Monday, November 30, 2020

Defense News: U.S. Air Force buys Swiss B&T APC9K sub compact weapons

U.S. Air Force buys Swiss B&T APC9K sub compact weapons


The submachine guns are reportedly likely to end up with security personnel of the U.S. Air Force, possibly as replacements for Heckler & Koch MP5s


By Eyal Boguslavsky,  Israel Defense, November 29, 2020

https://www.israeldefense.co.il/en/node/46791


The APC9 submachine gun. Swiss special forces vesion .Photo: B&T

The value of the contract is said to be $128,300. The contract is called "Prototype Opportunity Notice (PON) for Sub Compact Weapon (SCW) System" which may indicate that it is an initial order for evaluation, with a potential for more. It’s not known which configuration the APC9 will be in, but the website said that it could be the APC9K PRO version

The APC9K sub compact weapon (Brugger & Thomet) with forward hand grip 


The Firearm Blog website reported that Swiss company B&T won an order to supply the U.S. Air Force with 65 APC9K 9×19 mm carbines with magazines and associated spare parts.  the option of up to 1,000 more. 


Right side view B&T APC9K will almost fit in the palm of your hand,if you have really big hands. (Photos: Chris Eger/Guns.com) Note: US Army model optic sights,without forward hand grip


Left side view B&T APC9K will almost fit in the palm of your hand,if you have really big hands. (Photos: Chris Eger/Guns.com) Note: US Army model optic sights,without forward hand grip



Test driving the Army's new B&T APC-9K | GearScout Down Lowe, Dec 6, 2019


The website said that it is likely, but not mentioned or confirmed, that the new B&T APC9Ks will end up with the security personnel of the U.S. Air Force and that they may replace Heckler & Koch MP5s. The Miami Beach Police Department is another user of the B&T APC9K.



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Oral insulin, by Israeli mom-son team, starts final trials to become world’s 1st

By NATHAN JEFFAY , 25 November 2020
https://www.timesofisrael.com/oral-insulin-by-israeli-mom-son-team-starts-final-trials-to-become-worlds-1st/

Illustrative: A woman injecting Insulin
 (Tuned_In via iStock by Getty Images)

An Israeli company has started final-stage tests of its oral insulin, bidding to become the first to make the product available on the international market.

The product started phase three trials under the US Food and Drug Administration in California on Monday, after 14 years of development. If all goes well, Oramed Pharmaceuticals says it expects type 2 diabetics to start taking its pills in just over three years, followed by type 1 diabetics after further testing.

“This has the potential to improve lives of hundreds of millions of diabetics worldwide,” Oramed CEO Nadav Kidron told The Times of Israel. “And by improving treatment it can reduce complications and, in turn, reduce the cost of treating diabetics.”

He said that the dosing tech that is being used for insulin has “very significant” potential for the creation of oral versions of other medical injections.

An Indian company, Biocon, is also working on oral insulin, but unlike Oramed it has not started advanced trials with the FDA, which is seen as the main path to the international market.

Insulin pills produced by Oramed (courtesy of Oramed Pharmaceuticals)




Oramed has big money behind its innovation: In 2015 it signed a $50 million licensing and investment deal with China’s Hefei Life Science & Technology Park Investments and Development Co. (HLST), a subsidiary of Chinese pharma giant Sinopharm, for the rights to its oral insulin capsule in China.

Kidron said his product transports insulin to where the body can make the best use of it — the liver, rather than the bloodstream, where it is currently delivered.

“One benefit of oral insulin is that we overcome the fear of the needle, but, more importantly, the insulin is being delivered directly to the liver.

“By taking it to the liver we are stopping the excessive production of glucose in the place where the production actually happens. Usually, injections go into the bloodstream and deal with glucose there instead of stopping production in the liver, its source.”

Pills will become a major source of insulin, he predicted, but they won’t replace injections entirely, as type 1 diabetics will still need to inject some of their doses.

He said that as well as helping insulin-dependent diabetics, it will allow doctors who are hesitant to start injections to prescribe occasional insulin via pills.



A diabetic woman measures her blood sugar (dragana991 via iStock by Getty Images)




The direct delivery minimizes side effects, especially weight gain which is the bane of many diabetics’ lives, Kidron said.

“So far in the phases of trials conducted to date, we [have] not seen the weight gain that is associated with injected insulin,” he commented.

In Phase 2b trials, the oral insulin showed a statistically significant lowering of hemoglobin A1c levels, a key marker of diabetes, without serious adverse events or weight gain.

The initial technology was developed at Hadassah Medical Center in Jerusalem — by Kidron’s mother, biochemist Miriam Kidron, today Oramed’s chief scientific officer. The Nobel laureate and Israel Prize-winning biochemist Avram Hershko is one of the company’s scientific advisers.

Oramed Pharmaceuticals CEO Nadav Kidron
 (courtesy of Oramed)



Oramed Pharmaceuticals chief scientific officer Miriam Kidron (courtesy of Oramed)




The big obstacle to oral insulin has been that the gut would harm it before it reaches the liver. Oramed’s tech overcomes this with a specially-coated pill that stays whole and releases the insulin as it gets to the liver.

“The fact we’re able to get the pill to the liver, which is exactly where the insulin is needed, is a major achievement,” said Kidron. “For nearly 100 years the world has looked for ways to be able to give insulin orally. This technology could be a real game-changer in how we treat diabetes.”



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SPACE - S0 - 20201130 - And Then the Sun Erupted, Welcome to Cycle 25

SPACE - S0 - 20201130 - And Then the Sun Erupted, Welcome to Cycle 25

Good Morning, 0bservers!

   
    
Wow. That was unexpected. We're starting with the X-Ray Flux today, because we had a MAJOR flare spike just after noon UTC. Bypassed the Class C flare range and went right up to the midpoint of Class *M*. At 131Å, 193Å and 304Å, those videos show a massive explosion and a major coronal mass ejection. Now, the good news - it was NOT facing Earth. This happened on a new sunspot group that was approaching the Eastern lim in the Southern part of the disc, so it hadn't yet crossed. The explosion (and that's what it was, seriously -- check out the videos over at SpaceWeatherNews) was facing about 100° away from (and behind) the planet. That said, that sunspot group WILL start facing us in a few short days. If you haven't got backup electronics stowed away in a PMFC (a Poor Man's Faraday Cage) you might want to consider a trip to the hardware store.
 
Now, there was OTHER solar weather yesterday as well. Like that boring old Solar Wind speed, don'tchaknow. It stayed mostly along the 380 KPS line until 0400 UTC, when a Particle Density rise precipitated an increase almost immediately to 420 KPS, with it continuing upward to a current 480 KPS. There was a mild temperature rise around the same time. The KP-Index stayed green all day and night, actually lowering through the day to KP-1 before popping up again to KP-3 right after midnight. Electron Flux and Magnetometer readings remain nominal.

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Sunday, November 29, 2020

China and Japan race to dominate the future of high-speed rail

NOVEMBER 25, 2020, by River Davis
https://techxplore.com/news/2020-11-china-japan-dominate-future-high-speed.html

Credit: Pixabay/CC0 Public Domain

Japan and China are racing to build a new type of ultra-fast, levitating train, seeking to demonstrate their mastery over a technology with big export potential.

Magnetic levitation, or maglev, trains use powerful magnets to glide along charged tracks at super fast speeds made possible by the lack of friction. A handful of short distance and experimental maglev trains are already in operation, but Asia's two biggest economies are vying to develop what would be the world's first long-distance intercity lines.

On one side is Central Japan Railway Co.'s 9 trillion yen ($86 billion) maglev that's expected to connect Tokyo and Osaka by 2037. On the other is China's 100 billion yuan ($15 billion) on-again, off-again project that will run between Shanghai and the eastern port city of Ningbo. After several false starts, it's now forecast to be completed by around 2035. Japan's is more expensive largely because of the amount of excavation that will be required to tunnel through the mountainous countryside.

If Japan and China are able to unveil their long-distance projects successfully by their due dates, it should give them a leg up when they look to export the next-generation technology, rail experts say. At stake is a share of the estimated more than $2 trillion global market for rail infrastructure projects.

"Maglev technology has huge export potential, and China and Japan's domestic projects are like shop windows into how the technology could be successfully implemented abroad," said Christopher Hood, a professor at Cardiff University who's studied and written a book about Japan's shinkansen.

Japan, the creator of the world's first bullet train, or shinkansen, has long been a top supplier to global fast-rail projects. Former Prime Minister Shinzo Abe targeted infrastructure exports including high-speed rail technologies as a key plank of economic growth.

But over the past decade, Chinese competitors, often willing to supply parts and know how for cheaper, have been catching up. In 2015, Japanese suppliers lost out to Chinese rivals in a bid to build Indonesia's first high-speed railway from capital Jakarta to Bandung in West Java. Japan was eventually asked to rejoin the project after it began to face significant delays.

Japan is a "strong rival" in developing regular bullet and high-speed maglev trains, according to an article that appeared in July in state-backed China Daily and that quoted a professor who specializes in railways. This "tough reality" has pushed China to make quick breakthroughs in developing maglev trains "to ensure the country has adequate market share in both future domestic and global markets," the report said.

The maglev line that will connect financial hub Shanghai and Ningbo, via Hangzhou, is part of a plan by China's Zhejiang provincial government to inject 3 trillion yuan into building out the province's rail lines.

"There's the sense that in the technological world, Japan is falling further and further behind China, so if it can realize this new technology first, it would be an issue of immense national pride," Hood said. He points to China's recent development of a high-speed train prototype that can run on different track gauges, something Japan has been trying to master with varying degrees of success for several years.

In 2016, the Abe government approved a 3 trillion yen loan to help JR Central fund the so-called Chuo Shinkansen maglev line, resulting in the project's end-date being moved up to 2037 from 2045. Still, the development faces a number of challenges that may cause it to be delayed, including opposition from a prefectural government concerned about the line's environmental impact.

"We are making every effort to get the Chuo Shinkansen up and running as soon as possible," said Yuri Akahoshi, a spokeswoman for JR Central, adding that the line is an "indispensable piece of infrastructure for the future of Japan."

JR Central runs tests on a 43-kilometer line in Yamanashi prefecture southwest of Tokyo, where its trains have routinely clocked operating speeds of over 500 kilometers per hour.

One of the countries that JR Central is looking to export its maglev technology to is the U.S., where it's working with partners to lay the groundwork for a maglev line that would connect Washington D.C. and New York, costing an estimated $10 billion for the first D.C. to Baltimore leg alone. If constructed, the train would cut travel time between the hubs to one hour from the current three, according to JR Central, making it even faster than flying.

The Japanese government has pledged several billion dollars in financial backing for the U.S. east coast project and JR Central has said it doesn't plan to charge licensing fees for the technology. Authorities are "fully supporting" the project due to its "importance for the overseas expansion of Japan's railway systems," JR Central's Akahoshi said.

Still, some analysts question whether maglev technology is a viable export without strong government support. Construction costs associated with maglev trains can run to double or triple that of regular high-speed rail lines because of the types of power and substations required, according to Bloomberg Intelligence Asia infrastructure analyst Denise Wong.

The state-owned short-distance maglev that connects Shanghai Pudong International Airport to the city and that started in 2002 has struggled to turn a profit, losing more than 1 billion yuan in its early years. The hefty price-tag of Japan's Chuo Shinkansen has also been thrown into question amid the coronavirus pandemic, which surveys predict may permanently alter the need for business travel between major centers.

"What's important is which project will be better able to justify the cost," Wong said, referring to the intercity maglevs planned by China and Japan. That's more crucial than "who gets there first," she said.

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Beijing powers up first domestically-built nuclear reactor, construction of 6 more underway at home & abroad

28 Nov, 2020, by Russian News RT
https://www.rt.com/news/508093-china-new--nuclear-reactor/

© China National Nuclear Corporation

China has plugged in its first domestically-built nuclear reactor with hopes to become more energy-independent and to export its design across the globe.

The country’s first reactor using Hualong One technology was successfully connected to the grid and started generating electricity at the Fuqing Nuclear Power Plant in the southeast Fujian Province on Friday morning, Chinese media reported.

The plant’s general manager, Zhao Hao, was quoted as saying that the reactor was functioning well. The official said there will be a series of tests and trial runs before the reactor starts commercial operation.

The China National Nuclear Corporation (CNNC) said the reactor has a lifespan of 60 years and meets “the strictest safety standard in the world.”

The construction of the new power unit at Fuqing began in 2015. Currently, six more Hualong One reactors are being built in China and other countries, the CNNC said.

Earlier this month, the reactor’s design was certified by the European Utility Requirements Organization, which serves as a technical advisory board for major European electricity producers.


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SPACE - S0 - 20201129 - Major Hit to the Ozone, Earth's Magnetic Shift, Solar Forcing

SPACE - S0 - 20201129 - Major Hit to the Ozone, Earth's Magnetic Shift, Solar Forcing

Good Morning, 0bservers!

   
    
We saw a return to calmer space yesterday as the solar winds slowed from a peak of 480 KPS yesterday to a current 380 KPS. Oddly enough, as the speed went down the Particle Density actually went up a bit. Temperatures did move downward, though. The KP-Index remained in the higher end of the green range, same as yesterday, and the Electron Flux and Magnetometer readings remain nominal. And the X-Ray Flux is pretty much the same as the last three days - upper Class B flare range for the baseline, with some occasional jumps into low-to-mid Class C. The one large sunspot group should be crossing the midpoint today, and the magnetogram of it is frankly scary. That sucka is YUUUUUUGE! Thankfully, though, they are not magnetically complex, despite their size, so we've at least got some "whew" room there...

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Saturday, November 28, 2020

Defense News: U.S. Army to release new tender for OMFV program next month

 

U.S. Army to release new tender for OMFV program next month


The Optionally Manned Fighting Vehicle program is seeking to replace the Army’s Bradley Fighting Vehicles   

By Eyal Boguslavsky, Israel Defense, 11/26/2020


A Bradley Fighting Vehicle. Photo: Cpl. Alisha Grezlik/115th Mobile Public Affairs Detachment

The U.S. Army announced that it plans to publish next month a new solicitation for the Optionally Manned Fighting Vehicle (OMFV) program. According to Brig. Gen. Ross Coffman, director of the Next Generation Combat Vehicles Cross-Functional Team, the competitive request for proposal (RFP) is expected to be released on or around December 18.

Defpost.com reported that the new request is slated to ask for concept designs of the OMFV that will transform the way infantry soldiers and maneuver formations fight on a battlefield. Up to five contracts will be awarded in June as part of that effort, followed by a second competitive RFP for a detailed design about a year and a half later. The Army plans to field the OMFV to both active and National Guard armored brigade combat teams starting in fiscal year 2028. About $4.6 billion is currently invested in the program for fiscal years 2020-2026. 


Current  model Bradley's 


The OMFV program is seeking to replace the U.S. Army’s Bradley Fighting Vehicles. The program is part of the larger Next Generation Combat Vehicles (NGCV) program. Other programs under the NGCV are the Armored Multi-Purpose Vehicle, or AMPV; Mobile Protected Firepower, or MPF; future robotic combat vehicles, or RCV; and the next-generation main battle tank. The NGCV-OMFV will be designed to maneuver soldiers in the future operating environment to a position of advantage to engage in close combat and deliver decisive lethality during the execution of combined arms maneuver. The NGCV must exceed current capabilities while overmatching similar threat class systems.

According to the Army, the vehicle must have the following capabilities:

• Optionally manned - It must have the ability to conduct remotely controlled operations while the crew is off platform.

• Capacity - It should eventually operate with no more than two crewmembers and possess sufficient volume under armor to carry at least six Soldiers.


The newest  Bradley M2A4 version with the IAI  Iron Fist light active protective system 

• Transportability - Two OMFVs should be transportable by one C-17 aircraft and be ready for combat within 15 minutes.

• Dense urban terrain operations and mobility - Platforms should include the ability to super elevate weapons and simultaneously engage threats using main gun and an independent weapons system.

• Protection - It must possess requisite protection to survive on the contemporary and future battlefield.

• Growth - It will possess sufficient size, weight, architecture, power, and cooling for automotive and electrical purposes to meet all platform needs and allow for pre-planned product improvements.



Finally! The Army begins testing new Bradley fighting vehicle, weapons of the world, Oct 30, 2020



• Lethality - It should apply immediate, precise and decisively lethal extended range medium caliber, directed energy, and missile fires in day/night all-weather conditions, while moving and/or stationary against moving and/or stationary targets. The platform should allow for mounted, dismount, and unmanned system target handover.

• Embedded Platform Training - It should have embedded training systems that have interoperability with the Synthetic Training Environment.

• Sustainability - Industry should demonstrate innovations that achieve breakthroughs in power generation and management to achieve increased operational range and fuel efficiency; increased silent watch, part and component reliability, and significantly reduced sustainment burden.


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Earth faster, closer to black hole in new map of galaxy

NOVEMBER 27, 2020, by National Astronomical Observatory of Japan
https://phys.org/news/2020-11-earth-faster-closer-black-hole.html

Position and velocity map of the Milky Way Galaxy. Arrows show position and velocity data for the 224 objects used to model the Milky Way Galaxy. The solid black lines show the positions of the Galaxy’s spiral arms. The colors indicate groups of objects belonging the same arm. The background is a simulation image. 
Credit: NAOJ

Earth just got 7 km/s faster and about 2000 light-years closer to the supermassive black hole in the center of the Milky Way Galaxy. But don't worry, this doesn't mean that our planet is plunging towards the black hole. Instead the changes are results of a better model of the Milky Way Galaxy based on new observation data, including a catalog of objects observed over the course of more than 15 years by the Japanese radio astronomy project VERA.

VERA (VLBI Exploration of Radio Astrometry, by the way "VLBI" stands for Very Long Baseline Interferometry) started in 2000 to map three-dimensional velocity and spatial structures in the Milky Way. VERA uses a technique known as interferometry to combine data from radio telescopes scattered across the Japanese archipelago in order to achieve the same resolution as a 2300 km diameter telescope would have. Measurement accuracy achieved with this resolution, 10 micro-arcseconds, is sharp enough in theory to resolve a United States penny placed on the surface of the Moon.

Because Earth is located inside the Milky Way Galaxy, we can't step back and see what the Galaxy looks like from the outside. Astrometry, accurate measurement of the positions and motions of objects, is a vital tool to understand the overall structure of the Galaxy and our place in it. This year, the First VERA Astrometry Catalog was published containing data for 99 objects.

Based on the VERA Astrometry Catalog and recent observations by other groups, astronomers constructed a position and velocity map. From this map they calculated the center of the Galaxy, the point that everything revolves around. The map suggests that the center of the Galaxy, and the supermassive black hole which resides there, is located 25800 light-years from Earth. This is closer than the official value of 27700 light-years adopted by the International Astronomical Union in 1985. The velocity component of the map indicates that Earth is traveling at 227 km/s as it orbits around the Galactic Center. This is faster than the official value of 220 km/s.

Now VERA hopes to observe more objects, particularly ones close to the central supermassive black hole, to better characterizes the structure and motion of the Galaxy. As part of these efforts VERA will participate in EAVN (East Asian VLBI Network) comprised of radio telescope located in Japan, South Korea, and China. By increasing the number of telescopes and the maximum separation between telescopes, EAVN can achieve even higher accuracy.


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SPACE - S0 - 20201128 - Solar Awakening, Electric Atmosphere, Galaxy Surprise

SPACE - S0 - 20201128 - Solar Awakening, Electric Atmosphere, Galaxy Surprise

Good Morning, 0bservers!

   
    
Solar wind speeds were riding the 420 KPS line most of yesterday, but when the Phi Angle readings shifted to a new orientation before midnight UTC, it caused a jump/destabilization in those winds. They spiked to a high of 480 KPS right at midnight UTC, and have been on an up-and-down ride between that and 380 KPS. Current readings are at 440 KPS. Particle Density lowered on the shift, while temperatures rose slightly. The KP-Index has stayed mostly in the upper part of the green range, although the readings did drop to KP-1 around the time of the shift, but rose again to KP-3 levels. No change in the Electron Flux or Magnetometer readings. Pretty much the same can be said about the X-Ray Flux as well - high Class B background readings with smaller spikes into lower Class C range.

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Friday, November 27, 2020

Defense News: The Abrams tank: the next generation

The Abrams tank: the next generation 

According to reports in the American media, the US military has started to plan (again) the next generation of the main battle tanks. The reports say there are three variants being considered

By Ami Rojkes Dombe, Israel Defense , 11/25/2020

https://www.israeldefense.co.il/en/node/46734

OMT, Variant 1


The US has revealed three possible models for the next generation of Abrams tanks for the American Army. The tank is not supposed to be ready before 2023, but in the US they are starting to plan. According to a report by Popular Mechanics, it is a tank that weighs about 70 tons. "The event, a three-day workshop, was held in early October at the U.S. Army’s Ground Vehicle Systems Center at Detroit Arsenal."


OMT, Variant 2


The American military tried a number of times to replace the Abrams. At a certain stage in the 2000s, the service spent billions without building a single vehicle. The October workshop was part of an additional effort, called Optionally Manned Tank (OMT), to plan a new manned tank. The Dead District blog gave technical details on the variants (click on the link to read).


OMT, Variant 3

The additions to the tank that are being considered include active defense (the Abrams was equipped with Rafael's "Trophy" system), a drone that will enable the crew to acquire targets, and improvements in the comfort of the crew. 

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STEVE’S LITTLE GREEN CANNONBALLS OF LIGHT

NOVEMBER 26, 2020 CAP ALLON
https://electroverse.net/steves-little-green-cannonballs-of-light/


Just when you thought “STEVE” couldn’t get any weirder, a new paper published in the journal AGU Advances reveals that the luminous purple ribbon is often accompanied by green cannonballs of light that streak through the atmosphere at 1000 mph.

[Below is an abridged version of Dr. Tony Phillip’s excellent article–the full version of which is available at spaceweatherarchive.com, dated November 22, 2020.]

STEVE (Strong Thermal Velocity Enhancement) is a relatively recent discovery, first spotted and photographed by Canadian citizen scientists around 10 years ago. It looks like an aurora, but it is not. The purple glow is caused by hot (3000 °C) rivers of gas flowing through Earth’s magnetosphere faster than 13,000 mph. This distinguishes it from auroras, which are ignited by energetic particles raining down from space.

“Citizen scientists have been photographing these green streaks for years,” says Joshua Semeter of Boston University, lead author of the new paper. “Now we’re beginning to understand what they are.”

There is a dawning realization that STEVE is more than just a purple ribbon, as photographers routinely catch it flowing over a sequence of green vertical pillars known as the “picket fence” (example shown below).

“Picket fence” below STEVE: 
Taken by Harlan Thomas on April 10, 2018 in Alberta, Canada.

These aren’t auroras either.

And now, Semeter’s team has identified yet another curiosity: “Beneath the picket fence, photographers often catch little horizontal streaks of green light,” explains Semeter: “This is what we studied in our paper.”

Entitled The Mysterious Green Streaks Below STEVE, Semeter’s research involved gathering as many images of these little horizontal streaks as possible, and citizen scientists across North America and New Zealand were only too happy to help:


In a few cases, the same streaks were captured by widely-separated photographers, allowing a triangulation of their position:


Upon analyzing dozens of high-quality images, the researchers came to these three conclusions:

1. The streaks are not in fact streaks, they are instead point-like balls of gas moving horizontally through the sky. In photos, the ‘green cannonballs’ are smeared into streaks by the exposure time of the cameras.

2. The cannonballs are typically 350 meters wide, and located about 105 km above Earth’s surface.

3. The color of the cannonballs is pure green–much more so than ordinary green auroras, reinforcing the conclusion that they are different phenomena.

So, what exactly are STEVE’s green cannonballs?

Semeter and his team believe they are a sign of turbulence: “During strong geomagnetic storms, the plasma river that gives rise to STEVE flows at extreme supersonic velocities. Turbulent eddies and whirls dump some of their energy into the green cannonballs.”

This idea may explain their prevalence of late: given ongoing waning of Earths magnetic field (thought to be tied to a GSM and Pole Shift), geomagnetic storms could-well be having a bigger impact closer to the ground, with streams of plasma penetrating deeper into Earth’s atmosphere.

Semeter’s musings may also explain their pure color, writes Dr. Phillips. Auroras tend to be a mixture of hues caused by energetic particles raining down through the upper atmosphere. The ‘rain’ strikes atoms, ions, and molecules of oxygen and nitrogen over a wide range of altitudes. A hodge-podge of color naturally results from this chaotic process. STEVE’s cannonballs, on the other hand, are monochromatic. Local turbulence excites only oxygen atoms in a relatively small volume of space, producing a pure green at 557.7 nm; there is no mixture.

“It all seems to fit together, but we still have a lot to learn,” concludes Semeter. “Advancing this physics will benefit greatly from the continued involvement of citizen scientists.”

According the mainstream position, however, when it comes to science, “you must not do your own research“. By this logic, citizen scientists around the world should immediately cease all endeavors and their groups be disbanded.

But why? What do the powers-that-be deem so threatening and dangerous with people exploring the reality around them, and what business is it of theirs how a person searches for the truth?

The elite’s plan, it now seems obvious, is to herd society down one very specific thought-path, a path which offers a very narrow set of answers to all life’s questions and problems. People are misled into thinking science is definitive, that there is one simplistic answer to each and every query–but science doesn’t work on consensus, and even the most seemingly far-reaching hypothesis, if properly and honestly devised, has about as much chance being proven correct as any widely-held theory.

Nothing at all is settled.

Questioning everything is key, and mistakes are part-and-parcel.

This is science.


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SPACE - S0 - 20201127 - C(lie)mate Models, Dusty Universe, Solar Watch

SPACE - S0 - 20201127 - C(lie)mate Models, Dusty Universe, Solar Watch

Good Morning, 0bservers!

   
    

Solar winds took a pretty substantial jump around midday yesterday after riding the 380 KPS line for nearly 24 hours. It peaked at nearly 480 KPS before calming around midnight UTC to the 400-440 KPS range. There was no precursor rise in Particle Density this time, but Temperatures did rise along with the wind speed. Doesn't look like this was caused by any Phi Angle push. The midmorning readings on the KP-Index were on the low side, but when the speed increased so did the geomagnetic buffering as it rose to KP-2s with a few KP-3s interspersed. Electron Flux and Magnetometer readings remain nominal. X-Ray Flux readings stayed in the upper Class B Flare range, with a couple of strong mid-Class C spikes from the sunspots. One of those was a pretty strong ejection from the new Northeast sunspot group. You can also see some sparking and surging from the large sunspot group in the Southern hemisphere as it continues to approach the midpoint. Other than the Northern polar coronal hole, there's not much developing on the surface in that regard, and the one up North is not in a position to develop an Earth-disrupting stream.

* * *

Another new video from Suspicious0bservers, "Grateful Thanks on Thanksgiving". Some rather enjoyable digs on "Professor" Dave in this one, folks...


Enjoy!

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Thursday, November 26, 2020

Space News: Bizarre ‘super planet’ discovered for first time with radio observations

 

Bizarre ‘super planet’ discovered for first time with radio observations


By Chris Ciaccia, Fox News , November 24, 2020



Artist's impression of the discovery dubbed, Elegast. ASTRON/Danielle Futselaar


Researchers have discovered a bizarre “super-planet” for the first time using radio observations, according to a new study.

Known as BDR J1750+3809 or Elegast, the “super-planet” is actually a brown dwarf, a celestial object that is too cold and small to be a star. The discovery was made by researchers at the University of Hawaii, working in conjunction with tools from NASA and the Low-Frequency Array (LOFAR) telescope in Europe.

“This work opens a whole new method to finding the coldest objects floating in the sun’s vicinity, which would otherwise be too faint to discover with the methods used for the past 25 years,” the study’s co-author, Michael Liu, said in a statement.

Brown dwarfs are generally harder to find using methods that astronomers normally use to find other stars. However, the light they emit at radio wavelengths was vital in the discovery of Elegast, the researchers added.

Since they lack the mass to trigger hydrogen fusion, they can’t be considered stars. Given their gaseous atmospheres, brown dwarfs resemble Jupiter and Saturn, the gas giants in our solar system, more than they resemble stars themselves.

“We asked ourselves, ‘Why point our radio telescope at cataloged brown dwarfs?'” the study’s lead author, Harish Vedantham, added. “Let’s just make a large image of the sky and discover these objects directly in the radio.”

With the discovery of BDR J1750+3809, the researchers hope that more brown dwarfs — the closest things to exoplanets — could be discovered with radio telescopes.

The research has been published in the Astrophysical Journal Letters.

More than 4,500 exoplanets have been discovered so far, with only a small portion thought to have the properties to contain life.

In October, a separate group of researchers discovered 24 potential “superhabitable” planets that may have conditions more suited to host life.



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