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121002-M-PH080-271
Lance Cpl. Tony J. Keys-Fairclough with Marine Tactical Air Command Squadron 18 connects a RF-390 multiband vehicular whip antenna to an AN/MRQ 12(V) 4 communication interface system at Marine Corps Air Station Futenma Oct. 2. MTACS-18 fills a critical supporting role by providing communications to fellow service members engaged on the battlefield and in the skies above. Keys-Fairclough is an aviation communication system technician with MTACS-18, Marine Air Control Group 18, 1st Marine Aircraft Wing, III Marine Expeditionary Force. (U.S. Marine Corps photo by Lance Cpl. Brianna Turner/Released)
Description
Casio G-SHOCK The G Multiband 5 GW-M5600-1JF New Japanese Wristwatch
Condition: New
After your payment, I will send the item in 7days.
Shipping Cost by EMS
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Africa and South America : USD 20
I do very careful packing.
The reason is because it wants to send it in a complete state!
So the weight becomes heavier than you expected.
I will use carton case or cushioning .
(Don't worry about damage during shipping.)
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The infrared portrait of the Small Magellanic Cloud, taken by NASA's Spitzer Space Telescope, reveals the stars and dust in this galaxy as never seen before. The Small Magellanic Cloud is a nearby satellite galaxy to our Milky Way galaxy, approximately 200,000 light-years away..
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The image shows the main body of the Small Magellanic Cloud, which is comprised of the "bar" and "wing" on the left and the "tail" extending to the right. The bar contains both old stars (in blue) and young stars lighting up their natal dust (green/red). The wing mainly contains young stars. The tail contains only gas, dust and newly formed stars. Spitzer data has confirmed that the tail region was recently torn off the main body of the galaxy. Two of the tail clusters, which are still embedded in their birth clouds, can be seen as red dots..
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In addition, the image contains a galactic globular cluster in the lower left (blue cluster of stars) and emission from dust in our own galaxy (green in the upper right and lower right corners)..
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The data in this image are being used by astronomers to study the lifecycle of dust in the entire galaxy: from the formation in stellar atmospheres, to the reservoir containing the present day interstellar medium, and the dust consumed in forming new stars. The dust being formed in old, evolved stars (blue stars with a red tinge) is measured using mid-infrared wavelengths. The present day interstellar dust is weighed by measuring the intensity and color of emission at longer infrared wavelengths. The rate at which the raw material is being consumed is determined by studying ionized gas regions and the younger stars (yellow/red extended regions). The Small Magellanic Cloud, and its companion galaxy the Large Magellanic Cloud, are the two galaxies where this type of study is possible, and the research could not be done without Spitzer..
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This image was captured by Spitzer's infrared array camera and multiband imaging photometer (blue is 3.6-micron light; green is 8.0 microns; and red is combination of 24-, 70- and 160-micron light). The blue color mainly traces old stars. The green color traces emission from organic dust grains (mainly polycyclic aromatic hydrocarbons). The red traces emission from larger, cooler dust grains..
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The image was taken as part of the Spitzer Legacy program known as SAGE-SMC: Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud.
This is one segment of an infrared portrait of dust and stars radiating in the inner Milky Way. More than 800,000 frames from NASA's Spitzer Space Telescope were stitched together to create the full image, capturing more than 50 percent of our entire galaxy..
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As inhabitants of a flat galactic disk, Earth and its solar system have an edge-on view of their host galaxy, like looking at a glass dish from its edge. From our perspective, most of the galaxy is condensed into a blurry narrow band of light that stretches completely around the sky, also known as the galactic plane..
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This survey segment spans galactic longitudes of 57.8 to 66.0 degrees and is centered at a galactic latitude of 0 degrees. It covers about two vertical degrees of the galactic plane..
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The swaths of green represent organic molecules, called polycyclic aromatic hydrocarbons, which are illuminated by light from nearby star formation, while the thermal emission, or heat, from warm dust is rendered in red. Star-forming regions appear as swirls of red and yellow, where the warm dust overlaps with the glowing organic molecules. The blue specks sprinkled throughout the photograph are Milky Way stars. .
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The segment spans galactic latitidues of 57.8 to 66.0 degrees and is centered at a galactic longitude of 0 degrees. It covers about two vertical degrees of the galactic plane..
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This is a three-color composite that shows infrared observations from two Spitzer instruments. Blue represents 3.6-micron light and green shows light of 8 microns, both captured by Spitzer's infrared array camera. Red is 24-micron light detected by Spitzer's multiband imaging photometer. This combines observations from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and MIPSGAL projects.
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.
I was stuck for a 40 meter antenna & thought of going with my Buddipole with long whips, this setup is untested for that band in my hands.
After spending too much time experimenting I opted for a multiband end fed sloper instead which was narrow banded but got the job done on both 80/40 & 15 meters.
I'm not done experimenting with the Buddipole on 40 meters though...to be continued!
A graveyard stone
Inv. no.: 91.5.9.
found: Budapest, III. ker., Buda side foot-head of Árpád-bridge (1981)
Female figure with skirt-neck hidden by torques, a broad multiband bracelet on her left wrist. Her gown or shawl fitting close to her neck falls down from the hair which is parted in the middle, then lapping onto her shoulder.
This is my own home station -- an ICOM 7200, tuner, and my favorite keyer and paddle. Windows 7 is running on my mac in a virtual machine, with the N1MM logger software up and active. This station was connected (most of the time) to the 25' alpha-delta multiband dipole.
www.micro-tech-medical.com/products/multiple-band-ligator...
Multiband Ligators
Endoscopic banding has been demonstrated as an effective and simple treatment for internal hemorrhoids. Banding is readily performed in an ambulatory setting and can result in less pain and have a shorter recovery period than surgical hemorrhoidectomy.
The Micro-Tech Hemorrhoids Multiple Band Ligator Set is a cost-effective solution for the outpatient treatment of hemorrhoids during a routine colonoscopy.
KEY BENEFITS
EXCELLENT VISIBILITY
A clear ligating barrel with rear mounted bands optimizes the endoscopic view while maintaining suction.
BAND DESIGN
The square band design provides consistent shape and reliable retention. The set comes with four pre-loaded latex-free bands.
USER-FRIENDLY SYSTEM
The handle unit tie hole enables quick and easy loading of the pull wire. The alert band notifies the operator when only one band remains.
SPECIFICATION
Multiple band ligator set
REFRequired Working Channel (mm)Scope O.D. (mm)Bands/Ligating UnitBand TypePackaging
MBLS-7F-NL2.89.4-13.07pcsLatex Free1/Box
MBLS-6F-NL2.89.4-13.06pcsLatex Free1/Box
MBLS-4F-NL2.89.4-13.04pcsLatex Free1/Box
MBLS-3F-NL2.89.4-13.03pcsLatex Free1/Box
MBLS-7F2.89.4-13.07pcsLatex1/Box
MBLS-6F2.89.4-13.06pcsLatex1/Box
MBLS-4F2.89.4-13.04pcsLatex1/Box
MBLS-3F2.89.4-13.03pcsLatex1/Box
REFRequired Working Channel (mm)Scope O.D. (mm)Bands/Ligating UnitBand TypePackaging
MBLS-XL-7F-NL2.811.0-14.07pcsLatex Free1/Box
MBLS-XL-6F-NL2.811.0-14.06pcsLatex Free1/Box
MBLS-XL-4F-NL2.811.0-14.04pcsLatex Free1/Box
MBLS-XL-3F-NL2.811.0-14.03pcsLatex Free1/Box
MBLS-XL-7F2.811.0-14.07pcsLatex1/Box
MBLS-XL-6F2.811.0-14.06pcsLatex1/Box
MBLS-XL-4F2.811.0-14.04pcsLatex1/Box
MBLS-XL-3F2.811.0-14.03pcsLatex1/Box
The Hosemaster supplies everything from hose assemblies & adaptors to filters, lubricators, spray guns, airline tools & equipment.
Looking like a spider’s web swirled into a spiral, the galaxy IC 342 presents its delicate pattern of dust in this image from NASA’s Spitzer Space Telescope. Seen in infrared light, the faint starlight gives way to the glowing bright patterns of dust found throughout the galaxy’s 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 Spitzer’s 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).
Title
“Witch’s Broom in the Void: NGC 6960 (Western Veil Nebula)”
Description
Beneath the wing of the celestial swan, I captured the ghostly filaments of the Western Veil Nebula (NGC 6960) — a breath of cosmic memory from a star that died thousands of years ago. This delicate lacework of ionized hydrogen and oxygen drifts across space, the remnant of a supernova whose shock-wave, sweeping through the interstellar medium, carved and illuminated the shell we now see.
AstroBackyard
+3
Wikipedia
+3
Sky & Telescope
+3
At an estimated distance of ~2,100–2,400 light-years and spanning roughly 110 light-years across, this structure stretches nearly six moon-diameters across our sky.
NASA Science
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astro.nightsky.at
+2
The bright star 52 Cygni that appears embedded in the nebula is in fact a foreground star, giving us only the illusion of association.
Sky & Telescope
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Captured from the dark desert skies of the Desert Bloom Observatory (Bortle Class 2) on October 19, 20, 23, I used a Celestron NexStar EVO 9.25 f/10 and ZWO ASI2600MC PRO on a Sky-Watcher EQ-6R Pro mount, guided by a ZWO 30F4 Miniscope and ASI462 MC, with a ZWO ASIAir Plus controlling acquisition. A 2″ Optolong L-Pro multiband-pass filter was used to isolate emission detail, and exposures of 600 s each were stacked over 58 subs with DeepSkyStacker, then processed via PixInsight and Photoshop to bring out the fragile filament texture and subtle colour gradients.
The final frame reveals the interplay of glowing hydrogen (H-α) and doubly-ionised oxygen (O III) gas, sculpted by shock-fronts and cosmic currents into gossamer strands. It is a snapshot of stellar death and cosmic rebirth — a lament and a celebration, frozen in light.
May this image be a whisper from the universe: that even in destruction, there is beauty; even in silence, there is story.
It was the first my girlfriend gift for my birthday, I still have it, it is portable multiband receiver.
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.
a sinistra antenna vhf/uhf Diamond X-50, a destra antenna multibanda HF della Hy-Gain
modello AV-14AVQ + kit per gli 80m (MK80)
Questa antenna HF opera sulle bande dei 10, 15, 20, 40 e 80 metri
sotto l'antenna un paio di pinne rosa fucsia :D
This image layout reveals how the appearance of the North America nebula can change dramatically using different combinations of visible and infrared observations from the Digitized Sky Survey and NASA's Spitzer Space Telescope, respectively.
In this progression, the visible-light view (upper left) shows a striking similarity to the North America continent. The image highlights the eastern seaboard and Gulf of Mexico regions. The red region to the right is known as the "Pelican nebula," after its resemblance in visible light to a pelican.
The view at upper right includes both visible and infrared observations. The hot gas comprising the North America continent and the Pelican now takes on a vivid blue hue, while red colors display the infrared light. Inky black dust features start to glow in the infrared view.
In the bottom two images, only infrared light from Spitzer is shown -- data from the infrared array camera is on the left, and data from both the infrared array camera and the multiband imaging photometer, which sees longer wavelengths, is on the right. 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.
Color is used to display different parts of the spectrum in each of these images. In the visible-light view (upper right) from the Digitized Sky Survey, colors are shown in their natural blue and red hues. The combined visible/infrared image (upper left) shows visible light as blue, and infrared light as green and red. The infrared array camera (lower left) represents light with a wavelength of 3.6 microns as blue, 4.5 microns as green, 5.8 microns as orange, and 8.0 microns as red. In the final image, incorporating the multiband imaging photometer data, 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.
Credit: NASA et. al.
136-174/400-480Mhz
WEIERWEI UV-5R The transcevier is a micro-miniature multiband
FM transceiver with extensive receive frequency coverage,
providing local-area two-way amateur communications along with unmatched monitoring capability
To capture this image, I stacked and processed two sets of multiple night sessions; one with RGB data using an LPS quad band filter and the other set with Ha/OIII data using a dual narrowband filter. I used Photoshop to blend the Ha and OIII monochrome images with the RGB image, more details below.
Camera: ZWO ASI2600MC Pro
Telescope/Lens: Askar ACL200
Mount: iOptron GEM28 EC
Filters: SVBony SV220 Dual Narrowband, Antlia Quad Band
Image Scale: 3.88″
FOV: 6.73º
Integration Time: 8hrs Narrowband, 12hrs Multiband
Capture Dates: Jun 22 – Jul 4, 2025
Bortle Scale: Bortle 6, Bright Suburban Sky
Aquisition Software: NINA, PHD2
Processing Software: Siril, Sirilic, GraXpert, Cosmic Clarity and Photoshop.
More info at alexisantonio.com/2025/07/14/sadr-region-and-crescent-neb...