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"Following backlash from the general public after the NMTV published an article on its secret dealings with off-world entities, EMIT and its vast factories had to get more hired security to combat the growing “threat” that apparently is the public. Obviously, this was really a way to combat agents of RORG from infiltrating the organization even more. They’ve been going at the group in multiple ways, using such “notable” publishing organizations as the WOT to slander the group as enemies of the state, a threat on democracy and those who wish to suppress order in the future. That’s just what’s above ground, what’s in visible sight anyways. Down in the lower levels, that where the real treachery is taking place. Using a system of sewers I was tipped off about, I made my way to a lesser known part of section 2. Here, they had built an instillation for some more darker purposes. It was originally disguised as a water cleaning hub designed to make the disgusting, messy and quite toxic sewer water drinkable. This was promised many years ago, but we knew this wasn’t going to ever happen. Coming up on the exit, I noticed parts, crates and lights coming from the facilities windows. This was no cleaning installation. Experiments and who knows what technology is being tested. Coming around now, two guards are noticing my presence. Better silence them before I have an army to deal with."
Here I am, on the eve of 2021 with my final MOC of the year. This was built for the RebelLUG Cyberpunk which I am proud to be apart of. Please not only comment on the build, but the story as well. Put some work into both.
If you like this build, consider tapping the fave button ever so slightly and if you’re feeling like doing a bit extra, follow me here. Thanks!
~Noah
Emitting a pungent blue haze of exhaust 56064 is crawling out of Barry Docks with the 15.15 Barry to Burn Naze service.
The docks are the merest shadow of the once busy coal port which shipped good Welsh steam coal out to destinations all over the world.
56064 was built at Doncaster Works, it entered service 17/09/1979. The locomotive was withdrawn in September 2008 and cut at C.F. Booth (Rotherham) in March 2009
Copyright Geoff Dowling 20/04/96: All rights reserved
The chimneys emitting heavy smokes as the work is at full flow in Kolaghat Thermal Power Corporation throughout the night.The picture is taken on board Puri Howrah Garibrath Express at the crack of dawn.
I hadn't bargained on "Mayflower" emitting quite as much clag as it sped through Twyford station with the "Chairman's Train" on a London Paddington circular private tour via Oxford.
Locomotive: Thompson B1 Class 4-6-0 61306 "Mayflower".
Location: Twyford station, Berkshire.
Photons emitted from the surface of the Sun (sunlight) take an average of 8 minutes and 20 seconds to travel to the Earth. So, when you look at the Sun, you're actually viewing about 8 minutes in the past.
Why did I say "an average of"? Obviously, the speed of light doesn't change. However, the Earth's distance to the Sun does change, due to its elliptical orbit.
By comparison, other stars in the night sky are so far away from us, light takes much, much longer to reach us. From the closest stars, light takes a few years to get to Earth. From the farthest stars, light has taken literally billions of years to reach us.
So when you view these stars, you are actually viewing the distant, distant past. For instance, the light that you're seeing may have left that star while dinosaurs walked the Earth.
If you took the time to read this, I appreciate it. Hopefully, you found it interesting. I personally think the notion of viewing the distant past in the night sky is fascinating.
By the way, I took this photo of the sunset at a local park. I was able to capture the distant treetops over a large pond.
Curiosidades : Emite insistentemente un reclamo seco (tac), que repite con frecuencia irregular: tac-tac…, tac-tac-tac. El canto es más elaborado y melodioso. Reclama y canta a lo largo de todo el día, pero especialmente por la mañana muy temprano, incluso antes del amanecer.
Esta torre del siglo XIV, fue erigida por el obispo Diego de Padrón. Un sólido cubo defensivo coronado por almenas que fue utilizado, inicialmente, como torre vigía y después como campanario.
Su construcción finaliza en época del arzobispo Berenguel de Landoria, y a él se lo dedican.
Y la torre, contigua a la portada de As Praterías, ya tiene un nombre: La Berenguela.
En 1678, sobre el cubo gótico original, se instala un primer cuerpo cuadrado y sobre él, otro octogonal rematado por una linterna, en la que una luminaria indicar a los peregrinos el camino a la tumba del Apóstol.
Se enciende el primer día de los años Xacobeo y permanece así hasta el final del Año Santo.
La primera campana que se colocó en la torre fue en el año 1680, era considerada una campana con amplia mezcla de frecuencias acústicas y un sonido musicalmente muy agradable, pero se rajo y perdió su sonoridad original, siendo sustituida por otra construida en el año 1729. Campana que permaneció en activo hasta los años setenta del pasado siglo, ya que también se resquebrajo en 1976. Al final del Siglo XX la sustituyo la actual, fabricada en Holanda.
En el primer tercio del siglo XIX, se colocó un reloj en cada una de las cuatro caras de la torre, únicamente con la aguja horaria, ya que las horas las marca la Berenguela y los cuartos una campana más pequeña llamada, obviamente, campana de los cuartos.
En la linterna, en el remate sobre la cúpula, focos de tecnología led emiten una luz cálida, lo que le da un aspecto semejante a una llama y se convierte en un faro guía que señala en la noche, el sepulcro del apóstol Santiago.
Una hilera de fieles esperan ante la portada de As Praterías, la entrada al interior del templo para asistir a la Misa del Peregrino, que se celebra al mediodía en el altar mayor de la catedral.
...................................................................SIGUIENTE
Emission nebula lit by bright ultraviolet light from stars at the center.
Very active star forming region.
Nebula is 100 ly wide, and located at a distance of 5000 ly.
Latest results 12/2020 and 10/21
Telescope
ASA 500N, F-3.8
CAMERA FLI PL16803
50 cm Newtonian telescope
Chile
Telescope Live
200 minutes total exposure, SHO false color.
Pixinsight and photoshop, LR
Pro data set and advanced request.
“The Rosette Nebula (also known as Caldwell 49) is an H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula's matter.
The complex has the following New General Catalogue (NGC) designations:
NGC 2237 – Part of the nebulous region (Also used to denote whole nebula)
NGC 2238 – Part of the nebulous region
NGC 2239 – Part of the nebulous region (Discovered by John Herschel)
NGC 2244 – The open cluster within the nebula (Discovered by John Flamsteed in 1690)
NGC 2246 – Part of the nebulous region
The cluster and nebula lie at a distance of 5,000 light-years from Earth and measure roughly 130 light years in diameter. The radiation from the young stars excites the atoms in the nebula, causing them to emit radiation themselves producing the emission nebula we see. The mass of the nebula is estimated to be around 10,000 solar masses.
A survey of the nebula with the Chandra X-ray Observatory has revealed the presence of numerous new-born stars inside optical Rosette Nebula and studded within a dense molecular cloud. Altogether, approximately 2500 young stars lie in this star-forming complex, including the massive O-type stars HD 46223 and HD 46150, which are primarily responsible for blowing the ionized bubble.Most of the ongoing star-formation activity is occurring in the dense molecular cloud to the south east of the bubble.
A diffuse X-ray glow is also seen between the stars in the bubble, which has been attributed to a super-hot plasma with temperatures ranging from 1 to 10 million K.” Wikipedia
A shot of a speaker that i took in a warehouse in Hull. This speaker was just dangling above a doorway. I light painted this with an LED torch and a blue gel. I shot this RAW and with a 10-20mm lens
The Sun emitted a strong solar flare, peaking at 7:14 p.m. ET on July 2, 2023. NASA’s Solar Dynamics Observatory, which watches the Sun constantly, captured an image of the event.
Solar flares are powerful bursts of energy. Flares and solar eruptions can impact radio communications, electric power grids, navigation signals, and pose risks to spacecraft and astronauts.
This flare is classified as an X1.0 flare. X-class denotes the most intense flares, while the number provides more information about its strength.
To see how such space weather may affect Earth, please visit NOAA’s Space Weather Prediction Center spaceweather.gov/, the U.S. government’s official source for space weather forecasts, watches, warnings, and alerts. NASA works as a research arm of the nation's space weather effort. NASA observes the Sun and our space environment constantly with a fleet of spacecraft that study everything from the Sun's activity to the solar atmosphere, and to the particles and magnetic fields in the space surrounding Earth.
Image Credit: NASA/SDO
#NASA #space #NASAMarshall #msfc #sun #heliophysics #NASAGoddard #SolarDynamicObservatory #SDO
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Thor's Helmet or NGC 2359 is an emission nebula with a ionized HII region in the constellation of Canis Major. The nebula is about 30 light-years wide and lies about 12 000 light-years from Earth. The central star is a very hot Wolf-Rayet WR7 star, believed to be in a presupernova stage of evolution. This star inflates the interstellar bubble by emitting a stream of charged particles that expands outwards, producing the interstellar bubble. This bubble in turn interacts with molecular clouds, causing the ionizing radiation that gives it its glow. This nebula is also known as Sharpless 2-298 or Gum 4.
Color image taken at the remote observatory from the E-Eye site in Spain. The image is composed of 23 hours of exposure time with the ZWO ASI-2600MC color camera using a Takahashi CCA250 f3.6 astrograph, riding a unguided 10Micron GM2000.
An X9.3 class solar flare flashes in the middle of the Sun on Sept. 6, 2017. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 171 and 131 angstrom wavelengths.
Image credit: NASA/GSFC/SDO
The sun emitted a solar flare on Dec. 4, 2014, seen as the flash of light in this image from NASA's Solar Dynamics Observatory. The image blends two wavelengths of extreme ultraviolet light – 131 and 171 Angstroms – which are typically colored in teal and gold, respectively. Read more: 1.usa.gov/121n7PP
Image Credit: NASA/SDO
The sun emitted a significant solar flare, peaking at 5:40 p.m. EDT on Oct. 24, 2014. The flare erupted from a particularly large active region -- labeled AR 12192 -- on the sun that is the largest in 24 years. This is the fourth substantial flare from this active region since Oct. 19.
Read more: www.nasa.gov/content/goddard/giant-sunspot-erupts-with-4t...
Guttation is the loss of water in the form of water droplets from hydathodes (small pores) on the leaf margin of a small herbacious plant.
There is a difference between Guttation and Dew. Dew is formed on the plant's surface from condensation of moisture in the air. Guttation, on the other hand, is moisture emitted from the plant itself.
Phenomena across the Universe emit radiation spanning the entire electromagnetic spectrum — from high-energy gamma rays, which stream out from the most energetic events in the cosmos, to lower-energy microwaves and radio waves.
Microwaves, the very same radiation that can heat up your dinner, are produced by a multitude of astrophysical sources, including strong emitters known as masers (microwave lasers), even stronger emitters with the somewhat villainous name of megamasers and the centers of some galaxies. Especially intense and luminous galactic centers are known as active galactic nuclei. They are in turn thought to be driven by the presence of supermassive black holes, which drag surrounding material inwards and spit out bright jets and radiation as they do so.
The two galaxies shown here, imaged by the NASA/ESA Hubble Space Telescope, are named MCG+01-38-004 (the upper, red-tinted one) and MCG+01-38-005 (the lower, blue-tinted one). MCG+01-38-005 (also known as NGC 5765B) is a special kind of megamaser; the galaxy’s active galactic nucleus pumps out huge amounts of energy, which stimulates clouds of surrounding water. Water’s constituent atoms of hydrogen and oxygen are able to absorb some of this energy and re-emit it at specific wavelengths, one of which falls within the microwave regime, invisible to Hubble but detectable by microwave telescopes. MCG+01-38-005 is thus known as a water megamaser!
Image Credit: ESA/Hubble & NASA
For this image, the NASA/ESA Hubble Space Telescope turned its powerful eye toward an emission-line galaxy called NGC 3749.
When astronomers explore the contents and constituent parts of a galaxy somewhere in the universe, they use various techniques and tools. One of these is to spread out the incoming light from that galaxy into a spectrum and explore its properties. This is done in much the same way as a glass prism spreads white light into its constituent wavelengths to create a rainbow. By hunting for specific signs of emission from various elements within a galaxy’s spectrum of light —so-called emission lines — or, conversely, the signs of absorption from other elements — so-called absorption lines — astronomers can start to deduce what might be happening within.
If a galaxy’s spectrum shows many absorption lines and few emission lines, this suggests that its star-forming material has been depleted and that its stars are mainly old, while the opposite suggests it might be bursting with star formation and energetic stellar newborns. This technique, known as spectroscopy, can tell us about a galaxy’s type and composition, the density and temperature of any emitting gas, the star formation rate, or how massive the galaxy’s central black hole might be.
While not all galaxies display strong emission lines, NGC 3749 does. It lies over 135 million light-years away and is moderately luminous. The galaxy has been used as a “control” in studies of especially active and luminous galaxies — those with centers known as active galactic nuclei, which emit copious amounts of intense radiation. In comparison to these active cousins, NGC 3749 is classified as inactive, and has no known signs of nuclear activity.
Image credit: ESA/Hubble & NASA, D. Rosario et al.
More about Chandra's 20th Anniversary
The sun emitted a trio of mid-level solar flares on April 2-3, 2017. The first peaked at 4:02 a.m. EDT on April 2, the second peaked at 4:33 p.m. EDT on April 2, and the third peaked at 10:29 a.m. EDT on April 3. NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured images of the three events. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however — when intense enough — they can disturb the atmosphere in the layer where GPS and communications signals travel.
Image Credit: NASA/SDO
At this time of year in the UK, it gets dark very very late in the evening. And when you're a wage slave like me, staying up till 3am is not a good idea with the ensuing hangover I get from lack of sleep! So when @ryuslightworks and his partner decided to take a holiday in the UK, who am I to refuse a lightpainting session in the dark?
To get around staying up so late in the evening, I suggested we collaborate in a local to me abandoned railway tunnel. I've visited and lightpainted in the tunnel quite a few times and knew it would be a safe bet to provide a dark location. And not to mention at a more socialable and work friendly hour!
One of the items of lightpainting gear Dennis had brought along was his Laser Cube. I've been eager to see one of these cool laser devices which emit all kinds of static and moving laser lights of all colours. You can see details for the Laser Cube here: www.laseros.com/lasercube/?wcmlc=GBP
This is a camera rotated image where the camera is rotated on it's lens axis and is created in one photographic exposure.
The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 2015. NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel.
This flare is classified as an M5.6-class flare. M-class flares are a tenth the size of the most intense flares, the X-class flares. The number provides more information about its strength. An M2 is twice as intense as an M1, an M3 is three times as intense, etc.
Credit: NASA/Goddard/SDO
NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.
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An LED video light, taken using a star filter; the result given the NIK Collection Silver Efex Pro Bleach Bypass and Infrared Filter treatment in Photoshop.
Volatile terpenoids emitted in large quantities by the abundant eucalyptus trees in the Blue Mountains may cause Mie scattering and thus the blue haze for which the mountains were named.
Peveril Point in Swanage, Dorset. Earlier in the evening we had been here shooting lightning storms on the horizon as they crossed the channel between Calais and Dover, more than a hundred miles away.
A later visit for some quiet contemplation after midnight, produced a different form of optical phenomenon; Airglow. Similar in appearance to the aurora borealis, the Green glow is emitted by particles in Earth's upper atmosphere, energised by the sun's rays during the day. This process occurs all the time, all over our planet but there is usually far too much light pollution to see it in the UK. I've only ever seen it once before, coincidentally it was in the same location roughly two years ago.
As an amateur photographer, whose photographic skills have been described by an eminent friend and photographer as ‘sure as the earth is flat, the man can take an awesome image’, I am not always sure what to shoot. Do I go for that iconic spot or shoot something that hasn’t yet set the internet on fire? Like the rest of you outstanding landscape photographers, do I wait for that amazing light or keep shooting in the current bland light cursing all the while in Kodak chrome color? Do I pay attention to rules of photography and expectations of the human mind like a trained artist or do I shoot that Hilly Billy wind blowing over nothing? You see, it is never clear to me, what my role as a photographer exactly is.
But that is not the whole truth. I may not always know what to shoot, but I know what not to miss. Sometimes, certain moments in certain places emit a resonance that shiver my emotions and move me. These snippets of time and space are not always iconic, may not always have the best light or photographic contours, but they leave me speechless and strikingly alive. The Mono Lake dead bush, the dead dream atop the Watson Lake, the Grand Canyon Redwall lime-stone set ablaze by the setting sun, the moon shining through the smoky Yosemite tunnel, or, the milky way caressing Mt. Lassen in utter darkness... these are good examples of such extraordinary resonances. They are like eye-contacts with beautiful strangers that somehow drum up the heartbeat while lasting past that critical fourth second.
And then, there are eye contacts with glamorous eyes where it takes a few second to see past the initial bedazzlement and spot their turbulent and covert pain. The above place – hidden next to a beautiful wash in the Valley of Fire State Park – is one such siren that allured me in with its mind-numbing colors, lines and beauty. After a steep climb, I had a very narrow ledge to shoot this eye-candy from. While doing so, I noticed how this beautiful arch, which is in ruins, was bleeding for ages as pink sand and was resting all its hope on a weak pillar that was almost ready to give up. In contrary to above mentioned places, this place did not leave me speechless and alive. Resonating in a different channel, it instead left me numb and bereft of emotions … just as I feel when I must carry the unbearable within while wearing a lie-smile on the outside.
PS: This shot defies color-depth 'rules' of photography quite arrogantly. Guess what, it's one of those days today when defying something is all I feel like doing. (insert lie-smile) :-]
This is another shot of the Multiverse light sculpture by Leo Villareal. It is currently on display at the moving walkway at the National Gallery of Art in Washington, DC. The 40,000 light emitting diodes are constantly changing patterns as you move down the walkway between the East and West Gallery.
That 'tongue' - see inset - does look a bit like a Hoover, but it functions quite differently. Flies such as this Greenbottle don't chew or bite their food. Instead their mouthparts 'sponge', that is to say that they function by capillary action.
The labellum - the part of the 'tongue' that looks like the sucking end of our Hoover - has many grooves (visible only under a microscope) called pseudotracheae. If the food on its sweeping area is not sufficiently liquid they can emit a kind of saliva. The liquid mixture - in the case of these Alexanders flowers: nectar - moves upwards into Lucilia's narrow labium not by its own sucking action but through intermolecular forces in play between the liquid and the inner wall of the labial tube; so a bit like a sponge.
Yaaay! No storms tonight! Clear Sky, lots of ideas, and the lights cooperated! ;-)
Light Painting - Single Exposure
Son solitarios.
Los machos son territoriales y emiten sus cantos desde los árboles altos del bosque, lo que ayuda a que estos se difundan a una mayor distancia. Los machos estiran sus carúnculas mientras cantan y las contraen cuando salen del territorio para alimentarse. Las notas más fuertes se pueden escuchar hasta 0.5 km. de distancia o más. Mientras el macho emite sus notas, abre el pico ampliamente y exhibe su boca negra como una caverna.
Los machos poseen un territorio al que protegen y donde pasan todo el día. Lo abandonan por poco tiempo para alimentarse. Estos territorios varían en tamaño y fluctúan en extensión desde 70 por 30 m. hasta 450 por 50 m.
Los machos estiran las carúnculas mientras cantan y las retraen cuando salen del territorio para alimentarse. Casi siempre se alimentan fuera de su territorio y cuando esto sucede, o cuando visita el territorio de otro macho, retrae las carúnculas, mientras que el macho dominante (dueño del territorio) las extiende; posteriormente este último acompaña al subordinado fuera de su territorio.