background radiation did spend most of the day increasing steadily as well, and that too is just now reaching Class B. The coronal hole systems, both North and South, began their transit across the midpoint around 0200 UTC, and they'll be doing that most of today. The Southern hole has a longer component than the North (excluding the polar region) and will keep the flow up for at least another day. Didn't see any flaring or ejections at 131Ă… or 304Ă…, however, and that's confirmed on the LASCO C3. I am seeing something new on the Solar Visible Light image, though - a small-ish pair of dark spots, probably a newly developing sunspot group. It does show up on the Magnetogram as well as tightly clustered, probably a minimum Beta-Delta complexity. The "good" news is it is pretty far South (perhaps 60° or so) and it is well past the midpoint and already about two days from the Western lim, so unless it does something spectacularly nasty we should be good.
  
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Monday, August 2, 2021

Thales to Provide New Avionics Equipment for Dassault Aviation Rafale

23.07.2021


Thales has received an order from the French defence procurement agency (DGA) for 350 Scorpion® helmet-mounted sight and display systems and 400 digital multi-function displays.

The systems deliver enhanced tactical situational awareness and slave the weapon or mission systems to the pilot’s line of sight to improve the effectiveness of air operations.

This new equipment will further enhance the operational effectiveness of the Rafale F4 standard.

Thales has been awarded the contract to supply Scorpion® helmet-mounted sight and display systems and digital multi-function displays for all the Dassault Aviation Rafale aircraft in service with the French Air and Space Force and the French Navy.

From reconnaissance to air defence and precision strike missions, the Rafale has helped ensure the success of countless military operations. But future aircrews will have to analyse more data in less time on combat missions carried out in increasingly complex environments. Coupled with the aircraft's weapon systems, the Scorpion® helmet-mounted sight and display enhances tactical situational awareness and enables crews to respond more quickly and with greater agility to a whole range of threats. Its progressive rollout on the Rafale F4 standard will be a decisive advantage in ensuring the success of airborne missions and protecting populations.

The helmet-mounted display symbology brings together information from the aircraft’s onboard sensors to help pilots perform their missions even in the most challenging situations. It creates a continuum between the cockpit and the outside world to radically improve awareness of the tactical situation. Coupled with the weapon system, the display can be used to designate and track targets anywhere in the crew's field of view in daylight and at night.

Scorpion® delivers all of these capability enhancements in addition to the protection and survivability functions of a conventional flight helmet. It is optimised for weight and balance to maximise pilot comfort and mission effectiveness.

The 400 digital multi-function displays on order will replace the lateral displays on France's in-service Rafale aircraft, which are primarily used to inform the pilot about the status of the aircraft's systems and provide imagery from its onboard sensors. The new equipment offers a larger display area, an improved touchscreen interface and greater processing power.

“When the success of a mission is decided in a fraction of a second, aircrews must be able to understand the tactical environment quickly and interact intuitively with the aircraft’s systems. We are delighted to have this opportunity to provide future Rafale F4 crews with an operational advantage that will be critical to the success of their missions, thanks to latest-generation equipment offering advanced display capabilities and enhanced interaction with the weapon systems.” Jean-Paul Ebanga, Vice President, Flight Avionics, Thales.

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SPACE - S0 - 20210802 - Magnetic Biology, Solar Cycle Progression, Nova Jumpers

SPACE - S0 - 20210802 - Magnetic Biology, Solar Cycle Progression, Nova Jumpers

Good Morning, 0bservers!

    
     
Space weather remains in an overall calm state. Solar Wind Speeds continued their slow decline all through yesterday and this morning, dropping below the 400 KPS level around 0300 UTC with the current range 370-390 KPS. We did see a brief dip down to 350 KPS around 0930 UTC. Particle Density, on the other hand, started a precipitous rise around 0800 UTC. Temperatures were riding just under the 5000°K line through most of yesterday, but then briefly popped above it around 0600 UTC before dropping to around 4100°K at 0930 UTC. Phi Angle readings were not too variable, but two Bt/Bz polarity collisions at 1000 and 1200 UTC did cause a pretty sharp shift. The Phi Angle dis restabilize a few hours later, with a new "skip" coming around 0930. Bt/Bz readings beyond the collisions had the positive polarity mostly steady with the negative more variable, but both started a precipitous rise above the zero-line a short while ago. The KP-Index was quite calm, with only a single KP-2 reading at 0300 UTC Sunday followed by mostly KP-1s and a couple of KP-0s scattered in for good measure. The Magnetometer's sine wave pattern is shallowing again for the last two days, so we should see another day of that before the high/low kicks in. Electron Flux and Proton Flux readings are steady and nominal. X-Ray Flux readings did show a flare on Saturday mid-afternoon UTC with a slow/steady decline into early Sunday morning. There haven't been any further flares, and the background radiation is only slightly higher than before the spike. This morning's ENLIL Spiral is showing a slight CME "ptoo" (yes, that is a scientific term) heading out well ahead of our orbit. It doesn't appear to be visible on any of the video loops, but I did see it on the LASCO C3 as broad and quite diffuse. However, what IS visible at 173Ă… is a rather large Northern polar coronal hole, which has connected to another hole trailing down to the mid-latitudes. There's also a further hole South of the equator with a third (fourth?) hole about two days behind it. That one is just ahead of a couple of new bright spots which are just crossing the Eastern lim. Because of those coronal holes, there's an elevated earthquake risk for the next couple of days, but I'm not seeing any forecast from NOAA for elevated particle density or KP-Index warnings.
* * *
A new video from Suspicious0bservers, "Geomagnetic Climate Science | Mini Info Nugget". It's less than three minutes, but it's packed with some pretty solid information.
 
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Defense News:

US military warns China is building more nuclear missile silos



https://www.militarytimes.com/news/your-military/2021/07/30/us-military-warns-china-is-building-more-nuclear-missile-silos/


TAIPEI, Taiwan — The U.S. military is warning about what analysts have described as a major expansion of China’s nuclear missile silo fields at a time of heightened tension between Beijing and Washington.

Researchers at the Federation of American Scientists estimate that China has approximately 250 underground missile silos under construction after they used satellite imagery to identify a new field being built in western China.

U.S. Strategic Command tweeted a link Wednesday to a story in The New York Times on the federation’s findings, which were published this week.

“The public has discovered what we have been saying all along about the growing threat the world faces and the veil of secrecy that surrounds it,” said Strategic Command, which oversees America’s nuclear arsenal.

The field in the Xinjiang region is the second one reported this summer. In June, researchers at the James Martin Center for Nonproliferation Studies in California identified another field under construction in neighboring Gansu province.

China has not commented on the reports. Asked about the latest one, the Foreign Ministry said Friday that it was not aware of the situation.

The reports come at a time when relations between the U.S. and China have plunged to their worst level in decades. The two nations remain sharply at odds over a range of issues, including trade, technology, cybersecurity, human rights and China’s increasingly assertive foreign policy under President Xi Jinping.

The expansion of China’s nuclear force would likely factor into any U.S. calculations for potential military confrontations over flashpoints such as Taiwan or the South China Sea.


China building more than 100 ‘nuclear’ missile silos in desert , 1 Jul 2021


The outspoken editor of the state-owned Global Times newspaper said this week that U.S. institutions and the media are hyping the reports about the missile fields to pressure China, but that the nation shouldn’t be cowed.

“Look at what American politicians are saying about China and look at the provocative actions of their warplanes and warships near China,” Hu Xijin said. “China must fully step up construction of its military force and nuclear deterrence as the cornerstone of its national security.”

Both sites are around 800 square kilometers (300 square miles). Ground-based silos can house intercontinental ballistic missiles. Spreading the silos across such a wide area makes targeting the field much more complicated. Analysts say some of the silos may serve as decoys as well.

“The Chinese missile silo program constitutes the most extensive silo construction since the U.S. and Soviet missile silo construction during the Cold War,” researchers Matt Korda and Hans Kristensen wrote in the Federation of American Scientists report.

Kuo Yu-jen, a defense studies expert at the Institute for National Policy Research in Taiwan, said it’s very difficult to get an accurate count of the underground silos of any country, but that the recently released satellite imagery looks “very, very similar” to missile silos.

He characterized the findings as a warning by the U.S. to others that China, in developing its nuclear weapon capabilities, is violating an international consensus geared toward nuclear disarmament.

“It’s also to let Russia know. China, if it increases its number of missiles, it threatens not only the U.S., but also Russia and Europe,” said Kuo, the director at the Institute for National Policy Research in Taiwan.

The U.S. and Russia, who have the world’s largest nuclear arsenals, held inconclusive talks this week in Geneva in a bid to avoid a new nuclear arms race.

China’s nuclear arsenal is estimated by the Stockholm International Peace Research Institute at 350 warheads, while the United States or Russia each has about 6,000. The Pentagon says China will at least double the size of its arsenal in 10 years.

The recent research follows a finding by Kristensen in February of construction of 11 underground silos at a vast missile training range near Jilantai in north-central China.


Sunday, August 1, 2021

Astronomers develop sky model to help ultralong-wavelength observations

JULY 30, 2021, by Zhang Nannan, Chinese Academy of Sciences

The predicted sky maps, from left to right, at 10, 3 and 1 MHz. 
Credit: Cong et al. 2021
(colour renditions,   4.6-6.0 left,   6.2 - 7.2 centre,     6.7 - 8.2 right    CC)

(Added by CC
Frequency,    Wavelength,     1/20 Wavelength
1 MHz,         300 meters,          15 meters     
        10 MHz,        30 meters,              1.5 meters           )

The radio sky at frequencies below ~30 MHz, particularly below ~10 MHz, is still largely unknown. Due to the absorption and distortion by the ionosphere, it is quite difficult to receive radio signal of such ultra-long wavelength by telescopes on Earth.

Some future space projects have been proposed to map the ultra-long wavelength sky with unprecedented resolution, and help to study the astrophysics behind.

To prepare for these upcoming projects, scientists from the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) recently developed a radio sky model that can be applied to this ultra-long wavelength band.

The study was published in The Astrophysical Journal on June 23.

Their sky map showed unique features at the ultralong wavelengths. They predicted the morphology of the radio sky down to ~1 MHz, which is very different from higher frequencies. For example, the high galactic latitude regions are brighter while the galactic plane is dark.

Moreover, one can see clearly the shadows of galactic spiral arms and the radio signal leaks from the gaps between arms. The model also provides interpretation for the observed global radio spectrum downturn at ~3-5 MHz.

The model (including the data and maps) can be accessed at https://github.com/Yanping-Cong/ULSA. The model has been used for designing instruments, developing imaging algorithm and optimizing survey strategy in the DSL project.


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