#dust ionizer

[kyodoindia]

Medical Equipment Suppliers in Delhi | Quick Mold Change System: Kyodo India

In the dynamic and critical industry of medical equipment supply, selecting the correct partner can have a considerable impact on the efficiency and efficacy of healthcare services. Among the leading players in this business, Kyodo India stands out as a top choice for medical equipment suppliers in Delhi. Kyodo India has built out a niche in the competitive market by focusing on innovation, quality, and client happiness. This article explores what makes Kyodo India a market leader in medical equipment supply, including revolutionary technology such as the Quick Mold Change System and Quick DIE Change System.

Why Kyodo India is a Top Medical Equipment Supplier in Delhi

1. Comprehensive Product Range

Kyodo India is well-known for its vast range of medical equipment, which caters to a variety of needs in the healthcare sector. The company provides high-quality items across several categories, such as diagnostic equipment, medicinal devices, and surgical instruments. Their extensive product line guarantees that healthcare facilities may obtain all of the necessary equipment from a single reliable provider, reducing procurement processes and increasing operational efficiency.

2. Commitment to Quality and Compliance

One of the main things that distinguishes Kyodo India from other medical equipment suppliers in Delhi is its continuous commitment to quality. Kyodo India’s products meet high quality and regulatory criteria. The company assures that its medical equipment fulfills worldwide quality standards, delivering dependable and safe solutions to healthcare practitioners.

Kyodo India’s commitment to these standards is critical in an industry where precision and dependability are essential. By upholding high quality standards, Kyodo India not only improves patient safety but also fosters trust among healthcare professionals and institutions.

3. Innovative Technologies: Quick Mold Change System and Quick DIE Change System

Kyodo India is in the forefront of integrating cutting-edge technology into its products. Two of the company’s notable technologies are the Quick Mold Change System and the Quick DIE Change System. These technologies are especially useful for increasing the efficiency of medical equipment manufacturing and maintenance.

Quick Mold Change System

Kyodo India created the Quick Mold Change System to expedite the manufacturing process by considerably lowering the time necessary to change molds. This technique is especially beneficial in the manufacturing of medical equipment, where precision and quick turnaround are essential.

The Quick Mold Change System offers the following advantages:

● Increased Productivity: By lowering mold change times, the technology enables more efficient production cycles, resulting in higher output and less downtime.

● Enhanced Flexibility: The system allows for quick adaptability to changing manufacturing requirements, making it easier to convert between different medical equipment models.

● Cost Efficiency: Faster mold changes lead to cheaper production costs and greater resource usage.

Quick DIE Change System

Kyodo India’s Quick DIE changing System, like the Quick Mold Change System, is designed to optimize the die changing process in manufacturing. This technology is critical for sectors that require frequent die replacements, such as those that manufacture sophisticated medical devices.

Key advantages of the Quick DIE Change System include:

● Reduced Changeover Time: The technology reduces the time required to swap dies, which improves overall production efficiency.

● Improved Accuracy: Quick DIE changes keep manufacturing operations precise and consistent, which is essential for high-quality medical equipment.

● Operational Flexibility: The system enables quick adjustments to meet changing production demands, improving the responsiveness of manufacturing operations.

4. Customer-Centric Approach

Kyodo India’s success as a major medical equipment supplier is also due to its customer-centric approach. The organization emphasizes knowing and meeting its clients’ individual demands. This technique involves the following:

● Personalized Service: Kyodo India offers bespoke solutions to address the specific needs of various healthcare facilities. Their team works closely with clients to ensure that the equipment delivered meets their operational requirements.

● Kyodo India provides full support, from pre-sales consultations to post-sales support, to guarantee that their equipment is integrated and used smoothly.

● Training and Maintenance: The organization educates healthcare workers on the proper use of equipment and provides maintenance services to ensure long-term performance and reliability.

5. Strong Industry Reputation

Kyodo India has established a solid name in the medical equipment business by delivering consistent results and exceeding customer expectations. The company’s commitment to providing high-quality products and innovative solutions has gained it the trust of several healthcare facilities in Delhi and elsewhere.

This reputation is evident in the good feedback and long-term connections that Kyodo India has built with its clients. The company’s dedication to excellence is demonstrated by its ability to continually meet and exceed client expectations.

Kyodo India is the Right Choice!

In the competitive landscape of medical equipment suppliers in Delhi, Kyodo India stands out for its diverse product offering, dedication to quality, and innovative technologies. The Quick Mold Change System and Quick DIE Change System are excellent examples of how the company uses sophisticated technology to improve manufacturing productivity and suit the changing needs of the healthcare sector.

For healthcare professionals looking for a dependable and forward-thinking medical equipment supplier, Kyodo India is an excellent alternative. Their commitment to quality, customer service, and technical innovation has positioned them as an industry leader.

Visit Kyodo India’s website to learn about their vast selection of medical equipment and technological solutions. Learn how Kyodo India can provide your healthcare facility with high-quality equipment and exceptional services.

[nasa]

A Tour of Cosmic Temperatures

We often think of space as “cold,” but its temperature can vary enormously depending on where you visit. If the difference between summer and winter on Earth feels extreme, imagine the range of temperatures between the coldest and hottest places in the universe — it’s trillions of degrees! So let’s take a tour of cosmic temperatures … from the coldest spots to the hottest temperatures yet achieved.

First, a little vocabulary: Astronomers use the Kelvin temperature scale, which is represented by the symbol K. Going up by 1 K is the same as going up 1°C, but the scale begins at 0 K, or -273°C, which is also called absolute zero. This is the temperature where the atoms in stuff stop moving. We’ll measure our temperatures in this tour in kelvins, but also convert them to make them more familiar!

We’ll start on the chilly end of the scale with our CAL (Cold Atom Lab) on the International Space Station, which can chill atoms to within one ten billionth of a degree above 0 K, just a fraction above absolute zero.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Just slightly warmer is the Resolve sensor inside XRISM, pronounced “crism,” short for the X-ray Imaging and Spectroscopy Mission. This is an international collaboration led by JAXA (Japan Aerospace Exploration Agency) with NASA and ESA (European Space Agency). Resolve operates at one twentieth of a degree above 0 K. Why? To measure the heat from individual X-rays striking its 36 pixels!

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Resolve and CAL are both colder than the Boomerang Nebula, the coldest known region in the cosmos at just 1 K! This cloud of dust and gas left over from a Sun-like star is about 5,000 light-years from Earth. Scientists are studying why it’s colder than the natural background temperature of deep space.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Let’s talk about some temperatures closer to home. Icy gas giant Neptune is the coldest major planet. It has an average temperature of 72 K at the height in its atmosphere where the pressure is equivalent to sea level on Earth. Explore how that compares to other objects in our solar system!

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

How about Earth? According to NOAA, Death Valley set the world’s surface air temperature record on July 10, 1913. This record of 330 K has yet to be broken — but recent heat waves have come close. (If you’re curious about the coldest temperature measured on Earth, that’d be 183.95 K (-128.6°F or -89.2°C) at Vostok Station, Antarctica, on July 21, 1983.)

We monitor Earth's global average temperature to understand how our planet is changing due to human activities. Last year, 2023, was the warmest year on our record, which stretches back to 1880.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

The inside of our planet is even hotter. Earth’s inner core is a solid sphere made of iron and nickel that’s about 759 miles (1,221 kilometers) in radius. It reaches temperatures up to 5,600 K.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

We might assume stars would be much hotter than our planet, but the surface of Rigel is only about twice the temperature of Earth’s core at 11,000 K. Rigel is a young, blue star in the constellation Orion, and one of the brightest stars in our night sky.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger 

We study temperatures on large and small scales. The electrons in hydrogen, the most abundant element in the universe, can be stripped away from their atoms in a process called ionization at a temperature around 158,000 K. When these electrons join back up with ionized atoms, light is produced. Ionization is what makes some clouds of gas and dust, like the Orion Nebula, glow.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

We already talked about the temperature on a star’s surface, but the material surrounding a star gets much, much hotter! Our Sun’s surface is about 5,800 K (10,000°F or 5,500°C), but the outermost layer of the solar atmosphere, called the corona, can reach millions of kelvins.

Our Parker Solar Probe became the first spacecraft to fly through the corona in 2021, helping us answer questions like why it is so much hotter than the Sun's surface. This is one of the mysteries of the Sun that solar scientists have been trying to figure out for years.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Looking for a hotter spot? Located about 240 million light-years away, the Perseus galaxy cluster contains thousands of galaxies. It’s surrounded by a vast cloud of gas heated up to tens of millions of kelvins that glows in X-ray light. Our telescopes found a giant wave rolling through this cluster’s hot gas, likely due to a smaller cluster grazing it billions of years ago.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Now things are really starting to heat up! When massive stars — ones with eight times the mass of our Sun or more — run out of fuel, they put on a show. On their way to becoming black holes or neutron stars, these stars will shed their outer layers in a supernova explosion. These layers can reach temperatures of 300 million K!

Credit: NASA's Goddard Space Flight Center/Jeremy Schnittman

We couldn’t explore cosmic temperatures without talking about black holes. When stuff gets too close to a black hole, it can become part of a hot, orbiting debris disk with a conical corona swirling above it. As the material churns, it heats up and emits light, making it glow. This hot environment, which can reach temperatures of a billion kelvins, helps us find and study black holes even though they don’t emit light themselves.

JAXA’s XRISM telescope, which we mentioned at the start of our tour, uses its supercool Resolve detector to explore the scorching conditions around these intriguing, extreme objects.

Credit: NASA's Goddard Space Flight Center/CI Lab

Our universe’s origins are even hotter. Just one second after the big bang, our tiny, baby universe consisted of an extremely hot — around 10 billion K — “soup” of light and particles. It had to cool for a few minutes before the first elements could form. The oldest light we can see, the cosmic microwave background, is from about 380,000 years after the big bang, and shows us the heat left over from these earlier moments.

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

We’ve ventured far in distance and time … but the final spot on our temperature adventure is back on Earth! Scientists use the Large Hadron Collider at CERN to smash teensy particles together at superspeeds to simulate the conditions of the early universe. In 2012, they generated a plasma that was over 5 trillion K, setting a world record for the highest human-made temperature.

Want this tour as a poster? You can download it here in a vertical or horizontal version!

Credit: NASA's Goddard Space Flight Center/Scott Wiessinger

Explore the wonderful and weird cosmos with NASA Universe on X, Facebook, and Instagram. And make sure to follow us on Tumblr for your regular dose of space!

[foone]

The best thing about Star Trek is that there are two possibilities:

1. All of Starfleet is like this. Every ship keeps getting stuck in negative space wedgies where they become their own parents and accidentally marry JFK while learning a lesson about what it means to be human, every week

2. Only the ships/stations we see are like this. Most ships spend their time ferrying diplomats around, delivering supplies, and charting nebulae. The diplomats never have a dark secret that endangers the ship. The supplies get there in time, and they never have to play a deadly game with a sufficiently advanced alien to survive, and the nebulae? Beautiful, but they're just a bunch of ionized hydrogen and assorted space dust. They never conceal a romulan battle fleet ready to invade Thrackus VII that's only uncovered because a teenager accidentally beats them all at space checkers.

These are the only two possibilities. And they are both hilarious.

Either there's an entire interstellar organization that's constantly tripping into weird science shit and plots against the universe and alien worlds where everyone has to eat their shoes or they are put to death...

Or there are like 8 ships out there which are just SO WEIRD and the rest of the organization is like "oh God not them again. We sent them to go stop an asteroid and they got their whole ship duplicated, one of the crew murdered their other self, they blew up their ship to stop aliens from turning them into spiders, then went back in time to stop space Nazis from killing Alexander Graham Bell and preventing the invention of the communicator. Next time, just send the USS Hatshepsut. The last weird thing that happened to them is that once they left Starbase 17 only to discover a week later that they'd gotten 20,000 boxes of self-sealing stembolts instead of oscillation overthrusters by mistake, so they had to stop by Deep Space 4 and get some extra supplies."

Like I said, both of these possibilities are hilarious.

[apod]

2024 September 17

Melotte 15 in the Heart Nebula Image Credit & Copyright: Richard McInnis

Explanation: Cosmic clouds form fantastic shapes in the central regions of emission nebula IC 1805. The clouds are sculpted by stellar winds and radiation from massive hot stars in the nebula's newborn star cluster, Melotte 15. About 1.5 million years young, the cluster stars are scattered in this colorful skyscape, along with dark dust clouds in silhouette against glowing atomic gas. A composite of narrowband and broadband telescopic images, the view spans about 15 light-years and includes emission from ionized hydrogen, sulfur, and oxygen atoms mapped to green, red, and blue hues in the popular Hubble Palette. Wider field images reveal that IC 1805's simpler, overall outline suggests its popular name - the Heart Nebula. IC 1805 is located about 7,500 light years away toward the boastful constellation Cassiopeia.

∞ Source: apod.nasa.gov/apod/ap240917.html

[all-roads-are-now-bent]

Caldwell 33//NGC 6992//Eastern Veil Nubula. Photo taken and processed by me.

A cloud of heated and ionized dust located 2,400ly from earth. Part of the Cygnus Loop, this is the remnant of a star 20 times more massive than our sun that went supernova 10,000–20,000 years ago. At the time, the resulting explosion would have appeared brighter than Venus in the night sky and would have been visible during the daytime.

[mindblowingscience]

The sun warms the Earth, making it habitable for people and animals. But that's not all it does, and it affects a much larger area of space. The heliosphere, the area of space influenced by the sun, is over a hundred times larger than the distance from the sun to the Earth. The sun is a star that constantly emits a steady stream of plasma—highly energized ionized gas—called the solar wind. In addition to the constant solar wind, the sun also occasionally releases eruptions of plasma called coronal mass ejections, which can contribute to the aurora, and bursts of light and energy, called flares. The plasma coming off the sun expands through space, along with the sun's magnetic field. Together they form the heliosphere within the surrounding local interstellar medium—the plasma, neutral particles and dust that fill the space between stars and their respective astrospheres. Heliophysicists like me want to understand the heliosphere and how it interacts with the interstellar medium.

Continue Reading.

[brightestofcentaurus]

Orion Nebula

"The dusty side of the Sword of Orion is illuminated in this striking infrared image from the European Space Agency's Hershel Space Observatory. This immense nebula is the closest large region of star formation, situated about 1,500 light years away in the constellation of Orion. The parts that are easily observed in visible light, known alternatively as the Orion Nebula or Messier 42, correspond to the light blue regions. This is the glow from the warmest dust, illuminated by clusters of hot stars that have only recently been born in this chaotic region.

The red spine of material running from corner to corner reveals colder, denser filaments of dust and gas that are scattered throughout the Orion nebula. In visible light this would be a dark, opaque feature, hiding the reservoir of material from which stars have recently formed and will continue to form in the future.

Herschel data from the PACS instrument observations, at wavelengths of 100 and 160 microns, is displayed in blue and green, respectively, while SPIRE 250-micron data is shown in red.

Within the inset image, the emission from ionized carbon atoms (C+), overlaid in yellow, was isolated and mapped out from spectrographic data obtained by the HIFI instrument."

Image and information from NASA.

[thepastisalreadywritten]

The Year’s Most Spectacular Photos from the James Webb Telescope

By Jeffrey Kluger

December 22, 2023

Close to 1,500 light years from Earth lie a pair of baby stellar twins known as Herbig-Haro 46/47 — which are barely a few thousand years old.

A star the size of our sun, by contrast, takes an average of 50 million years to reach even the stellar equivalent of young adulthood It's Herbig-Haro 46/47's extreme youth that gives the formation more of a blob-like appearance than the stellar duo it is.

Young stars are buried in clouds of dust and gas, which they absorb as they grow. Sometimes, however the infant stars ingest too much material too fast.

When that happens, dust and gas erupts from both sides of the formation, giving the young pair their misshapen look.

But if you have patience — 50 million years worth of patience — what is a blob today will be stars tomorrow.

NASA, ESA, CSA. Image Processing: Joseph DePasquale (STScI)

A pair of brilliant stellar nurseries located 1,600 light years from Earth, the Orion Nebula and Trapezium Cluster are home to a relative handful of very young but very bright stars.

Four of the stars are easy to see with a simple, amateur, four-inch telescope.

One of the four — the beast of the young litter — is especially visible, a full 20,000 times brighter than our sun.

Apart from their four main stars, the Orion Nebula and Trapezium cluster contain approximately 700 additional young stars at various stages of gestation.

NASA, ESA, CSA/Science leads and image processing: M. McCaughrean, S. Pearson, CC BY-SA 3.0 IGO

(L): It’s not easy being a Wolf-Rayet star, like this specimen imaged by the Webb telescope at a distance of 15,000 light years.

A rare species of stellar beast — NASA estimates there are only 220 of them in a Milky Way galaxy with at least 100 billion stars — the Wolf-Rayet burns hot and burns fast, with temperatures 20 to 40 times the surface of the sun.

All of that rapidly expended energy causes the star to lose its hydrogen envelope quickly and expose its helium core.

The result: a very early and very violent death.

A star like our sun burns for about 10 billion years. As for a Wolf-Rayet? Just a few hundred thousand before it dissolves into cosmic dust.

NASA, ESA, CSA, STScI, Webb ERO Production Team

(R): If the Wolf-Rayet star dies an ugly and violent death, the celebrated Ring Nebula, photographed by the Webb at a distance of 2,000 light years from Earth, has been expiring beautifully.

The glowing remains of a sun-like star, the nebula was discovered in 1779 by the French astronomer Antoine Darquier de Pellepoix.

As the nebula throws off its outer layers of ionized gas, it reveals its characteristic blue interior, composed of hydrogen and oxygen that have not yet been expelled off by the nebula’s stellar wind.

ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University)

Dwarf galaxy NGC 6822 lives up to to its name — home to just 10 million stars, compared to the minimum of 100 billion in the Milky Way.

But what NGC 6822 lacks in numbers, it makes up in spectacle — which the keen eye of the Webb telescope has revealed.

Discovered in 1884 by American astronomer E.E Barnard, NGC 6822, is now known to have a prodigious dust tail measuring 200 light years across..

What's more, it's home to a dense flock of stars that glow 100,000 times brighter than our sun.

ESA/Webb, NASA & CSA, M. Meixnev

Spiral galaxies are often defined by uneven — and even ragged — arms.

But not galaxy M51, which lies 27 million light years from Earth and is defined by the tautness of its arms and the compactness of its structure.

M51 isn't alone in space. Nearby lies the companion galaxy NGC 5195.

The two galaxies are engaged in something of a gravitational tug of war — one that the NGC 5195 is winning.

NGC's constant gravitational pull is thought to account for both the tightly woven structure of M51's arms and for tidal forces that are thought lead to the creation of new stars in the arms.

ESA/Webb, NASA & CSA, A. Adamo (Stockholm University) and the FEAST JWST team

Just below Orion’s belt lies one of the most celebrated objects in the night sky: the Orion Nebula, a stellar nursery that is home to about 700 young stars.

This Webb image focuses not on the entirety of the nebula but on a structure in the lower left-hand quadrant known as the Orion Bar.

So named because of its diagonal, ridge-like appearance, the bar is shaped by the powerful radiation of the hot, young stars surrounding it.

ESA/Webb, NASA, CSA, M. Zamani (ESA/Webb), and the PDRs4All ERS Team

A baby by stellar standards, the IC 348 Star cluster is just five million years old and located about 1,000 light years from Earth.

Composed of an estimated 700 stars, IC 348 has a structure similar to wispy curtains, created by dust that reflects the light of the stars.

The conspicuous loop in the right hand side of the image is likely created by the gusting of solar winds blowing in the direction that, from Earth, would be west to east.

NASA, ESA, CSA, STScI, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA)

When it comes to galaxies, there's big and then there's huge and by any measure, Pandora's Cluster — more formally, known as Abell 2744 — qualifies as the latter.

Not just a galaxy, and not even a cluster of galaxies, Abell 2744 is a cluster of four clusters, which long ago collided with one another.

Located 3.5 billion light years from Earth, Pandora's Cluster measures a staggering 350 million years across.

The cluster's massive collective gravity allows astronomers to use it as a gravitational lens, bending and magnifying the light of foreground objects, making them easier to study.

NASA, ESA, CSA, I. Labbe (Swinburne University of Technology) and R. Bezanson (University of Pittsburgh). Image processing: Alyssa Pagan (STScI)

Webb was built principally to look at the oldest and most distant objects in the universe, some of 13.4 billion light years away.

But doesn't prevent the telescope from peering into its own back yard.

This image of Saturn and some of its 146 moons, rivals the images obtained by the Pioneer and Voyager probes.

NASA, ESA, CSA, STScI, Matt Tiscareno (SETI Institute), Matt Hedman (University of Idaho), Maryame El Moutamid (Cornell University), Mark Showalter (SETI Institute), Leigh Fletcher (University of Leicester), Heidi Hammel (AURA). Image processing: J. DePasquale (STScI)

Infant stars are born all over the universe, but the closest stellar birthing suite to Earth is the Rho Ophiuchi cloud complex, located just 460 light years distant.

A turbulent — even violent — place, Rho Ophiuchi is defined by jets of gas roaring from young stars.

Most of the stars in this comparatively modest nursery are more or less the size of the sun.

But one, known as S1, is far bigger — so much so that it is self-immolating, carving a great cavity around itself with its stellar wind, the storm of charged particle's all stars emit, though few with the gale-force power of S1.

NASA, ESA, CSA, STScI, Klaus Pontoppidan (STScI)

[shaythempronouns]

IC 5146 - the Cocoon Nebula (HaRGB)

An especially fun target to shoot, because it's a combination emission and reflection nebula. The red in its center is ionized hydrogen, which emits a deep red glow, but the areas around the nebula with fewer stars are filled with dust, which reflects nearby starlight to produce the pale blue glow at the nebula's apparent edges.

Shot at 1600mm with a 200mm RC telescope and a ZWO ASI533MM Pro. 2h of Ha integrated exposure time, plus 1h each of RGB data.

All images on my blog, unless noted, are shot from my backyard in Bortle 7 skies.

[rwby-soh]

“Wild Oat”

Sex: Female

Race: Human

Height: 5’7”

Age (circa 99 AGW): 18

Aura Density: Low

Aura Reserves: Below Average

Aura Color: Violet

Semblance: Retrocognition

Weapon: Morgan

Jacques Gele's youngest daughter. The oldest among the four Schnee family soap opera girls at Beacon and the leader of team BGEL. She puts up a bitchy and arrogant front in order to cover up her various insecurities, such as the loneliness she feels from how most of her extended family doesn’t want anything to do with her, the sense of abandonment she feels over her parents leaving her with a family friend to actually raise her, the fact that she’s a bastard child, how she feels useless because her Semblance (Retrocognition - the ability to read people’s memories by touching them) has next-to-no practical use in combat, or how she’s the weakest member of her team in both skill and strength. Belka’s weapon is a laser rifle-naginata combo named Morgan that can use specialized, exuberantly expensive Dust cores fuel and modify the attributes of the beams it shoots (such as using an ice dust core to create freeze rays, or a lighting dust core to ionize the beam). She’s unfortunately bullied by the hands of team SLVR, especially Alaska. Belka’s name and weapon of choice are references to the Belkan Federation and the Belkan War from Ace Combat.

[thefirststarr]

SPACEMAS DAY 11 ✨🪐🌎☄️☀️🌕

Ridges of glowing interstellar gas and dark dust clouds inhabit the turbulent Lagoon Nebula. Also known as M8, The bright star forming region is about 5,000 light-years away. It makes for a popular stop on telescopic tours of the constellation Sagittarius which lies toward the center of our Milky Way Galaxy. It is dominated by the red emission of ionized hydrogen atoms that are recombining with stripped electrons. This view of the Lagoon's central region reaches about 40 light-years across. The bright hourglass shape near the center of the frame is gas ionized by radiation and extreme stellar winds from a massive young star.

Image Credit: Josep Drudis

[mysticstronomy]

HOW IS OUR UNIVERSE EXPANDING??

Blog#308

Saturday, June 24th, 2023

Welcome back,

The universe was born with the Big Bang as an unimaginably hot, dense point. When the universe was just 10-34 of a second or so old — that is, a hundredth of a billionth of a trillionth of a trillionth of a second in age — it experienced an incredible burst of expansion known as inflation, in which space itself expanded faster than the speed of light. During this period, the universe doubled in size at least 90 times, going from subatomic-sized to golf-ball-sized almost instantaneously.

The work that goes into understanding the expanding universe comes from a combination of theoretical physics and direct observations by astronomers. However, in some cases astronomers have not been able to see direct evidence — such as the case of gravitational waves associated with the cosmic microwave background, the leftover radiation from the Big Bang.

A preliminary announcement about finding these waves in 2014 was quickly retracted, after astronomers found the signal detected could be explained by dust in the Milky Way.

According to NASA, after inflation the growth of the universe continued, but at a slower rate. As space expanded, the universe cooled and matter formed. One second after the Big Bang, the universe was filled with neutrons, protons, electrons, anti-electrons, photons and neutrinos.

During the first three minutes of the universe, the light elements were born during a process known as Big Bang nucleosynthesis. Temperatures cooled from 100 nonillion (1032) Kelvin to 1 billion (109) Kelvin, and protons and neutrons collided to make deuterium, an isotope of hydrogen. Most of the deuterium combined to make helium, and trace amounts of lithium were also generated.

For the first 380,000 years or so, the universe was essentially too hot for light to shine, according to France's National Center of Space Research (Centre National d'Etudes Spatiales, or CNES).

he heat of creation smashed atoms together with enough force to break them up into a dense plasma, an opaque soup of protons, neutrons and electrons that scattered light like fog.

Roughly 380,000 years after the Big Bang, matter cooled enough for atoms to form during the era of recombination, resulting in a transparent, electrically neutral gas, according to NASA. This set loose the initial flash of light created during the Big Bang, which is detectable today as cosmic microwave background radiation.

However, after this point, the universe was plunged into darkness, since no stars or any other bright objects had formed yet.

About 400 million years after the Big Bang, the universe began to emerge from the cosmic dark ages during the epoch of reionization. During this time, which lasted more than a half-billion years, clumps of gas collapsed enough to form the first stars and galaxies, whose energetic ultraviolet light ionized and destroyed most of the neutral hydrogen.

Although the expansion of the universe gradually slowed down as the matter in the universe pulled on itself via gravity, about 5 or 6 billion years after the Big Bang, according to NASA, a mysterious force now called dark energy began speeding up the expansion of the universe again, a phenomenon that continues today.

A little after 9 billion years after the Big Bang, our solar system was born.

The Big Bang did not occur as an explosion in the usual way one think about such things, despite one might gather from its name. The universe did not expand into space, as space did not exist before the universe, according to NASA. Instead, it is better to think of the Big Bang as the simultaneous appearance of space everywhere in the universe. The universe has not expanded from any one spot since the Big Bang — rather, space itself has been stretching, and carrying matter with it.

Originally published on space.com

COMING UP!!

(Wednesday, June 28th, 2023)

"IS THE MOON RUSTING??"

[apod]

2024 August 28

Tulip Nebula and Black Hole Cygnus X-1 Image Credit & Copyright: Anirudh Shastry

Explanation: When can you see a black hole, a tulip, and a swan all at once? At night -- if the timing is right, and if your telescope is pointed in the right direction. The complex and beautiful Tulip Nebula blossoms about 8,000 light-years away toward the constellation of Cygnus the Swan. Ultraviolet radiation from young energetic stars at the edge of the Cygnus OB3 association, including O star HDE 227018, ionizes the atoms and powers the emission from the Tulip Nebula. Stewart Sharpless cataloged this nearly 70 light-years across reddish glowing cloud of interstellar gas and dust in 1959, as Sh2-101. Also in the featured field of view is the black hole Cygnus X-1, which to be a microquasar because it is one of strongest X-ray sources in planet Earth's sky. Blasted by powerful jets from a lurking black hole, its fainter bluish curved shock front is only faintly visible beyond the cosmic Tulip's petals, near the right side of the frame.

∞ Source: apod.nasa.gov/apod/ap240828.html

[palmiz]

Lista dei brevetti per la modifica del clima.

Dal 1891 al 2023.

United States Patent and Trademark Office​.

...

0462795 – July 16, 1891 – Method Of Producing Rain-Fall

803180 – October 31, 1905 – Means for Producing High Potential Electrical Discharges

1103490 – August 6, 1913 – Rain-Maker

1225521 – September 4, 1915 – Protecting From Poisonous Gas In Warfare

1279823 – September 24, 1918 – Process and Apparatus for Causing Precipitation by Coalescence of Aqueous Particles Contained in the Atmosphere

1284982 – November 19, 1918 – Process and Apparatus for Procuring and Stimulating Rainfall

1338343 – April 27, 1920 – Process And Apparatus For The Production of Intense Artificial Clouds, Fogs, or Mists

1358084 – November 9, 1920 – Method of Producing Fog-Screens

1619183 – March 1, 1927 – Process of Producing Smoke Clouds From Moving Aircraft

1665267 – April 10, 1928 – Process of Producing Artificial Fogs

1892132 – December 27, 1932 – Atomizing Attachment For Airplane Engine Exhausts

1895765 – January 31, 1933 – Artificial Production of Fog

1928963 – October 3, 1933 – Electrical System And Method

1957075 – May 1, 1934 – Airplane Spray Equipment

1993316 – March 5, 1935 – Apparatus for and Method of Producing Oil Fog

2052626 – September 1, 1936 – Method of Dispelling Fog

2097581 – November 2, 1937 – Electric Stream Generator – Referenced in 3990987

2173756 – September 19, 1939 – Process of Producing Fog or Mist by Partial and Flameless Combustion

2352677 – July 4, 1944 – Artificial Fog Production

2476171 – July 18, 1945 – Smoke Screen Generator

2409201 – October 15, 1946 – Smoke Producing Mixture

2480967 – September 6, 1949 – Aerial Discharge Device

2527230 – October 24, 1950 – Method of Crystal Formation and Precipitation

2527231 – October 24, 1950 – Method of Generating Silver Iodide Smoke

2550324 – April 24, 1951 – Process For Controlling Weather

2582678 – June 15, 1952 – Material Disseminating Apparatus For Airplanes

2611992 – September 30, 1952 – Engine Exhaust Operated Fluent Material Distributor

2614083 – October 14, 1952 – Metal Chloride Screening Smoke Mixture

2633455 – March 31, 1953 – Smoke Generator

2688069 – August 31, 1954 – Steam Generator – Referenced in 3990987

2721495 – October 25, 1955 – Method And Apparatus For Detecting Minute Crystal Forming Particles Suspended in a Gaseous Atmosphere

2730402 – January 10, 1956 – Controllable Dispersal Device

2903188 – April 2, 1956 – Control of Tropical Cyclone Formation

2756097 – July 24, 1956 – Process for Weather Control

2801322 – July 30, 1957 – Decomposition Chamber for Monopropellant Fuel – Referenced in 3990987

2835530 – May 20, 1958 – Process for the Condensation of Atmospheric Humidity and Dissolution of Fog

2871344 – January 27, 1959 – Long Distance Communication System

2881335 – April 7, 1959 – Generation of Electrical Fields

2908442 – October 13, 1959 – Method For Dispersing Natural Atmospheric Fogs And Clouds

2962450 – November 29, 1960 – Fog Dispelling Composition

2963975 – December 13, 1960 – Cloud Seeding Carbon Dioxide Bullet

3019989 – February 6, 1962 – Atmospheric Space Charge Modification

2986360 – May 30, 1962 – Aerial Insecticide Dusting Device

3046168 – July 24, 1962 – Chemically Produced Colored Smokes

3056556 – October 2, 1962 – Method of Artificially Influencing the Weather

3126155 – March 24, 1964 – Silver Iodide Cloud Seeding Generator

3127107 – March 31, 1964 – Generation of Ice-Nucleating Crystals

3131131 – April 28, 1964 – Electrostatic Mixing in Microbial Conversions

3140207 – July 7, 1964 – Pyrotechnic Composition

3174150 – March 16, 1965 – Self-Focusing Antenna System

3234357 – February 8, 1966 – Electrically Heated Smoke Producing Device

3274035 – September 20, 1966 – Metallic Composition For Production of Hydroscopic Smoke

3284005 – November 8,1966 – Weather Control by Artificial Means

3300721 – January 24, 1967 – Means For Communication Through a Layer of Ionized Gases

3313487 – April 11, 1967 – Cloud Seeding Apparatus

3338476 – August 29, 1967 – Heating Device For Use With Aerosol Containers

3375148 – March 26, 1968 – Pyrotechnics Comprising Silver Iodate, Ammonium Nitrate, Nitrocellulose and Nitrate Esters

3378201 – April 16, 1968 – Method for Precipitating Atmospheric Water Masses

3410489 – November 12, 1968 – Automatically Adjustable Airfoil Spray System With Pump

3418184 – December 24, 1968 – Smoke Producing Propellant

3429507 – February 25, 1969 – Rainmaker

3432208 – November 7, 1967 – Fluidized Particle Dispenser

3441214 – April 29, 1969 – Method And Apparatus For Seeding Clouds

3445844 – May 20, 1969 – Trapped Electromagnetic Radiation Communications System

3456880 – July 22, 1969 – Method Of Producing Precipitation From The Atmosphere

3518670 – June 30, 1970 – Artificial Ion Cloud

3517512 – June 30, 1970 – Apparatus for Suppressing Contrails

3534906 – October 20, 1970 – Control of Atmospheric Particles

3545677 – December 8, 1970 – Method of Cloud Seeding

3564253 – February 16, 1971 – System And Method For Irradiation Of Planet Surface Areas

3587966 – June 28, 1971 – Freezing Nucleation

3595477 – July 27, 1971 – Fog Dispersing Method and Compositions

3601312 – August 24, 1971 – Methods of Increasing The Likelihood oF Precipitation By The Artificial Introduction Of Sea Water Vapor Into The Atmosphere Winward Of An Air Lift Region

3608810 – September 28, 1971 – Methods of Treating Atmospheric Conditions

3608820– September 20, 1971 – Treatment of Atmospheric Conditions by Intermittent Dispensing of Materials Therein

3613992 – October 19, 1971 – Weather Modification Method

3630950 – December 28, 1971 – Combustible Compositions For Generating Aerosols, Particularly Suitable For Cloud Modification And Weather Control And Aerosolization Process

USRE29142 – May 22, 1973 – Combustible compositions for generating aerosols, particularly suitable for cloud modification and weather control and aerosolization process

3659785 – December 8, 1971 – Weather Modification Utilizing Microencapsulated Material

3666176 – March 3, 1972 – Solar Temperature Inversion Device

3677840 – July 18, 1972 – Pyrotechnics Comprising Oxide of Silver For Weather Modification Use

3690552 – September 12, 1972 – Fog Dispersal

3722183 – March 27, 1973 – Device For Clearing Impurities From The Atmosphere

3748278 – July 24, 1973 – Process and Agents Having an Influence on the Weather

3751913 – August 14, 1973 – Barium Release System

3769107 – October 30, 1973 – Pyrotechnic Composition For Generating Lead Based Smoke

3784099 – January 8, 1974 – Air Pollution Control Method

3785557 – January 15, 1974 – Cloud Seeding System

3788543 – January 29, 1974 – Uniform Size Particle Generator

3795626 – March 5, 1974 – Weather Modification Process

3802971 – April 9, 1974 – Pyrotechnic Formulations for Weather Modification Comprising a Mixture of Iodates

3808595 – April 30, 1974 – Chaff Dispensing System

3813875 – June 4, 1974 – Rocket Having Barium Release System to Create Ion Clouds In The Upper Atmosphere

3835059 – September 10, 1974 – Methods of Generating Ice Nuclei Smoke Particles For Weather Modification And Apparatus Therefore

3835293 – September 10, 1974 – Electrical Heating Apparatus For Generating Super Heated Vapors

3858805 – January 7, 1975 – Ice Nucleation by Micas

3877642 – April 15, 1975 – Freezing Nucleant

3882393 – May 6, 1975 – Communications System Utilizing Modulation of The Characteristic Polarization of The Ionosphere

3887580 – June 3, 1975 – Method of Crystallization of Water in Supercooled Clouds and Fogs and Reagent Useful in Said Method

3896993 – July 29, 1975 – Process For Local Modification of Fog And Clouds For Triggering Their Precipitation And For Hindering The Development of Hail Producing Clouds

3899129 – August 12, 1975 – Apparatus for generating ice nuclei smoke particles for weather modification

3899144 – August 12, 1975 – Powder contrail generation

3915379 – October 28, 1975 – Method of Controlling Weather

3940059 – February 24, 1976 – Method For Fog Dispersion

3940060 – February 24, 1976 – Vortex Ring Generator

3990987 – November 9, 1976 – Smoke generator

3992628 – November 16, 1976 – Countermeasure system for laser radiation

3994437 – November 30, 1976 – Broadcast dissemination of trace quantities of biologically active chemicals

4042196 – August 16, 1977 – Method and apparatus for triggering a substantial change in earth characteristics and measuring earth changes

RE29,142 – February 22, 1977 – Combustible compositions for generating aerosols, particularly suitable for cloud modification and weather control and aerosolization process

4009828 – March 1 1977 – Organic Nucleating Agent for both Warm and Cold Clouds

4035726 – July 12, 1977 – Method of controlling and/or improving high-latitude and other communications or radio wave surveillance systems by partial control of radio wave et al

4096005 – June 20, 1978 – Pyrotechnic Cloud Seeding Composition

4129252 – December 12, 1978 – Method and apparatus for production of seeding materials

4141274 – February 27, 1979 – Weather modification automatic cartridge dispenser

4167008 – September 4, 1979 – Fluid bed chaff dispenser

4347284 – August 31, 1982 – White cover sheet material capable of reflecting ultraviolet rays

4362271 – December 7, 1982 – Procedure for the artificial modification of atmospheric precipitation as well as compounds with a dimethyl sulfoxide base for use in carrying out said procedure

4373391 – February 15, 1983 – Relative Humidity Sensitive Material

4396152 – August 2, 1983 – Aerosol Dispenser System

4402480 – September 6, 1983 – Atmosphere modification satellite

4412654 – November 1, 1983 – Laminar microjet atomizer and method of aerial spraying of liquids

4415265 – November 15, 1983 – Method and apparatus for aerosol particle absorption spectroscopy

4470544 – September 11, 1984 – Method of and Means for weather modification

4475927 – October 9, 1984 – Bipolar Fog Abatement System

4600147 – July 15, 1986 – Liquid propane generator for cloud seeding apparatus

4633714 – January 6, 1987 – Aerosol particle charge and size analyzer

4643355 – February 17, 1987 – Method and apparatus for modification of climatic conditions

4653690 – March 31, 1987 – Method of producing cumulus clouds

4684063 – August 4, 1987 – Particulates generation and removal

4686605 – August 11, 1987 – HAARP Patent / EASTLUND PATENT – Method and apparatus for altering a region in the earth’s atmosphere, ionosphere, and/or magnetosphere

4704942 – November 10, 1987 – Charged Aerosol

4712155 – December 8, 1987 – Method and apparatus for creating an artificial electron cyclotron heating region of plasma

4742958 – May 10, 1988 – Method for Making Artificial Snow

4744919 – May 17, 1988 – Method of dispersing particulate aerosol tracer

4766725 – August 30, 1988 – Method of suppressing formation of contrails and solution therefor

4829838 – May 16, 1989 – Method and apparatus for the measurement of the size of particles entrained in a gas

4836086 – June 6, 1989 – Apparatus and method for the mixing and diffusion of warm and cold air for dissolving fog

4873928 – October 17, 1989 – Nuclear-sized explosions without radiation

4948257 – August 14, 1990 – Laser optical measuring device and method for stabilizing fringe pattern spacing

1338343– August 14, 1990 – Process and Apparatus for the production of intense artificial Fog

4999637 – March 12, 1991 – Creation of artificial ionization clouds above the earth

5003186 – March 26, 1991 – Stratospheric Welsbach seeding for reduction of global warming

5005355 – April 9, 1991 – Method of suppressing formation of contrails and solution therefor

5038664 – August 13, 1991 – Method for producing a shell of relativistic particles at an altitude above the earths surface

5041760 – August 20, 1991 – Method and apparatus for generating and utilizing a compound plasma configuration

5041834 – August 20, 1991 – Artificial ionospheric mirror composed of a plasma layer which can be tilted

5056357 – October 15, 1991- Acoustic method for measuring properties of a mobile medium

5059909 – October 22, 1991 – Determination of particle size and electrical charge

5104069 – April 14, 1992 – Apparatus and method for ejecting matter from an aircraft

5110502 – May 5, 1992 – Method of suppressing formation of contrails and solution therefor

5156802 – October 20, 1992 – Inspection of fuel particles with acoustics

5174498 – December 29, 1992 – Cloud Seeding

5148173 – September 15, 1992 – Millimeter wave screening cloud and method

5242820 – September 7, 1993 – Army Mycoplasma Patent Patent

5245290 – September 14, 1993 – Device for determining the size and charge of colloidal particles by measuring electroacoustic effect

5286979 – February 15, 1994 – Process for absorbing ultraviolet radiation using dispersed melanin

5296910 – March 22, 1994 – Method and apparatus for particle analysis

5327222 – July 5, 1994 – Displacement information detecting apparatus

5357865 – October 25, 1994 – Method of cloud seeding

5360162 – November 1, 1994 – Method and composition for precipitation of atmospheric water

5383024 – January 17, 1995 – Optical wet steam monitor

5425413 – June 20, 1995 – Method to hinder the formation and to break-up overhead atmospheric inversions, enhance ground level air circulation and improve urban air quality

5434667 – July 18, 1995 – Characterization of particles by modulated dynamic light scattering

5436039 – July 25, 1995 – Artificial Snow in an Aggregate Form of Snow Granules

5441200 – August 15, 1995 – Tropical cyclone disruption

5492274 – February 20, 1996 – Method of and Means for Weather Modification

5546183 – August, 13, 1996 – LIDAR Droplet Size Monitor for In-Flight Measurement of Aircraft Engine Exhaust Contrails, Droplets and Aerosols

5556029 – September 17, 1996 – Method of hydrometeor dissipation (clouds)

5628455 – May 13, 1997 – Method and apparatus for modification of supercooled fog

5631414 – May 20, 1997 – Method and device for remote diagnostics of ocean-atmosphere system state

5639441 – June 17, 1997 – Methods for fine particle formation

5762298 – June 9, 1998 – Use of artificial satellites in earth orbits adaptively to modify the effect that solar radiation would otherwise have on earth’s weather

5800481 – September 1, 1998 – Thermal excitation of sensory resonances

5912396 – June 15, 1999 – System and method for remediation of selected atmospheric conditions

5922976 – July 13, 1999 – Method of measuring aerosol particles using automated mobility-classified aerosol detector

5949001 – September 7, 1999 – Method for aerodynamic particle size analysis

5984239 – November 16, 1999 – Weather modification by artificial satellites

6025402 – February 15, 2000 – Chemical composition for effectuating a reduction of visibility obscuration, and a detoxifixation of fumes and chemical fogs in spaces of fire origin

6030506 – February 29, 2000 – Preparation of independently generated highly reactive chemical species

6034073 – March 7, 2000 – Solvent detergent emulsions having antiviral activity

6045089 – April 4, 2000 – Solar-powered airplane

6056203 – May 2, 2000 – Method and apparatus for modifying supercooled clouds

6315213B1 – June 21, 2000 – Method of modifying weather

6110590 – August 29, 2000 – Synthetically spun silk nanofibers and a process for making the same

6263744 – July 24, 2001 – Automated mobility-classified-aerosol detector

6281972 – August 28, 2001 – Method and apparatus for measuring particle-size distribution

20030085296 – November 2, 2001 – Hurricane and tornado control device

6315213 – November 13, 2001 – Method of modifying weather

2002009338 – January 24, 2002 – Influencing Weather Patterns by way of Altering Surface or Subsurface Ocean Water Temperatures

20020008155 – January 24, 2002 – Method and System for Hurricane Control

6382526 – May 7, 2002 – Process and apparatus for the production of nanofibers

6408704 – June 25, 2002 – Aerodynamic particle size analysis method and apparatus

6412416 – July 2, 2002 – Propellant-based aerosol generation devices and method

6520425 – February 18, 2003 – Process and apparatus for the production of nanofibers

6539812 – April 1, 2003 – System for measuring the flow-rate of a gas by means of ultrasound

6553849 – April 29, 2003 – Electrodynamic particle size analyzer

6569393 – May 27, 2003 – Method And Device For Cleaning The Atmosphere

20040060994 – April 1, 2004 – Method for Influencing Atmospheric Formations

20040074980 – April 22, 2004 – Method and Device for Generating a Liquid Mist

0056705 A1 – March 17, 2005 – Weather Modification by Royal Rainmaking Technology

6890497 – May 10, 2005 – Method For Extracting And Sequestering Carbon Dioxide

2446250 – January 4, 2007 – A dust or particle-based solar shield to counteract global warming

20070056436 – March 15, 2007 – Challenger to Natural Twisters, Technology

2007033448 – March 29, 2007 – Production of Localized Artificial Rains in Polar Stratospheric Clouds, to Promote a Rain Wash in the CIO Gas, Reduce the Destruction of the Ozone Layer and a Replacement Process in situ of the Stratospheric Ozone

20070114298 – May 24, 2007 – Hurricane Abatement Method and System

20070158449 – July 12, 2007- Tropical Hurricane Control System

20070215946 – September 20, 2007 – Broadband Communications System via Reflection from Artificial Ionized Plasma Patterns in the Atmosphere

7965488 – November 9, 2007 – Methods Of Removing Aerosols From The Atmosphere

8048309 – August 28, 2008 – Seawater-Based Carbon Dioxide Disposal

20080203328 – August 28, 2008 – Outer Space Sun Screen for Reducing Global Warming

20100072297 – September 24, 2008 – Method for controlling hurricanes

7434524 – October 14, 2008 – Machine to Get Rid of Hurricanes

8012453 – October 27, 2008 – Carbon Sequestration And Production Of Hydrogen And Hydride

20090008468 – January 8, 2009 – How to Tame Hurricanes and Typhoons with Available Technology

7520237 – April 21, 2009 – Hurricane Prevention System and Method

20090255999 – October 15, 2009 – Production or Distribution of Radiative Forcing Elements

20090290761 – November 26, 2009 – Upper Troposphere and Lower Stratosphere Wind Direction, Speed, and Turbidity Monitoring using Digital Imaging and Motion Tracking

7645326 – January 12, 2010 – RFID environmental manipulation

7655193 – February 2, 2010 – Apparatus For Extracting And Sequestering Carbon Dioxide

20100074390 – March 25, 2010 – Method for Weather Modification and Vapor Generator for Weather Modification

20100127224 – May 27, 2010 – Atmospheric Injection of Reflective Aerosol for Mitigating Global Warming

7748662 – July 6, 2010 – Aerial Delivery System

20100170958 – July 8, 2010 – Hurricane Mitigation by Combined Seeding with Condensation and Freezing Nuclei

20100252648 – October 7, 2010 – Climate Processor

20100264230 – October 21, 2010 – Severe Storm / Hurricane Modification Method and Apparatus

20100282914 – November 11, 2010 – Enhanced Aerial Delivery System

20110005422 – January 13, 2011 – Method and Apparatus for Cooling a Planet

20110049257 – March 3, 2011 – Method and Apparatus for Local Modification of Atmosphere

20110101124 – May 5, 2011- Hurricane Abatement System and Method

2011073650 – June 23, 2011 – Atmospheric Delivery System

20110168797 – July 14, 2011 – Method of Weakening a Hurricane

20110174892 – July 21, 2011 – Apparatus and Related Methods for Weather Modification by Electrical Processes in the Atmosphere

20110198407 – August 18, 2011 – Method and Apparatus to Break Up or Annihilate Typhoons, Tornadoes, Cyclones or Hurricanes

20110204159 – August 25, 2011 – Weather Management Using Space-Based Power System

20110284649 – November 24, 2011 – Apparatus and Method for the Mitigation of Rotating Wind Storms

8079545 – December 20, 2011 – Ground based Manipulation and Control of Aerial Vehicle during nonflying operations

20120024971 – February 2, 2012 – Methods for Environmental Modification with Climate Control Materials and Coverings

8262314 – September 11, 2012 – Method for Decreasing the Intensity and Frequency of Tropical Storms or Hurricanes

0117003 – October 5, 2012 – Geoengineering Method Of Business Using Carbon Counterbalance Credits

20120267444 – October 25, 2012- Artificial Freezing Apparatus and Freezing Method Therefor

20120286096 – November 15, 2012 – Aerial Delivery Devices, Systems and Methods

20130008365 – January 10, 2013 – System and Method for Decreasing the Intensity and Frequency of Tropical Storms or Hurricanes

20130015260 – January 17, 2013 – Concept and Model for Utilizing High-Frequency or Radar or Microwave Producing or Emitting Devices to Produce, Effect, Create or Induce Lightning or Lightspeed or Visible to Naked Eye Electromagnetic Pulse or Pulses, Acoustic or Ultrasonic Shockwaves or Booms in the Air, Space, Enclosed, or Upon any Object or Mass, to be Used Solely or as Part of a System, Platform or Device Including Weaponry and Weather Modification

8373962 – February 12, 2013 – Charged seed cloud as a method for increasing particle collisions and for scavenging airborne biological agents and other contaminants

20130038063 – February 14, 2013 – Apparatus and Method for Inhibiting the Formation of Tropical Cyclones

201300043322 – February 21, 2013 – Processes and Apparatus for Reducing the Intensity of Tropical Cyclones

8402736 – March 26, 2013 – Method and Apparatus for Suppressing Aeroengine Contrails

8439278 – May 14, 2013 – Apparatus for Producing a Mass of Water Vapor, Apparatus for Producing, Moving, and Climbing a Mass of Water Vapor, and Method of Causing Artificial Stimulation of Rain

20130175352 – July 11, 2013 – Method to Influence the Direction of Travel of Hurricanes

20130186127 – July 25, 2013 – Ice Floater for Facilitating Ice-Freezing on Water Surface

20130206912 – August 15, 2013 – Moisture Dispersion

20140055876 – February 27, 2014 – Method for Controlling Land Surface Temperature using Stratospheric Airships and Reflector

20140131471 – May 15, 2014 – Apparatus to Channel Large Air Masses for Climate Modification

20140145002 – May 29, 2014 – System for Facilitating Cloud Formation and Cloud Precipitation

20140224894 – August 14, 2014 – Technique to Mitigate Storms using Arrays of Wind Turbines

8825241 – September 2, 2014 – Autonomous Wave-Powered substance Distribution Vessels for Fertilizing Plankton, Feeding Fish, and Sequestering Carbon from the Atmosphere

8944363 – February 3, 2015 – Production or Distribution of Radiative Forcing Agents

20150077737 – March 19 2015 – System and Methods for Monitoring an Environment

9002660 – April 7, 2015 – Device and Method for Determining and Indicating Climate-Relevant Effects of a Contrail Produced by an Airplane

20150230415 – August 20, 2015 – Methods for Decreasing Local Temperature using High Albedo Materials

20150337224 – November 26, 2015 – Microwave Acceleration of Carbon Gasification Reactions

9311539 – April 12, 2016 – Aircraft Contrail Detection

9429348 – August 30, 2016 – Method and Device for Producing Snow

9491911 – November 15, 2016 – Method for Modifying Environmental Conditions with Ring Comprised of Magnetic Material

9589473 – March 7, 2017 – Method and System for Automatically Displaying Flight Path, Seeding Path, and Weather Data

9715039 – July 25, 2017 – Apparatus and System for Smart Seeding within Cloud Formations

20170217587 – August 3, 2017 – Vehicles and Systems for Weather Modification

20170303479 – October 26, 2017 – Warm Cloud Catalyst, Preparation Method Therefor and Application Thereof

20180006422 – January 4, 2018 – Methods for Disrupting Hurricane Activity

20180006421 – January 4, 2018 – Methods for Disrupting Tornadic Activity

9924640 – March 27, 2018 – Modifying Sunlight Scatter in the Upper Atmosphere

20180217119 – August 2, 2018 – Process and Method for the Enhancement of Sequestering Atmospheric Carbon through Ocean Iron Fertilization, and Method for Calculating net Carbon Capture from said Process and Method

10189753 – January 29, 2019 – Fog-Generating Device Comprising a Reagent and Ignition Means

2019203461 – June 6, 2019 – Airships for Weather Manipulation

10314249 – June 11, 2019 – Systems and Methods of Inducing Rainfall

10375900 – August 13, 2019 – Rain Induced by Supercontinuum Laser Beams

10433408 – October 1, 2019 – Methods for Affecting Spinning Atmospheric Phenomena

10435165 – October 8, 2019 – Aircraft Electrically-Assisted Propulsion Control System

20190364748 – December 5, 2019 – Method and System for Expressing Airborne Cloud Seeding Line Considering Cloud Water

20200187430 – June 18, 2020 – Helical Artificial Generator of Tornado, Hurricane, Yellow Dust, and Typhoon

20200196539 – June 25, 2020 – Device for Seeding a Cloud Cell

10701871 – July 7, 2020 – Systems for Maintaining and/or Decreasing Water Temperature using High Albedo Materials

20200233115 – July 23, 2020 – Method and System for Determining Cloud Seeding Potential

WO2020148644A1 – July 23, 2020 – 3d Reduced Graphene Oxide/Sio 2 Composite for Ice Nucleation

20200261939 – August 20, 2020 – Apparatus for Generating and Optically Characterizing an Aerosol

2020101897 – September 9, 2020 – Artificial Rainmaking by High Power Laser Initiation Endothermic Reactions through Drone Aircraft Remote Control System

20200288650 – September 17, 2020 – Technology and Technique to Prevent, Diminish or Interfere with the Formation of Hurricanes on Earth from one or more Platforms in Space

20200288651 – September 17, 2020 – Methods for Cooling Water Temperature using High Albedo Materials

20200315104 – October 8, 2020 – Propagating Sound Through Bodies of Water, to Generate and Direct Wind, for the Purpose of Moderating and Affecting Weather Patterns

20200386970 – December 10, 2020 – Aerostatically Stabilized Atmospheric Reflector to Reduce Solar Irradiance

10888051 – January 12, 2021 – Intelligent Systems for Weather Modification Programs

20210037719 – February 11, 2021 – Planetary Weather Modification System

10941705 – March 9, 2021 – Hanson-Haber Aircraft Engine for the Production of Stratospheric Compounds and for the Creation of Atmospheric Reflectivity of Solar Radiation in the 555nm Range and to Increase Jet Engine Thrust and Fuel Economy through the Combustion of Ammonia and Ammonia By-Products

2021063943 – April 8, 2021 – Bacterial Preparations for Ice Nucleation

20210153442 – May 27, 2021 – Systems and Methods for Rain Cloud Initiation

20210163157 – June 3, 2021 – Artificial Ring, Solenoid System to Terraform

20210235638 – August 5, 2021 – Weather Management of Cyclonic Events

2021152336 – August 8, 2021 – Method of Cloud Seeding using Natural Ice Nucleating Agents

20210285851 – September 16, 2021- System for Sampling and Analyzing Contrails Generated by an Aircraft

20210289720 – September 23, 2021 – Systems and Methods for Producing Rain Clouds

2021105881 – October 21, 2021 – Process for Generating Marine Clouds and Ocean Microbubbles

20210329922 – October 28, 2021 – Compositions and Methods for Enhanced CO2 Capture and Storage

20210329852 – October 28, 2021 – Method for Preventing a Formation of, and/or for Dispersing, a Tropical Cyclone, and Arrangement Therefor

20210352856 – November 18, 2021 – Aerial Electrostatic System for Weather Modification

2021107294 – December 9, 2021 – Wind Turbines for Marine Cloud Brightening Dispersion

2022003028 – January 6, 2022 – Apparatus for Precipitation of Atmospheric Water

23220065599 – March 3, 2022 – Rocket for Artificial Rainfall using Ejection Hygroscopic Flare

11274534 – March 15, 2022 – Artificial rain to support water flooding in remote oil fields

20220113450 – April 14, 2022 – Calculation Method of Total Artificial Precipitation in Seeding Area Compared to Non-Seeding Area

2022094269 – May 5, 2022 – Reflective Hollow SRM Material and Methods

3994976 – May 11, 2022 – Apparatus for Electro-Spray Cloud Seeding

11330768 – May 17, 2022 – Systems and Methods for Producing Rain Clouds

20220268505 – August 25, 2022 – Method and Apparatus for Making Falling Snow

2022186970 – September 9, 2022 – Method of Geoengineering to Reduce Solar Radiation

20220355925 – November 10, 2022 – Aeronautical Car and Associated Features

20220357482 – November 10, 2022 – Method and System of Analyzing Ingredients of Artificial Rainfall for Verification of Cloud Seeding Effect

20230050373 – February 16, 2023 – Electromagnetic System to Modify Weather

20230075132 – March 9, 2023 – System for Moderating Energy Absorption at the Earth’s Surface with a Programmable Forcing Network of Climate Control Panels

20230117390 – April 20, 2023 – System and Method for Proactive and Reversible Mitigation of Storm/Hurricane/Typhoon/Cyclone

20230126982 – April 27, 2023 – Method for Analyzing Effect of Hygroscopic Seeding Material Sprayed on Ground Aerosol Concentration Through Airborne Cloud Seeding Experiment

20230141493 – May 11, 2023 – Device for Unmanned Aerial Vehicle to Deploy a Rainfall Catalytic Bomb

20230149876 – May 18, 2023 – Coated Chloride Salt Particles and Methods of Making and Using the Same.

[quiltofstars]

De Mairan's Nebula, M43 // Seokhee Kim

No, this is not necessarily a repeat! Instead of on the beautiful Orion Nebula, focus your attention at the small star-forming region in the top left of the image. That is De Mairan's Nebula, separated from the larger Orion Nebula by just a dark dust lane.

Discovered by Jean-Jacques d'Ortous de Mairan (1678-1771) some time before 1731, this star-forming region is ionized by a single star system, which you can see in the image! The main star is about 1,300 light years away, and is radiating over 26,000 times the Sun's luminosity. It's unknown why Messier considered this star-forming region to be separate from Orion, but the earlier discovery which Messier knew about likely helped.

[santoschristos]

In the Heart of the Heart Nebula

“You’ll be given love. You’ll be taken care of. You have to trust it. Maybe not from the sources you have poured yours. Maybe not from the directions you are staring at. Twist your head around. It’s all around you. All is full of love.”

The Heart Nebula, or IC 1805, is a beautiful emission nebula located 7,500 light-years away in the constellation Cassiopeia. Discovered by William Herschel in 1787, it's characterized by glowing ionized hydrogen and dark molecular dust. The nebula's distinctive red color and dramatic shape are due to radiation from the nearby star cluster Melotte 15, which contains stars about 50 times brighter than our sun. A

Heart for Valentina --Mahaboka