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#Thermographic inspection Ottawa#ThermoElite#Infrared imaging services#Ottawa property inspection#Energy efficiency assessment
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delivery app made me drive to spencer again
#i used rni's aerochrome filter for this#as much as it sounds like a thing i might do i do not take my infrared camera with me everywhere#i took these one handed with my phone without looking#anyway#livali's delivery service#my photography#me posts#the signs may be hard to read so i have transcribed them in the image descriptions
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Calling Long-Distance: 10 Stellar Moments in 2022 for Space Communications and Navigation
Just like your phone needs Wi-Fi or data services to text or call â NASA spacecraft need communication services.
Giant antennas on Earth and a fleet of satellites in space enable missions to send data and images back to our home planet and keep us in touch with our astronauts in space. Using this data, scientists and engineers can make discoveries about Earth, the solar system, and beyond. The antennas and satellites make up our space communications networks: the Near Space Network and Deep Space Network.
Check out the top ten moments from our space comm community:Â
1. Space communication networks helped the Artemis I mission on its historic journey to the Moon. From the launch pad to the Moon and back, the Near Space Network and Deep Space Network worked hand-in-hand to seamlessly support Artemis I. These networks let mission controllers send commands up to the spacecraft and receive important spacecraft health data, as well as incredible images of the Moon and Earth.
The Pathfinder Technology Demonstration 3 spacecraft with hosted TeraByte InfraRed Delivery (TBIRD) payload communicating with laser links down to Earth. Credit: NASA/Ames Research Center
2. Spacecraft can range in size â from the size of a bus to the size of a cereal box. In May 2022, we launched a record-breaking communication system the size of a tissue box. TBIRD showcases the benefits of a laser communications system, which uses infrared light waves rather than radio waves to communicate more data at once. Just like we have upgraded from 3G to 4G to 5G on our phones, we are upgrading its space communications capabilities by implementing laser comms!
3. The Deep Space Network added a new 34-meter (111-foot) antenna to continue supporting science and exploration missions investigating our solar system and beyond. Deep Space Station 53 went online in February 2022 at our Madrid Deep Space Communications Complex. It is the fourth of six antennas being added to expand the networkâs capacity.
4. Youâve probably seen in the news that there are a lot of companies working on space capabilities. The Near Space Network is embracing the aerospace communityâs innovative work and seeking out multiple partnerships. In 2022, we met with over 300 companies in hopes of beginning new collaborative efforts and increasing savings.
5. Similar to TBIRD, we're developing laser comms for the International Space Station. The terminal will show the benefits of laser comms while using a new networking technique called High Delay/Disruption Tolerant Networking that routes data four times faster than current systems. This year, engineers tested and proved the capability in a lab.
6. In 2021, we launched the James Webb Space Telescope, a state-of-the-art observatory to take pictures of our universe. This year, the Deep Space Network received the revolutionary first images of our solar system from Webb. The telescope communicates with the networkâs massive antennas at three global complexes in Canberra, Australia; Madrid, Spain; and Goldstone, California.
7. Just like we use data services on our phone to communicate, we'll do the same with future rovers and astronauts exploring the Moon. In 2022, the Lunar LTE Studies project, or LunarLiTES, team conducted two weeks of testing in the harsh depths of the Arizona desert, where groundbreaking 4G LTE communications data was captured in an environment similar to the lunar South Pole. We're using this information to determine the best way to use 4G and 5G networking on the Moon.
8. A new Near Space Network antenna site was unveiled in Matjiesfontein, South Africa. NASA and the South African Space Agency celebrated a ground-breaking at the site of a new comms antenna that will support future Artemis Moon missions. Three ground stations located strategically across the globe will provide direct-to-Earth communication and navigation capabilities for lunar missions.
9. Quantum science aims to better understand the world around us through the study of extremely small particles. April 14, 2022, marked the first official World Quantum Day celebration, and we participated alongside other federal agencies and the National Quantum Coordination Office. From atomic clocks to optimizing laser communications, quantum science promises to greatly improve our advances in science, exploration, and technology.
10. We intentionally crashed a spacecraft into an asteroid to test technology that could one day be used to defend Earth from asteroids. The Double Asteroid Redirection Test, or DART, mission successfully collided with the asteroid Dimorphos at a rate of 4 miles per second (6.1 kilometers per second), with real-time video enabled by the Deep Space Network. Alongside communications and navigation support, the global network also supports planetary defense by tracking near-Earth objects.
We look forward to many more special moments connecting Earth to space in the coming year.
Make sure to follow us on Tumblr for your regular dose of space!
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At long last, I can post the finished art! I had been sitting on it for some weeks, waiting for the inspiration to hit to write a short piece to accompany it. Definitely recommend full viewing.
oOo ----------------------------------------------------- oOo
Glittering motes of dust hung suspended in waning late afternoon light shining through the skylights. The upper levels of the City-Beneath-The-Cube were lighter and airier than outsiders realized, but the walls, planters and walkways of planed and etched stone that went down many stories made the whole of the place feel like some kind of precision-wrought canyon dotted with workshops, passages and arcades where the locals and laborers bustled.
(continued under the cut)
Lorr still knew this place well, despite the many years separating his former life and younger self from his current one. It hadnât changed much, the smells and the noise were the same but he noted that there were new, more effective safety railings in the Public Commons and that the local favorite dive, Piâs had updated their signage (finally).
The bounty hunter rubbed a hand across his face, closing his eyes momentarily as he let his ears take over, picking up all the sounds surrounding him. He would need to move further away from the Commons to better filter the urban background static. Lorr had just sent out his hawk Deputy to scope out the area in case they got lucky and found their mark momentarily out in the open. Both he and Deputy were already familiar with her, so that wouldnât be difficult. Problem was, it also meant sheâd immediately recognize the hawk for who he was and what it meant as well. A part of Lorr secretly hoped sheâd get tipped off early.
Why did I agree to this? It wasnât the money, not this time. Am I trying to make a point? She nearly got us killed and then ran for it. But I know her. Knew her. I canât just erase all this history just because of one incident, one indiscretion can I? Maybe this is how I have to get through to her.
He sighed inwardly and braced against his spear as he rose from a crouch, the movement preternaturally smooth and deliberate, like a predatory animal. He looked down from his high vantage as he faced the section of the Undercube that was known to the denizens as the Plexus. It was a network of tunnels, access âports, antechambers, quarries and dwellings that confounded natural senses of direction. Less public-facing, much more closed in and easier to hide. Or lose a pursuer.
The slim asura made his way down the ledge he was using to survey, walking along a catwalk only just wide enough to admit a mid-sized labor golem at most. His ears twitched and he sniffed, feeling the minute air currents of a service tunnel cleverly tucked behind a cleft in the worked stone. Still not certain this was were his mark had proceeded but knowing it would get him into the center of the Plexus quicker, he decided to go for it anyway. Forced to stow his spear in such close quarters, he kept a hand on his dagger as he stalked forward into the passage, the inside only dimly lit by a track of dim yellow quartz-lights along the floor.
Infrared imaging on his monocle made it easy for him to get an idea of the topography of the inner workings of the maze of service tunnels he found himself in, but he was careful to not rely on it solely. He stopped every so often, using his eyes and ears but also a generous amount of intuition to pick the correct course. Chambers became somewhat larger and more spacious as he passed golem foundries, making his way steadily downward. He was becoming more aware that he knew where he was going, it was like retracing steps from his childhood back to the colorful yet rundown living warrens and slums that he grew up in.
She wouldnât go all the way back there, would she? Lorr was starting to think it wasnât just him that was trying to make some kind of point.
The smells and noise were subtly changing and it wasnât long before he found himself in the center of the Plexus. Part bazaar, part manufactory, it acted as the working class nerve center and was a riot of activity, industrial clamor and smells.
He was certain of where he was going now. He didnât know why exactly she came all the way down here where they had all met in the early days before the nonsense with the Whispers and fighting dragons happened, but he was determined to find where this chase ended. Heâd get answers, and if it meant having to fail his mission and come back to his current boss empty handed, then so be it.
#GW2#Guild Wars 2#Asura#guildwars2 fanart#traditional art#my art#my writing#my characters#Lorr the Hawk#May or may not continue this story thread#depending if I get ideas for it and if people would actually be inclined to read it#but for now enjoy the art a little bit of fun if mysterious insight into Lorr
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U.S. Air Force Awards RTX $1 Billion Contract to Upgrade F-22 Sensors
The contract follows the recent news about the tests of new advanced sensors on the F-22 Raptor, which the U.S. Air Force is planning to field quickly as part of the ongoing upgrade program.
Parth Satam
F-22 new sensors contract
An F-22 Raptor takes off from Nellis Air Force Base, Nevada, June 30, 2022. (U.S. Air Force photo by Senior Airman Zachary Rufus)
Amid the acute need for 5th generation fighters in modern combat scenarios against peer adversaries, the U.S. Air Force is looking to upgrade its F-22 Raptor with a series of sensors to make it more survivable and relevant. The service announced on Aug. 29, 2024, the award of a $1 billion contract to RTXâs Raytheon for new sensors that are categorized as âGroup B hardwareâ, together with spares and support equipment.
âWork will be performed in McKinney, Texas, and is expected to be completed by May 8, 2029,â said the DoD contracts statement. The Aviationist had recently reported that the Air Force was testing new sensors on the F-22 to extend its service life, which would also be applied to the NGAD (Next Generation Air Dominance) family of systems.
That report also quoted Brig. Gen. Jason D. Voorheis, the Program Executive Officer for Fighter and Advanced Aircraft, who said they were hoping to field these sensors faster. The Raptor team had conducted six flight tests to demonstrate the advanced sensors.
âThe F-22 team is working really hard on executing a modernization roadmap to field advanced sensors, connectivity, weapons, and other capabilities. Weâre executing that successfully, and that will lead to [âŚ] a rapid fielding in the near future.â This would be done through a Middle Tier Acquisition (MTA) program.
Some of the sensors included in the contract could be the stealthy pods seen on the F-22. Air and Space Forces earlier quoted officials who confirmed that the pods host IRST (Infrared Search and Track) sensors. The development of a new IRST sensor for the Raptor was also confirmed by the serviceâs 2025 budget request, which however did not mention the sensor being podded.
This work is part of an F-22 improvement campaign that calls for $7.8 billion in investments before 2030, which includes $3.1 billion for research and development and $4.7 billion in procurement.
An F-22 Raptor with the Air Combat Command F-22 Raptor Demonstration Team performs a flyover and air demonstration at the U.S. Air Force Academy in Colorado Springs, Colo., Aug 13, 2024. (U.S Air Force Photo by Trevor Cokley)
F-22âs future in the U.S. Air Force
The development is also in contrast with previously reported USAF plans to retire the older F-22 airframes, for which it had sought approval from the Congress. These F-22s are 32 Block 20 units from a total fleet of 186. At the same time, the service aims to upgrade the remaining 154 with new cryptography, an expanded open architecture, new weapons and an advanced threat warning receiver, beside the IRST.
However, the service now appears to be reconsidering that plan, after Voorheis was quoted in the ASF report: âFrom an F-22 sunsetting perspective, I donât have a date for you.â âWhat I can tell you is that we are hyper-focused on modernization to sustain that air superiority combat capability for a highly contested environment for as long as necessary,â he added.
IMAGE 3: A U.S. Air Force F-22 Raptor assigned to the 3rd Wing takes off above Joint Base Elmendorf-Richardson, Alaska, Jun. 17, 2024. (Image credit: USAF/Senior Airman Julia Lebens)
The U.S. Air Force describes the Raptor as a combination of stealth, supercruise, maneuverability, and integrated avionics, designed to project air dominance, rapidly and at great distance. Initially introduced as an air-superiority-only asset, the F-22 later started performing both air-to-air and air-to-ground missions.
The F-35 is largely a strike fighter and an airborne sensor-fusion and data-processing capable command post in its tactical orientation. But the Raptor is a pure air dominance interceptor. Although costly to upgrade and maintain, it nevertheless can play an important role in degrading adversary air power through either long-range BVR (Beyond Visual Range) and dogfights.
Moreover, having F-22s also increases the number of LO (Low Observable) aircraft in the inventory, at least until more F-35s are available, especially the TR-3 (Technology Refresh-3) Block 4 upgraded variants.
In 2021 too, then Air Force chief General Charles Q. Brown Jr. revealed his â4+1â fighter plan, suggesting the F-22 to be replaced by the NGAD while retaining the F-35, F-15E and EX, and the F-16. The âplus 1â was the A-10, but in March 2023, Brown said the A-10s were being retired faster than expected and the entire fleet would possibly be divested by 2030.
Meanwhile the NGADâs future itself is uncertain after U.S.A.F have noted its technical complexity and financial implications. The F-22 thus seems to be back in the running.
On Jul. 10, 2024, Air Combat Command chief Gen. Kenneth Wilsbach said during a Mitchell Institute event that the service has no official plan to retire its F-22 Raptors. âRight now, thereâsâŚfrankly isnât an F-22 replacement and the F-22 is a fantastic aircraft,â said Wilsbach. âIâm in favor of keeping the Block 20s. They give us a lot of training value, and even if we had to in an emergency use the Block 20s in a combat situation, theyâre very capable.â
F-22 Indonesia
U.S. Air Force F-22 Raptors assigned to the 27th Expeditionary Fighter Squadron, conduct Dynamic Force Employment operations at I Gusti Ngurah Rai Air Force Base, Indonesia, on Aug. 6, 2024. (U.S. Air Force photo by Senior Airman Mitchell Corley)
Other known F-22 upgrades
Other upgrades mentioned in the 2025 budget request are a Mode 5 Identification Friend or Foe (IFF), Link 16, a Multifunction Information Distribution System Joint Tactical Radio System (MIDS JTRS), a new Operational Fight Program, advanced radar Electronic Protection and an Embedded GPS/Inertial Navigation System (INS) Modernization (EGI-M).
Voorheis also mentioned the GRACE (Government Reference Architecture Compute Environment) software that would allow ânon-traditional F-22 softwareâ to be installed on the aircraft and provide âadditional processing and pilot interfaces.â
A new helmet is also being tested, as part of the Next Generation Fixed Wing Helmet program to replace the current 40-year-old HGU-55P headgear. The new helmet would also allow the introduction of helmet-mounted devices which provide essential flight and weapon aiming information through line of sight imagery, easing the workload of the pilots.
About Parth Satam
Parth Satam's career spans a decade and a half between two dailies and two defense publications. He believes war, as a human activity, has causes and results that go far beyond which missile and jet flies the fastest. He therefore loves analyzing military affairs at their intersection with foreign policy, economics, technology, society and history. The body of his work spans the entire breadth from defense aerospace, tactics, military doctrine and theory, personnel issues, West Asian, Eurasian affairs, the energy sector and Space.
@Theaviationist.com
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A Colorful Aurora Paints the Night Sky
As we move into the peak of solar cycle 25, activity on the Sun has been ratcheting up. One sign of that appeared in Earthâs atmosphere in the form of an impressive display of the aurora borealis, or northern lights, which was visible to observers on the ground beyond the Arctic Circle and deep into the midlatitudes in October 2024.
Millions of skywatchers were treated to the green, pink, and red lights of the aurora overnight on October 10-11. At 1:55 a.m. Eastern Time (05:55 Universal Time) on October 11, the VIIRS (Visible Infrared Imaging Radiometer Suite) on the NOAA-20 satellite acquired this image of the aurora. The VIIRS day-night band detects nighttime light in a range of wavelengths from green to near-infrared and uses filtering techniques to observe signals such as city lights, reflected moonlight, and auroras.
In this view, the northern lights appear as ribbons of white crossing parts of Minnesota, Wisconsin, and Michigan in the U.S., and several provinces in Canada. But auroras are dynamic, and different coverage and patterns of light would have been visible at other times of the night. While these satellite data are shown in grayscale, viewers on the ground saw colors from green (the most common) to purple to red. Atmospheric compounds found at different altitudes influence an auroraâs color.
An astronaut on the International Space Station captured the photograph below of green hues of the aurora dancing across the planetâs surface, with a layer of deep red light above.
The light show was the visible manifestation of a severe geomagnetic stormâa disturbance of the upper atmosphere caused by the interaction of pressure waves and electromagnetic energy from the Sun interacting with Earthâs magnetic field, or magnetosphere.
In this case, the storm was caused by energized material emitted from the Sun, also known as a coronal mass ejection, that occurred in tandem with an intense solar flare on October 8, 2024. Whereas solar flares reach the planet in a matter of minutes and interfere with radio communications, coronal mass ejections may take several days to travel to Earth.
Coronal mass ejections contain large amounts of plasma from the Sunâs corona and carry with them an embedded magnetic field. Interactions between these expulsions from the Sun and the upper atmosphere of Earth produce the colorful auroral displays. According to NOAAâs Space Weather Prediction Center, the storm ranked 4 out of 5 in severity.
The aurora was visible from many areas worldwide, including latitudes where sightings of auroras are uncommon. Auroras occur high in the atmosphere, so observers on the ground can potentially witness them from far awayâwell beyond the areas covered by the band of light in the satellite image at the top of this page. Photographs of the aurora were shared from Nevada, North Carolina, Arizona, and Texas. The National Weather Service in Lubbock, Texas, shared photos of the aurora in shades of pink and green.
NASA Earth Observatory image by Michala Garrison, using VIIRS day-night band data from NASA EOSDIS LANCE, GIBS/Worldview, and the Joint Polar Satellite System (JPSS). Story by Emily Cassidy.
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One wouldnât have to spend much time going through my work to figure out that I really like this old Aermotor windmill that is still very much in service, pumping water from the ground for cattle. It sits on a ranch near the northern end of Lassen County California in plain sight just off US-395. I have photographed it several times at different times of the day and year. On this particular spring drive it was nearly mid-day, not normally optimal for visible light photography. I pulled over to shoot it with my infrared gear which is typically better suited to shooting in bright sun. I captured a nice âfalse colorâ image, accomplishing the mission. But as I stood there looking at the wonderful clouds and wildflowers I figured I better grab my visible light gear too. The clouds softened what would otherwise been very harsh light and added some wonderful interest to the sky while still allowing some nice warm spring light on the flowering field. In my Etsy Shop: https://buff.ly/3SdHshe Prints and merch on demand: https://buff.ly/3vrfBkt
#original photographers#photographers on tumblr#northern california#original photographic works#original photography on tumblr#lassen county#rural america#windmill#aermotor#ranching
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Today in space, it's the Hubble Telescope's 34th birthday!
34 years ago today, on April 24th, 1990, the Hubble Space Telescope launched into low earth orbit within the payload bay of the Space Shuttle Discovery.
Though not the first space telescope, the Hubble was and still remains one of the most powerful. Its placement in low earth orbit allows the telescope to see and photograph distant stars, galaxies, and other space objects without the pesky atmosphere getting in the way.
When initially launched, the Hubble had a problem. Its mirror was flawed. It had been made according to incorrect specifications. This caused significant issues in imaging and photography, and NASA had to work quickly to determine a fix so that the telescope would not be abandoned. The versatility of the Space Shuttle to work in space allowed NASA astronauts to provide repairs to the Hubble, and in 1993 aboard the Space Shuttle Endeavour, astronauts serviced the telescope and replaced lenses in order to resolve the issue.
Since then, the Hubble has provided groundbreaking imagery of space, expanding our knowledge of the universe considerably. Without the impediment of the atmosphere, the Hubble is able to take clear photography of distant stars and galaxies... as well as places a little closer to home.
The last mission servicing the Hubble was STS-125 in 2009, when astronauts on the Space Shuttle Atlantis replaced and repaired instruments which allowed the Hubble's views to extend even further. The instrumentation installed also allowed the Hubble to view light beyond the visible spectrum, including near-infrared and ultraviolet.
Though no further servicing missions are planned, the Hubble is expected to remain in use until at least the late 2020's. Pictures from Hubble are what many of us think about when we think about space. It has long been our floating companion, sharing views of the universe around us we could never have even imagined while on earth. Happy birthday, Hubble!
All pictures sourced from NASA. For more information on the Hubble and more images taken by the telescope, click here.
#the whiscash administration#nasa#space program#hubble telescope#hubble space telescope#space shuttle
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Fresh Flows Across Iceland
"Lava poured from a volcanic fissure near the town of GrindavĂk, Iceland, in spring 2024. The eruption, which began on March 16 and remained active over two weeks later, was the largest in a string of four volcanic events on the Reykjanes peninsula starting in December 2023.Â
The OLI (Operational Land Imager) on Landsat 8 captured this image of the ongoing eruption on March 30, 2024. The natural color scene is overlaid with an infrared signal to help distinguish the lavaâs heat signature. The active part of the fissure and the origin of a volcanic plume are apparent. While the eruption was still active at this time, additional satellite and ground observations indicated it was likely waning.Â
The eruption began at 8:23 p.m. local time on March 16, the Icelandic Met Office (IMO) reported. A fissure nearly 3 kilometers (2 miles) long quickly opened in a similar location to the February 2024 eruption. Hundreds of people at the Blue Lagoon, as well as a small number in GrindavĂk, were evacuated within about 30 minutes of the eruption starting.Â
In the days that followed, lava flowed toward infrastructure such as water pipes and roads, the town of GrindavĂk, and the ocean. Human-constructed barriers of earth and rock diverted lava away from town, although a flow extended across one road. Officials were initially concerned that lava would reach the coast and cool rapidly upon contacting water. This could have posed additional hazards such as the production of hydrogen chloride gas, but the flow stopped short.
This Landsat image comparison shows the recent changes on the Reykjanes peninsula. In September 2023 (left), the area was quiet volcanically. By February 10, 2024 (center), three separate fissure eruptions had occurred. The footprint of new basaltic rock grew in March 2024 (right) as new lava spanned nearly 6 square kilometers (2.3 square miles), according to the IMO.Â
Like the eruptions that preceded it, the spring 2024 event was effusive, not explosive. Effusive eruptions tend to emit minimal ash, and their plumes typically contain water vapor, sulfur dioxide, carbon dioxide, and small amounts of other volcanic gases.Â
This eruption did not disrupt air travel, but sulfur dioxide (SO2) emissions were hazardous locally at times. Workers evacuated the power plant north of GrindavĂk on March 18 due to gas pollution, the Icelandic National Broadcasting Service reported. The SO2 emissions from this eruption were forecast to drift across the United Kingdom and northern Europe, according to models based on satellite observations, but at an altitude too high to affect surface air quality.Â
Unlike the other recent eruptions in this region, the springtime event stretched out over weeks rather than a couple of days. The reason for the relatively prolonged eruption may be that magma now has an easier path to the surface, experts suggested in news reports. Others think that magma is no longer accumulating in the shallow magma chamber beneath the area and that this eruption could be the last in the longer cycle.Â
NASA Earth Observatory images by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Story by Lindsey Doermann."
And to think we were there in September about the time the first photo was made! The main road connecting Grindavik to the remainder of Iceland has been cut in two places. According to their website, the popular tourist attraction Blue Lagoon is closed due to "unfavourable air quality" but is scheduled to reopen tomorrow 11 April.
Wish I could hop on a plane to see this in person, but other obligations preclude such a trip anytime soon.
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NGC 1999
ESA/Hubble & NASA, ESO, K. Noll
THE Cosmic Keyhole, or by the government name of NGC 1999, is a reflection nebula in the Orion constellation. Located near the Orion Nebula, in a region of the Milky Way where stars are actively being formed, NGC 1999 is ~1350ly from Earth and is the composition of young starâs (V380 Orionis) formation discards.
UNLIKE emission nebulae, which alone emit light due to radiation ionization involving starsâ ultraviolet rays and nebulaâs hydrogen atoms, NGC 1999 canât shine unless a fixed light source illuminates the nebula due to its reflective type. The Cosmic Keyhole, however, is brightened by V380 Orionis (the light diffracting in the image above), a T Tauri star that sits covered by the smog of its birth.
REGARDING the âkeyhole,â astronomers initially thought the hole was a Bok globule, a dense molecular cloud of gas and cosmic dust that absorbs light. In 2009, further observations were conducted using the Herschel Space Observatory (an infrared telescope that can penetrate dense material such as in this case), with supporting analyses from the Atacama Pathfinder Experiment, Nicholas U. Mayall Telescope, and the Magellan telescopes, debunking the Bok globule beliefâinstead concluding that NGC 1999âs mark isnât anything but empty space. To this day, itâs still unknown why NGC 1999 has its iconic hole, but experts speculate that its creation is from local, new starsâ jets of gas puncturing the nebulaâs foggy wall.
THE nebula was first discovered in the late 18th century by astronomer siblings Sir William and Caroline Herschel. It was later listed as object 1999 in the New General Catalogueâhence its formal name. In 1999, shortly after Servicing Mission 3A, the WFPC2 observations captured the image above.
CAPTION SOURCES
Main article w/ picture: "Hubble Peers at Mysterious Cosmic âKeyholeâ" (NASA).
ADS
| "Hier ist wahrhaftig ein Loch im Himmel. The NGC 1999 dark globule is not a globule"
A&A
| "Herschel: the first science highlights"
CfA
| "Bok Globules"
ESA/Hubble
| "Cosmic Keyhole"
NASA
| "The Reflection Nebula in Orion"
| "NGC 1999"
| "Hubble's Nebulae"
| "Hubble Images Bok Globules"
(Caption written by @kaitropoli (me) using information from the sources above. Astronomy--knowledge of the universe, its population, fundamentals, and how everything is *known* to operate--is expanding every day with new things being discovered; the information listed could expire, so note that what I've gathered spans from 1990-2010 (with particular articles from the 2020s affirming up-to-date information with unchanged data).)
#NASA#ESAHubble#hubble#ESA#astronomy#space#nebula#nebulae#telescope#cosmic#cosmickeyhole#ngc1999#1999#science#stars#reflectionnebula#herschel#newgeneralcatalogue#milkyway#history
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Fog Down in the Valley
"The Willamette Valley in Oregon is rich with farms and orchards, home to 70 percent of the stateâs population, and dotted with more than 500 wineries. But all of that can disappear under a blanket of white when the valley fills in with fog, as it has several times in recent weeks.
Fog is common in the region in the autumn and winter, as moist Pacific air moves inland, cools, and sinks into the vast valley between the Cascade Mountains and the Oregon Coast Range. As that air gives up its heat to the upper atmosphere, the layer near the surface becomes saturated and essentially forms clouds at ground level.
Such fog has been locked in the Willamette Valley for several long stretches in January and February 2022 due to temperature inversions, where warm air high in the atmosphere moved in over the cooler, denser air in the lowlands. Normally, temperatures are warmer at the land surface, cooling higher up in the sky. This allows for most of the rising air and pollutants to continue to disperse out into the atmosphere. But an inversion acts like an atmospheric âlid��� that can trap moisture and air pollution in a valley for days.
On February 10, 2022, the Operational Land Imager-2 (OLI-2) on Landsat 9 acquired these natural- and false-color views of thick fog in the Willamette Valley. The false-color image was composed from shortwave infrared, near-infrared, and red light (OLI-2 bands 6-5-4). Scientists turn to these wavelengths to distinguish clouds (white and pink) from snow and ice (cyan).
Oregon has already seen at least three extended periods of valley fog in 2022, as observed by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASAâs Terra satellite from February 8-12, January 22-29, and January 14-17.
Fog is essentially a low-lying cloud composed of tiny water droplets suspended in the air. As nights lengthen with the season, the atmosphere has more time to cool down and approach the dew pointâthe temperature at which the air becomes saturated and water vapor condenses into fog. Since cold, moist air is denser than warm air, it sinks and drains into valleys, meaning fog develops there first. Many valleys like the Willamette also have rivers and streams that amplify the fog with a ready supply of moisture.
Fog can pose serious risks for drivers. Fog-related traffic accidents typically cause more deaths in the United States each year than other high-profile weather events like heat waves, tornadoes, and floods, according to data from the National Weather Service and the Federal Highway Administration. The foggiest parts of the United States, including Oregon, see dense fog at least 40 days per year.
NASA Earth Observatory images by Joshua Stevens, using Landsat data from the U.S. Geological Survey. Story by Michael Carlowicz and Adam Voiland.
View this area in EO Explorer
Oregonâs Willamette Valley had endured several long stretches of thick fog in January and February 2022 due to temperature inversions."
Source: NASA Earth Observatory
Remembering long drives to California in the distant past, Oregon was about 400 km of potential fog. This photo published last year brought back memories.
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Discover unparalleled precision in Infrared thermographic inspections with ThermoElite, your trusted partner in Montreal. Our cutting-edge technology and skilled technicians ensure a thorough analysis of your systems, identifying potential issues before they escalate. Elevate your safety standards and operational efficiency with ThermoElite's reliable thermographic inspection services!
#Thermographic Inspection Montreal#ThermoElite#Infrared Imaging Services#Montreal Building Inspections#Thermal Analysis Experts
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Youtube comment from the image in the first post copy and pasted:
Great video clip. I had a job once at the US Steel Pipe Works, Geneva Plant, Utah where I took "slag temperatures" before they sprayed "devils liquor" sump water on it to cool it down. I wore wooden shoe "clogs" to protect my shoes from melting (the same kind coke oven operators wear when servicing the ovens). 24 hours after a "thimble car" dump of red-hot slag was made, I went out and traversed the dump-site, measuring congealed slag surface temperatures, sometimes up to and often exceeding 600 degrees F. I wore thick canvas over-clothes, but anywhere my body came into pointed contact with the canvas (elbows and knees) I would get "burned" because of the heat transferred from the canvas material through my regular clothes. The heat at breathing height was about 200 degrees F. I wore a face shield (clear) to protect my face from the heat and had to wear a scarf over my nose to prevent breathing in super-heated air. As it was, I still singed the hairs inside my nose if I inhaled a little too quickly.
Imagine walking around inside a pizza oven, that is what it felt like. It dried me out, like desiccating me from the inside out breathing in all that super hot and very dry air.
Watching the thimble cars dump slag at night was one of the most incredible visual experiences I have ever had. The second after they tip a thimble, when the splash of red hot slag boiling down the slope glows intensely red, there follows milliseconds later, a "blast" of intense infrared radiation, that hits you in the face like a gust of hot wind.
The sea-gulls around dusk, would often ride the intense thermals created by the super-heated air, drawing cooler air up from below the slag pits, combining with the hot air whoosh it would go, rushing up the precipitous cliffs, man-made mini-mountains of slag, there they would fly along the thermals updraft about 100 feet up and nearly parallel to the rail car dump line. Their white underbelly's "glowing" brilliantly orange, phoenix like they hovered there almost motionless reflecting the bright yellow-orange and red hues of the cooling slag. It was like they were on fire it was so bright in the fading light of the day. It was the only beautiful sight to see in an otherwise desolate and foreboding wasteland of glassy rock-like congealed blast furnace slag.
Geneva Works is now defunct.
mrc109Â
y'ever get haunted by the fear you will never write anything as beautiful as the US Steel Pipe Works Slag Dump Youtube Comment cuz hoo boy i sure do:
shoutout to you, youtube user mrc109, wherever you may be today
#Wish I'd scrolled down and clicked the link first#my freaking eyes hurt reading that#though i suspect not as much as they would from actually doing the job
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VX-9 F/A-18F Spotted With Heavy Air-to-Air Load of AIM-174s and AIM-120s
The U.S. Navy is continuing to test the new AIM-174B missile, derived from the SM-6, aboard the Super Hornet, with a VX-9 jet carrying four AIM-174s, three AIM-120s and two AIM-9Xs.
Stefano D'Urso
Super Hornet four AIM-174s
The F/A-18F "Vandy 1" of VX-9 loaded with four CATM-174B, three CATM-120 and two CATM-9X. (Image credit: @point_mugu_skies)
A U.S. Navy F/A-18F Super Hornet of VX-9 âVampiresâ was spotted with a heavy air-to-air loadout, which includes four AIM-174Bs, three AIM-120s and two AIM-9Xs, in addition to a targeting pod and an InfraRed Search and Track installed on the external fuel tank. Aviation photographer @point_mugu_skies was one of the few to capture the aircraft in this previously unseen configuration and kindly provided us the images you can see in this article.
The aircraft is the Vampiresâ flagship, âVandy 1â, which sports the black livery applied for the unitâs 30th anniversary to pay tribute to the original one which was used on VX-4 commanderâs F-4s and F-14s, also known as âVandy 1â. The callsign originated from the abbreviation of the unitâs official callsign âVanderbiltâ used at the time.
As The Aviationist has reported in detail in the last few months, the AIM-174B is a Standard Missile (SM) 6 variant developed for the air-to-air role. The SM-6 is the surface-to-air missile designed to be used on Navy ships in conjunction with the Aegis Combat System and also known as the RIM-174 Standard Extended Range Active Missile (ERAM).
The idea of adapting the SM-6 to be air-launched is not new, as the weapon was already seen on a Super Hornet of VX-31 in 2018 and 2021. However, it wasnât until earlier this year that the testing got a new impulse and operational units were involved.
In fact, after another F/A-18 was spotted in April with an SM-6 under the wing, the weapon then appeared on operational jets assigned to the USS Carl Vinson aircraft carrier during the Rim of The Pacific 2024 (RIMPAC 2024) exercise in July. The heaviest load seen so far included two AIM-174s and two AIM-120s.
The one seen in the latest photo is reportedly the heaviest air-to-air load to date with the new weapon, with the AIM-174 both on the inner and middle wing hardpoints. Itâs interesting to note also the presence on the external fuel tank of the ASG-34A IRST, which acts as a complementary sensor to the AN/APG-79 fire control radar in a heavy electronic attack or radar-denied environment.
Another shot of the F/A-18F âVandy 1â with the heavy air-to-air loadout. (Image credit: @point_mugu_skies)
AIM-174B
As previously explained, the AIM-174 is an air-launched version of the RIM-174 Standard Extended Range Active Missile (ERAM), a crucial element of the US Navyâs air defense strategy. Integrated into the Aegis Combat System, the RIM-174 is primarily designed for long-range anti-air warfare but can also be employed for terminal phase ballistic missile defense and as an anti-ship missile. This year marked the first official combat use of the SM-6, with the Department of Defense confirming that the USS Carney intercepted and destroyed an anti-ship ballistic missile fired by Houthi rebels in the Gulf of Aden on January 30, 2024.
The SM-6 uses the airframe of the SM-2ER Block IV (RIM-156A) missile, upgraded with an active radar homing seeker derived from the AIM-120 AMRAAM air-to-air missile. This missile can reach speeds of up to Mach 3.5 and has a maximum range of 200 nautical miles. To that respect, itâs not clear what the maximum range of the air-launched version could be: despite the lack of a booster, launching it at high speed and altitude would result in significantly greater range compared to the surface-launched variant.
With the induction of the AIM-174B into service, the U.S. Navy joins a number of air arms capable of deploying an extra-long-range beyond-visual-range air-to-air missile (BVRAAM), like the MBDA Meteor, the Russian R-37M and Chinese PL-15 and PL-21. In fact, the AIM-174B enables the U.S. Navy Super Hornets to engage targets at much greater distances than is currently possible with the AIM-120 AMRAAM. Integrated with the E-2D, F-35, and AEGIS within the Naval Integrated Fire Control-Counter Air (NIFC-CA) system, the AIM-174B would extend the Navyâs capability to intercept aerial targets at ranges comparable to (if not greater than) those achieved against naval targets using the baseline SM-6.
In essence, this new missile fills the gap left by the retirement of the AIM-54 Phoenix. The AIM-54 was a long-range air-to-air missile used by the U.S. Navyâs F-14 Tomcat and retired in 2004 alongside the F-14. Known for its impressive range of over 100 nautical miles and multiple-target engagement capability, the AIM-54 left a significant void in long-range engagement capabilities.
While there wasnât a direct replacement for the AIM-54 Phoenix in terms of range, the U.S. military has been developing advanced air-to-air missiles to enhance its fighter aircraft capabilities. The AIM-260 Joint Advanced Tactical Missile (JATM) is one such development intended to replace the AIM-120 AMRAAM. Although not a direct replacement for the AIM-54 Phoenix, the AIM-260 aims to offer improved range and performance compared to the AIM-120.
SM-6
I
F/A-18E of VFA-192 carrying two air-launched SM-6 missiles (Image credit: @aeros808)
Operationally deployed
The photo of the new weapon during a test flight in April 2024 was reportedly part of the testing that preceded the delivery of the AIM-174B to the squadron likely to carry out Operational Test and Evaluation (OT&E), a testing phase conducted on production, or production representative weapons, to determine whether systems are operationally effective and suitable to support a Full-Rate Production (FRP) decision.
In July, the U.S. Navy acknowledged that the AIM-174 is operationally deployed, likely in Initial Operating Capability (IOC) with the CVW-2 Air Wingâs Super Hornet squadrons aboard the USS Carl Vinson (CVN-70), as reported by Naval News. âThe SM-6 Air Launched Configuration (ALC) was developed as part of the SM-6 family of missiles and is operationally deployed in the Navy today,â said a U.S. Navy spokesperson.
While the service acknowledged the existence and the deployment of the weapon, so far only the NAIM-174B inert, CATM-174B captive carry, and DATM-174B ground training variants were seen installed on aircraft. However, the fact that the Navy mentioned the weapon being operationally deployed implies that live variants might also been delivered.
The Navy did not disclose other details about the AIM-174. So far, we know the standard SM-6 missile is about 21 feet (6.4 meters) long and, using persons for scale in some of the few photos available, the AIM-174B seems to be of similar length. According to the stencils visible on the photos of the missile carried by the CVW-2 Super Hornets taking part in RIMPAC, the weapon weighs 1,890 lb Âą 14 lb (857 kg Âą 6 kg).
Thanks again to @point_mugu_skies for the photos he sent us and make sure to follow him on Instagram for more!
About Stefano D'Urso
Stefano D'Urso is a freelance journalist and contributor to TheAviationist based in Lecce, Italy. A graduate in Industral Engineering he's also studying to achieve a Master Degree in Aerospace Engineering. Electronic Warfare, Loitering Munitions and OSINT techniques applied to the world of military operations and current conflicts are among his areas of expertise.
@TheAviationist .com
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Sentinel-2C sealed in the Vega rocket fairing
As preparations continue to launch the Copernicus Sentinel-2C satellite on 4 September, the team at Europe's Spaceport in Kourou, French Guiana, has bid farewell to their precious satellite as it was sealed from view within the Vega rocket fairing.
Once in orbit, Sentinel-2C will provide high-resolution images for a wide range of applications including land, water and atmospheric monitoring, as are currently provided by Sentinel-2A and Sentinel-2B.
Since its arrival at the spaceport in July, Sentinel-2C has been undergoing all that it takes to get it ready for liftoff. This includes a huge number of careful checks to ensure all its components are in good working order, the hazardous task of loading the satellite with over 130 kg of volatile fuel and mating the satellite the Vega to the launch adapter.
And now, the teams have encapsulated the satellite within the rocket fairing. Apart from being a significant milestone on the road to liftoff, it is also somewhat emotional as the satellite itself won't be seen again.
ESA's Sentinel-2C launch campaign manager, Patricia Lopez, said, "The campaign to ready Sentinel-2C for launch has gone extremely well and this is thanks to the hard work from all the teams involved. Indeed, encapsulation is an important milestone and while we are extremely happy to have reached this point, it was also time for us to say farewell.
"For a very short time before the fairing closure, the lucky ones who were here could see the satellite as never before, all dressed-up in its flight configuration and looking like a precious jewel that we will now keep safely packed until launch."
"Clearly, the real good-byes will come in less than two weeks nowâliftoff is scheduled for 3 September at 22:50 local time here in Kourou, which is 4 September 03:50 CESTâwhich we are all very much looking forward to."
As its name suggests, Sentinel-2C is the third in the Sentinel-2 series. Once commissioned in orbit, it will replace its predecessor, Sentinel-2A, which was launched in 2015. Later, Sentinel-2D will replace Sentinel-2B.
This all ensures the continuity of imagery for Copernicus Services and beyond.
The mission provides high-resolution optical imagery for a wide range of applications including land, water and atmospheric monitoring. The mission is based on a constellation of two identical satellites flying in the same orbit but 180° apart.
The satellites each carry a high-resolution multispectral imager that generates optical images in the visible, near-infrared and shortwave-infrared part of the electromagnetic spectrum. From their altitude of 786 km, they provide continuous imagery in 13 spectral bands with resolutions of 10 m, 20 m and 60 m, with a large swath width of 290 km.
Sentinel-2C will be taken into orbit on a Vega rocketâin fact the last rocket of its kind. Vega will be superseded by the new Vega-C.
IMAGE: Sentinel-2C being lifted onto the Vega launch adapter. Credit: ESA-CNES-ARIANESPACE/Optique vidĂŠo du CSGâS. Martin
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