View allAll Photos Tagged multiband
Created from RAW data of spitzer space telescope
This Spitzer infrared image is a composite mosaic obtained with the multiband imaging photometer and the infrared array camera. Thermal infrared emission at 24 microns detected by the photometer (red) is combined with camera data at 8.0 microns (green) and 3.6 microns (blue).
The 3.6-micron near-infrared data (blue) traces the distribution of stars, although the Spitzer image is virtually unaffected by obscuring dust and reveals a very smooth stellar mass distribution, with the spiral arms relatively subdued.
As one moves to longer wavelengths, the spiral arms become the dominant feature of the galaxy. The 8-micron emission (green) is dominated by infrared light radiated by hot dust that has been heated by nearby luminous stars.
The core is less blueish as compared to original spitzer image to show the delicate spiral structures around the core. I needed to scale up the 24 micron image , so red halos appear but i used minimum filter to reduce this artifact, but extensive use caused a loos in data in this channel so i used it moderately
It is a five channel composite,
3.6 , 4.5 , 5.8 , 8.0 and 24 microns.
Credits: Bipradeep Saha / NASA / SHA
The Pinwheel galaxy, otherwise known as Messier 101, sports bright reddish edges in this new infrared image from NASA's Spitzer Space Telescope. Research from Spitzer has revealed that this outer red zone lacks organic molecules present in the rest of the galaxy. The red and blue spots outside of the spiral galaxy are either foreground stars or more distant galaxies.
The organics, called polycyclic aromatic hydrocarbons, are dusty, carbon-containing molecules that help in the formation of stars. On Earth, they are found anywhere combustion reactions take place, such as barbeque pits and exhaust pipes. Scientists also believe this space dust has the potential to be converted into the stuff of life.
Spitzer found that the polycyclic aromatic hydrocarbons decrease in concentration toward the outer portion of the Pinwheel galaxy, then quickly drop off and are no longer detected at its very outer rim. According to astronomers, there's a threshold at the rim where the organic material is being destroyed by harsh radiation from stars. Radiation is more damaging at the far reaches of a galaxy because the stars there have less heavy metals, and metals dampen the radiation.
The findings help researchers understand how stars can form in these harsh environments, where polycyclic aromatic hydrocarbons are lacking. Under normal circumstances, the polycyclic aromatic hydrocarbons help cool down star-forming clouds, allowing them to collapse into stars. In regions like the rim of the Pinwheelas well as the very early universestars form without the organic dust. Astronomers don't know precisely how this works, so the rim of the Pinwheel provides them with a laboratory for examining the process relatively close up.
In this image, infrared light with a wavelength of 3.6 microns is colored blue; 8-micron light is green; and 24-micron light is red. All three of Spitzer's instruments were used in the study: the infrared array camera, the multiband imaging photometer and the infrared spectrograph.
Band alumni, parents, and friends gathered before Multibands to enjoy great company, drinks, and hors d’oeuvres. The 2017 recipients of the Band Alumni Scholarship and the 2017 Minuteman Band Hall of Fame class were honored and attendees got the first look at a special portrait of legendary former Minuteman Band announcer Jim MacRostie — as well as the band’s new uniforms!
The atomic bomb dropped on Nagasaki was actually intended for Kokura but due to heavy cloud over Kokura the next target is Nagasaki.
This image from NASA's Spitzer Space Telescope shows infant stars "hatching" in the head of the hunter constellation, Orion. Astronomers suspect that shockwaves from a supernova explosion in Orion's head, nearly three million years ago, may have initiated this newfound birth..
.
The region featured in this Spitzer image is called Barnard 30. It is located approximately 1,300 light-years away and sits on the right side of Orion's head, just north of the massive star Lambda Orionis..
.
Wisps of green in the cloud are organic molecules called polycyclic aromatic hydrocarbons (PAHs). PAHs are formed anytime carbon-based materials are burned incompletely. On Earth, they can be found in the sooty exhaust from automobile and airplane engines. They also coat the grills where charcoal-broiled meats are cooked..
.
Tints of orange-red in the cloud are dust particles warmed by the newly forming stars. The reddish-pink dots at the top of the cloud are very young stars embedded in a cocoon of cosmic gas and dust. Blue spots throughout the image are background Milky Way along this line of sight..
.
This composite includes data from Spitzer's infrared array camera instrument, and multiband imaging photometer instrument. Light at 4.5 microns is shown as blue, 8.0 microns is green, and 24 microns is red.
Band alumni, parents, and friends gathered before Multibands to enjoy great company, drinks, and hors d’oeuvres. The 2017 recipients of the Band Alumni Scholarship and the 2017 Minuteman Band Hall of Fame class were honored and attendees got the first look at a special portrait of legendary former Minuteman Band announcer Jim MacRostie — as well as the band’s new uniforms!
Vallone di Ribordone
Parco Nazionale del Gran Paradiso - Piemonte/Valle d'Aosta - Italia
Autopano PRO Pano-5 immagini-5974x3243-proiezione Sferica-interpolazione Bilineare-unione Multibanda
Edited Spitzer Space Telescope PR image of the Cepheus C and Cepheus B region and associated nebula. Inverted grayscale variant.
Image source: photojournal.jpl.nasa.gov/catalog/PIA23126
Original caption: This image was compiled using data from NASA's Spitzer Space Telescope using the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer (MIPS) during Spitzer's "cold" mission, before the spacecraft's liquid helium coolant ran out in 2009. The colors correspond with IRAC wavelengths of 3.6 microns (blue), 4.5 microns (cyan) and 8 microns (green), and 24 microns (red) from the MIPS instrument.
The green-and-orange delta filling most of this image is a nebula, or a cloud of gas and dust. This region formed from a much larger cloud of gas and dust that has been carved away by radiation from stars.
The bright region at the tip of the nebula is dust that has been heated by the stars' radiation, which creates the surrounding red glow. The white color is the combination of four colors (blue, green, orange and red), each representing a different wavelength of infrared light, which is invisible to human eyes.
The massive stars illuminating this region belong to a star cluster that extends above the white spot.
On the left side of this image, a dark filament runs horizontally through the green cloud. A smattering of baby stars (the red and yellow dots) appear inside it. Known as Cepheus C, the area is a particularly dense concentration of gas and dust where infant stars form. This region is called Cepheus C because it lies in the constellation Cepheus, which can be found near the constellation Cassiopeia. Cepheus-C is about 6 light-years long, and lies about 40 light-years from the bright spot at the tip of the nebula.
The small, red hourglass shape just below Cepheus C is V374 Ceph. Astronomers studying this massive star have speculated that it might be surrounded by a nearly edge-on disk of dark, dusty material. The dark cones extending to the right and left of the star are a shadow of that disk.
The smaller nebula on the right side of the image includes a blue star crowned by a small, red arc of light. This "runaway star" is plowing through the gas and dust at a rapid clip, creating a shock wave or "bow shock" in front of itself.
Some features identified in the annotated image are more visible in the IRAC data alone, found here.
The Jet Propulsion Laboratory in Pasadena, California, manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate in Washington. Science operations are conducted at the Spitzer Science Center at Caltech in Pasadena. Space operations are based at Lockheed Martin Space Systems in Littleton, Colorado. Data are archived at the Infrared Science Archive housed at IPAC at Caltech. Caltech manages JPL for NASA.
For more information on Spitzer, visit:
www.nasa.gov/spitzer and www.spitzer.caltech.edu/
Image Credit:
NASA/JPL-Caltech
Image Addition Date:
2019-05-30
Fabricada en material transpirable multibanda con dos bandas cruzadas, ballenas verticales en la espalda y cierre velcro delantero. Incorpora una placa lumbar de foam para dar calor en dicha zona, la cual puede retirarse cuando no se precise. Comodidad de uso y tacto suave en contacto con la piel. Tratamientos pre y post-quirúrgicos.
Para más información: www.exclusivasiglesias.com/es/product/ortesis-tronco/faja...
The Large Aperture Multiband Deployable Antenna (LAMDA) at Kunsan Air Base, Republic of Korea, receives signals to help boost the 8th Communication Squadron's capabilities, Jan. 14, 2009, during a Peninsula Wide Operation Readiness Exercise. The LAMDA, along with the U.S. Air Force Airmen that run it, are assigned to the 607th Air and Space Communications Squadron at Osan Air Base, Republic of Korea. (U.S. Air Force Photo by Staff Sgt. Jason Colbert/Released)
W5RTA (South Texas DX and Contest Club station near Bandera, Texas) - Photo by K5NON all rights reserved. If you'd like to use this photo please contact K5NON via qrz.com email or the contact page at photompr.com
Band alumni, parents, and friends gathered before Multibands to enjoy great company, drinks, and hors d’oeuvres. The 2017 recipients of the Band Alumni Scholarship and the 2017 Minuteman Band Hall of Fame class were honored and attendees got the first look at a special portrait of legendary former Minuteman Band announcer Jim MacRostie — as well as the band’s new uniforms!
Il Soundblox® Pro Multiwave Distortion incorpora 23 tipi di effetti diversi, moderni ed accattivanti, più un equalizzatore grafico a 7 bande e sei memorie a disposizione dell'utente. Con tutte queste caratteristiche di flessibilità e programmabilità è un pedale perfetto sia per il live che per lo studio di registrazione.
Quello che rende unico Multiwave è la possibilità di poter eseguire la distorsione processando il segnale sia in modalità singola che multi-banda. Il processo multi-banda divide il segnale in distinte frequenze, poi esegue la distorsione separatamente e ricombina il segnale per l'uscita. Il risultato è una distorsione chiara con un robusto attacco e una ottima articolazione di note.Il processo in modalità singola banda usa invece un approccio più convenzionale, applicando la distorsione all'intero segnale. Il risultato è un set di toni per chitarra "classici" ma ugualmente espressivi. Le categorie di processo sono ulteriormente suddivise in tre sottocategorie che vanno dal "normale" per una curva di distorsione tradizionale, al settaggio estremo "foldback" e "octave" per avere un suono più aggressivo e una distorsione da synth.
L'equalizzatore grafico a 7 bande con un controllo di +/-12 dB da la possibilità di fare una seria manipolazione sul suono. Inoltre i suoni personali possono essere salvati nelle sei memorie preset, pronti ad essere richiamati velocemente tramite tre footswitch.
La serie Pro include anche un MIDI input che permette un accesso ai preset e ai parametri tramite un MIDI controller esterno, ed è compatibile con il controllo di movimento Hot Hand® per avere ancora più capacità espressive.
Caratteristiche:
• Ampia gamma di suoni - 23 varianti dei nostri unici algoritmi di distorsione più una modalità CLEAN BOOST + EQ.
• Processore Multibanda - Il segnale viene diviso in bande per poi essere distorto individualmente per ottenere un suono più chiaro.
• DSP ultima generazione - Digital Signal Processor proprietario della Source Audio a 56 bit, il SA601, e convertitori AD/DA a 24-bit totalmente trasparenti.
• 6 preset programmabili - Preset facili da programmare in due banchi selezionabili con i tre interruttori per un accesso veloce accesso ai suoni preferiti.
• Equalizzatore a 7 bande — Equalizzatore a 7 bande estremamente preciso, memorizzabile nei preset per un controllo del suono più accurato .
• Sound Morphing - Ingresso per pedale d'espressione permette il passaggio morbido da un suono all'altro dei vari banchi di preset.
• Compatibilità MIDI - Ingresso MIDI per avere accesso dall'esterno ai preset e ai parametri
• Motion Control - tutti i pedali Soundblox e Soundblox Pro sono "Hot Hand® Ready" e possono essere usati con qualsiasi sensore di movimento Hot Hand® in modo da estendere la compatibilità delle unità .
• Active Analog Bypass - nel modo bypass il segnale di ingresso viene completamente escluso dal DSP in modo da non avere degradazioni del segnale (zero signal degradation).
• Alimentatore a 9V incluso.
• Dimensioni: 17.8cm (profondità ) x 15.25cm (larghezza) x 5cm (altezza, incluse le manopole).
Prezzo al pubblico: € 214,00 (iva esclusa)
------
Distribuito in Italia da Reference Laboratory s.r.l.
(Click on the picture and turn your phone sideways to fully see everything)
24P/ Schaumasse
This is a wide field two panel mosaic which was imaged on the morning of December 28, 2025 from my backyard. Comet 24P/ Schaumasse (green glow on the left side) made a somewhat close approach to Markarian’s Chain (line of galaxies on the right side).
Markarian’s Chain is a string of galaxies in the Virgo Cluster. This area of the night sky is filled with galaxies which are as far as 50-60 million light years away. 24P/ Schaumasse is a Jupiter family comet. It has an orbital period of 8.27 years.
During the month of December the weather had been mild and clear in the US southwest but shortly before Christmas, a series of storms finally started to bring clouds and precipitation. For that reason, I missed a couple good photographic opportunities. Luckily, the weather cleared just in time for me to get this image but not without some struggle.
I had to deal with dew and humidity on this particular morning. I normally have a dew heater attached to my main scope but since dew isn’t a big problem in the US southwest, I don’t have a dew heater on my guide scope. It was so humid that morning that the guide scope started to fog. I had trouble guiding. Fortunately, making a makeshift and oversized cardboard dew shield in the wee hours of the morning for the guide scope solved the problem!
Image Detail:
- 3 hours of total integration time (120 seconds, gain 100, camera cooled to 14 degrees). Both panels 1.5 hours of integration time.
- SVBONY SV503 80ED
- SVBONY SV260 multiband pass filter
- SVBONY SV226 filter drawer
- Sky Watcher Star Adventurer GTi
- ZWO ASI 2600MC Pro
- ZWO ASIAIR Mini
- ZWO EAF
- ZWO 120MM guide camera
- ZWO guide scope
Software:
- PixInsight
- Adobe Photoshop
- RC Astro Blur Xterminator
- RC Astro Noise Xterminator
- RC Astro Star Xterminator
Looking like a spiders web swirled into a spiral, the galaxy IC 342 presents its delicate pattern of dust in this image from NASAs Spitzer Space Telescope. Seen in infrared light, the faint starlight gives way to the glowing bright patterns of dust found throughout the galaxys disk.
At a distance of about 10 million light-years, IC 342 is relatively close by galaxy standards, however our vantage point places it directly behind the disk of our own Milky Way. The intervening dust makes it difficult to see in visible light, but infrared light penetrates this veil easily. It belongs to the same group as its even more obscured galaxy neighbor, Maffei 2.
IC 342 is nearly face-on to our view giving a clear, top-down view of the structure of its disk. It has a low surface brightness compared to other spirals, indicating a lower density of stars (seen here in blue). Its dust structures show up much more vividly (yellow-green).
New stars are forming in the disk at a healthy clip. Glowing like gems trapped in the web, regions of heavy star formation appear as yellow-red dots due to the glow of warm dust. The very center glows especially brightly in the infrared, highlighting an enormous burst of star formation occurring in this tiny region. To either side of the center, a small bar of dust and gas is helping to fuel this central star formation.
Data from Spitzers infrared array camera (IRAC) are shown in blue (3.6 and 4.5 microns) and green (5.8 and 8.0 microns) while the multiband imaging photometer (MIPS) observation is red (24 microns).
(yeah, celebrates finding some girl's gymnastics trophy)
Josh Stewart - multiband trumpet player, insturment and set builder, frequent model for the photographer Chris Engman, smartass, sweetheart, and original member of the www.degenerateartensemble.com
hahaha used here:
www.dumblittleman.com/2007/02/win-100-from-dumb-little-ma...
JAMINDAN, Philippines --U.S. Army soldier Cpl. Jeremy Boldt, assigned to 2nd Battalion, 3rd Infantry Regiment uses an Multiband Inter/Intra Team Radio in the jungle, during a combined-joint operation Handa Koa for Balikatan, April 14th, 2016. This year marked the 32nd iteration of the annual exercise Balikatan, which is an annual Philippine-U.S. military bilateral training exercise that is a signature element of the Philippine-U.S. alliance focused on a variety of missions, including humanitarian assistance, maritime law enforcement, and environmental protection. (U.S. Navy photo by Mass Communication Specialist 2nd Class Jerome D. Johnson)
Band alumni, parents, and friends gathered before Multibands to enjoy great company, drinks, and hors d’oeuvres. The 2017 recipients of the Band Alumni Scholarship and the 2017 Minuteman Band Hall of Fame class were honored and attendees got the first look at a special portrait of legendary former Minuteman Band announcer Jim MacRostie — as well as the band’s new uniforms!
he sousaphone players of the UMass Marching Band play for the audience of Friday's multibands concert as they exit.
Photo by Bryn Rothschild-Shea
Autosave-File vom d-lab2/3 dLeamington Spa, 1990 © neatephotos.com
The second in a series of classic multiband line up gigs from the early 1990s. I was living then in Oxford and caught a coach on Saturday not knowing where I'd stay. Fortunately the Preston crew secured a place for us all and I was back in time for a football match I was due to play in.
the Keatons, Thrilled Skinny & AC Temple 'live' in Leamington Spa: goo.gl/d53gqt
Band alumni, parents, and friends gathered before Multibands to enjoy great company, drinks, and hors d’oeuvres. The 2017 recipients of the Band Alumni Scholarship and the 2017 Minuteman Band Hall of Fame class were honored and attendees got the first look at a special portrait of legendary former Minuteman Band announcer Jim MacRostie — as well as the band’s new uniforms!
Edited Spitzer Space Telescope image of Rho Ophiuchi and its nebula. Color/processing variant.
Original caption: Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. Called "Rho Oph" by astronomers, it's one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth.
Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new stars to form from cold cosmic gas, with two long streamers trailing off in different directions. Recent studies using the latest X-ray and infrared observations reveal more than 300 young stellar objects within the large central cloud. Their median age is only 300,000 years, very young compared to some of the universe's oldest stars, which are more than 12 billion years old.
This false-color image of Rho Oph's main cloud, Lynds 1688, was created with data from Spitzer's infrared array camera, which has the highest spatial resolution of Spitzer's three imaging instruments, and its multiband imaging photometer, best for detecting cooler
materials. Blue represents 3.6-micron light; green shows light of 8 microns; and red is 24-micron light. The multiple wavelengths reveal different aspects of the dust surrounding and between the embedded stars, yielding information about the stars and their birthplace.
The colors in this image reflect the relative temperatures and evolutionary states of the various stars. The youngest stars are surrounded by dusty disks of gas from which they, and their potential planetary systems, are forming. These young disk systems show up as red in this image. Some of these young stellar objects are surrounded by their own compact nebulae. More evolved stars, which have shed their natal material, are blue.
This swirling landscape of stars is known as the North America nebula. In visible light, the region resembles North America, but in this new infrared view from NASA's Spitzer Space Telescope, the continent disappears.
Where did the continent go? The reason you don't see it in Spitzer's view has to do, in part, with the fact that infrared light can penetrate dust whereas visible light cannot. Dusty, dark clouds in the visible image become transparent in Spitzer's view. In addition, Spitzer's infrared detectors pick up the glow of dusty cocoons enveloping baby stars.
Clusters of young stars (about one million years old) can be found throughout the image. Slightly older but still very young stars (about 3 to 5 million years) are also liberally scattered across the complex, with concentrations near the "head" region of the Pelican nebula, which is located to the right of the North America nebula (upper right portion of this picture).
Some areas of this nebula are still very thick with dust and appear dark even in Spitzer's view. For example, the dark "river" in the lower left-center of the image -- in the Gulf of Mexico region -- are likely to be the youngest stars in the complex (less than a million years old).
The Spitzer image contains data from both its infrared array camera and multiband imaging photometer. Light with a wavelength of 3.6 microns has been color-coded blue; 4.5-micron light is blue-green; 5.8-micron and 8.0-micron light are green; and 24-micron light is red.
Banda ancha dorsal de tejido elástico multibanda transpirable. Dos bandas superiores que se prolongan sobre los hombros pasan por debajo de axilas, cruzan por la espalda y cierran en el abdomen permitiendo ejercer una tracción gradual de la espalda mediante la retropulsión de los hombros hasta suprimir la mala postura cifótica. Corrector de posiciones incorrectas y vicios posturales. No es recomendable utilizarla más de 3-4 horas al dÃa.
Para más información: www.exclusivasiglesias.com/es/product/ortesis-tronco/espa...
This cheap radio was pusrchased years ago to obtain the box for a electronic project, but the perfomance was so good so I decide not to use it.
G4ISJ/P 24/02/2012
Rig is ATS 4b by Steve Weber (KD1JV)
Multiband CW & PSK31.
4 - 5 Watts O/P
Altoids tin L tuner feeding EFHW
PSU 8xAA NiMh cells.
A very common endemic in Hawaii. Shown here with one of its favorite foods, Pocillopora coral. 105mm lens.
Multiband butterflyfish. (Chaetodon multicinctus)
Image ID: corl0023, NOAA's Coral Kingdom Collection
Location: Hawaii, Main Islands
Photographer: Kevin Lino NOAA/NMFS/PIFSC/ESD
This image layout compares visible (left) and infrared views of the North America nebula, taken by the Digitized Sky Survey and NASA's Spitzer Space Telescope, respectively..
.
The nebula is named after its resemblance to the North America content in visible light. This visible view highlights the eastern seaboard and Gulf of Mexico regions. In infrared light, the continent disappears. The "Mexican Riviera" -- the west coast of Mexico -- seems to invert in texture and brightness, as does the "neck" region of the Pelican nebula, named for its resemblance to a pelican. This nebula can be seen to the right of the North America nebula in the visible image. The Gulf of Mexico transforms from a dark cloud into a "river" of hundreds of young stars..
.
These pictures look different in part because infrared light can penetrate dust whereas visible light cannot. Dusty, dark clouds in the visible image become transparent in Spitzer's view. In addition, Spitzer's infrared detectors pick up the glow of dusty cocoons enveloping baby stars..
.
The Spitzer image contains data from both its infrared array camera and multiband imaging photometer. Light with a wavelength of 3.6 microns has been color-coded blue; 4.5-micron light is blue-green; 5.8-micron and 8.0-micron light are green; and 24-micron light is red.
This infrared image from NASA's Spitzer Space Telescope shows the Helix nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye.
The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these cosmic butterflies were named for their resemblance to gas-giant planets.
Planetary nebulae are actually the remains of stars that once looked a lot like our sun.
When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible-light colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years.
In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died.
The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded.
The Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found.
This image is made up of data from Spitzer's infrared array camera and multiband imaging photometer. Blue shows infrared light of 3.6 to 4.5 microns; green shows infrared light of 5.8 to 8 microns; and red shows infrared light of 24 microns.