View allAll Photos Tagged multiband
This pirate tin houses a 1:1 ferrite balun and feeds a trap multiband dipole antenna in my living room / hallway
Edited Spitzer Space Telescope image of the stars Cepheus C and Cepheus B. Color/processing variant.
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.
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.
OK, lemme talk a little about yet another chapter in my continuing education concerning things I apparently decided not to appreciate until I was past 50.
So this is a clone of the Demeter Compulator optical compressor.
I've owned a couple of compressors over the years and have never really been a fan. I had a TC Electronic Sustain+Parametric Equalizer pedal for decades. I mainly used it as an EQ to drive a little growl-y peak into my amp, but the compressor part of the pedal was usually annoying to me. It seemed to suck a lot of the life out of anything I played and you could hear it bringing up the level as stuff decayed. I also had a Scholz Sustainor for years and never really cared much for the compressor in that thing, either, although it wasn't as annoying as the TC box. I also use the Multipressor software multiband compressor for computer remaster-y stuff, which I've done with old live recordings. That thing is magic. You can target ranges and completely change the overall tonal balance of a mix without resorting to EQ. It's probably my favorite plugin. I even ran Jean-Luc Ponty's, 'Egocentric Molucules' through it because I've always hated the mix. I was able to make that track SO much better in so little time that it seemed like some kind of voodoo.
Anyway, I decided I'd try an optical compressor. Right out of the gate, the thing was breaking up when I'd bang out a chord. It has an internal trimmer, though, so you can adapt it to various instruments. I had to turn that trimmer almost all the way down to use my Junior without getting distortion, so my guess is that this box was designed for Strat players. Either that, or guys with humbuckers just don't cotton to no squishee-squeezy bidness. In any case, by the time I had it working properly I was all ready to hate it.
Except it's really transparent. It's kind of like you aren't running an effect at all, except at the same time it's like I'm just freakin' awesome. Havin' one of those good nights where everything rings out like I want it to and my technique is better than normal.
I'm not experienced enough to know better at this point, but I feel like I could leave this thing on all the time. I wonder if there's some kind of Compressors Anonymous for people who won't shut these things off?
So...uh...cool.
BTW, you can see how it's set. The left knob is set for unity gain, which was pretty high, IMO. Not much more travel there if I'd wanted to boost things a little. The right knob is compression and that seems pretty awesome just a little to the left of noon. I'm just learning to hear what this thing does, so that may be high and I'm just not hearing anything ugly because my ears are still learning its wicked ways, but that sounds pretty awesome to me right now.
Sgt. Raymond Walters, 1437thEngineer company, Sault Saint Marie, Mich., Michigan Army National Guard, demonstrates to AN/PRC-152 Multiband Handheld Radio to members of the Latvian Engineer Battalion ( ZS 54 ITBN), in Orge, Latvia, Sept. 28, 2014. The Michigan Army National Guard is training the Latvian Engineers on their equipment, while, in turn the Latvians train the Michigan soldiers on theirs. The Michigan and Latvian Engineers are training together in support of Operation Silver Arrow, in conjunction with United States Army Europe and Operation Northern Resolve. (U.S. Army photo by Sgt. 1st Class Helen Miller, Michigan National Guard/released)
Generations of stars can be seen in this new infrared portrait from NASA's Spitzer Space Telescope. In this wispy star-forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant-trunk-like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds.
W5 spans an area of sky equivalent to four full moons and is about 6,500 light-years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours.
Like other massive star-forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star-formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars.
This image contains some of the best evidence yet for the triggered star-formation theory. Scientists analyzing the photo have been able to show that the ages of the stars become progressively and systematically younger with distance from the center of the cavities.
This is a three-color composite showing 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.
Born of Darkness: Orion’s Fire in a Sky That Still Knows Night
Captured beneath the stillness of the Desert Bloom Observatory, where the sky rests at Bortle 2 and deepens toward near-Bortle 1 after midnight, this portrait of the Orion Nebula (M42) reveals what the universe shares only when darkness is allowed to remain unbroken. Across 161 exposures of 600 seconds, taken over 14 sleepless nights, 110 hours of ancient photons gathered here — each one a fragment of a star’s beginning.
Through a carefully tuned imaging system — the Celestron NexStar Evolution 9.25” Schmidt-Cassegrain with HyperStar, the ZWO ASI2600MC Pro, ZWO guiding optics, and the Sky-Watcher EQ-6R — every photon was captured with precision. In processing, the stars were shaped with restraint, preventing bloat and preserving their natural presence in the field. The nebula itself was handled with gentle care, allowing its filaments, dust lanes, and ionized fronts to unfold exactly as the light intended.
From this treatment, M42 emerges in a gentle pink-rose hue, the natural expression of hydrogen emission through a broadband L-Pro filter. Soft teal accents from oxygen slip between the clouds, revealing the dynamic physics at work: gravitational collapse forming new suns, ultraviolet radiation carving glowing hollows in the dust, and stellar winds sculpting shapes that will one day cradle forming worlds.
More than an image, this is a reminder of the fragile gift of darkness. Only under protected night skies can the universe reveal its deepest truths. When we defend the night from artificial light, we preserve not just beauty — but humanity’s ability to wonder, to learn, and to trace our origins to the stars themselves.
Technical Summary
Object: M42 — The Orion Nebula
Constellation: Orion
Distance: ~1,344 light-years
Total Integration: 110 hours (161 × 600s)
Processing Pipeline: DeepSkyStacker → PixInsight → Photoshop
Location: Desert Bloom Observatory — Bortle 2 sky, approaching near-Bortle 1 after midnight
Equipment Used:
• Celestron NexStar Evolution 9.25" SCT (235mm f/10)
• Starizona HyperStar 4
• ZWO ASI2600MC Pro
• Sky-Watcher EQ-6R Pro Mount
• ZWO 30F4 MiniScope (Guide Scope)
• ZWO ASI462MC (Guide Camera)
• Optolong L-Pro 2" Multiband Filter
• ZWO Electronic Automatic Focuser (EAF)
• ZWO ASIAir Plus Controller
• Starizona Telrad Reflex Sight
• Astrozap Dew Heater
• Celestron Dew Shield
• Samsung Phone
• Memory Card
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.
Faja sacrolumbar semirrígida en material transpirable multibanda con dos bandas elásticas tensoras cruzadas en la parte trasera que abrochan en el delantero, ballenas verticales en la espalda y cierre velcro delantero. Incorpora una bolsa de tela en la zona lumbar para poder insertar una placa intercambiable de material termomoldeable a baja temperatura. Fuerte apoyo y contención lumbar. Transpirable y muy cómoda de usar. Lumbalgias, procesos degenerativos, debilidad y atonía muscular, hernias discales, postoperatorio.
Para más información: www.exclusivasiglesias.com/es/product/ortesis-tronco/faja...
Soundblox® Pro Multiwave Bass Distortion
Il Soundblox Pro Multiwave Bass Distortion eredita le potenza e la chiarezza dell'originale Soundblox Multiwave Distortion ma con algoritmi che si addicono alla gamma di frequenze del basso elettrico. I bassisti combinano accordi complessi e intervalli con toni distorti - Il processo multi banda elimina l'impasto delle note e fa si che ognuna esca pulita e fedele. Il pedale ha anche la possibilità di avere il processo singola banda per avere suoni distorti più tradizionali. E' il pedale perfetto sia in studio che sul palco.
Il musicista ha accesso a 23 tipi di distorsione, attuali e distinti, con un modalità clean boost/EQ. I tipi di curve di distorsione vanno dal "normale" overdrive per suoni classici fino al "foldback" e "octave" per suoni più aggressivi simili a tonalità synth. Ogni tipo di distorsione può essere personalizzata tramite I'equalizzatore a 7 bande, il controllo Drive e controlli di livello separati per segnali puliti e distorti. Questi avanzati controlli di suono attenuano la tendenza alla riduzione delle basse frequenze tipica di molte unita di distorsori per basso.
Sei impostazioni predefinite dall'utente, accessibili tramite tre footswitch, aiutano a richiamare in velocità ogni nuovo suono creato e l'uso di pedale di espressione rende più morbido il passaggio da un preset all'altro. Un ingresso MIDI permette l' accesso ai preset e ai parametri tramite un MIDI controller esterno, e, come tutta la produzione Soundblox, il pedale 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™ 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).
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Distribuito in Italia da Reference Laboratory s.r.l.
The magnificent spiral arms of the nearby galaxy Messier 81 are highlighted in this image from NASA's Spitzer Space Telescope. Located in the northern constellation of Ursa Major (which also includes the Big Dipper), this galaxy is easily visible through binoculars or a small telescope. M81 is located at a distance of 12 million light-years.
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, bottom left inset) is combined with camera data at 8.0 microns (green, bottom center inset) and 3.6 microns (blue, bottom right inset).
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. Dust in the galaxy is bathed by ultraviolet and visible light from nearby stars. Upon absorbing an ultraviolet or visible-light photon, a dust grain is heated and re-emits the energy at longer infrared wavelengths. The dust particles are composed of silicates (chemically similar to beach sand), carbonaceous grains and polycyclic aromatic hydrocarbons and trace the gas distribution in the galaxy. The well-mixed gas (which is best detected at radio wavelengths) and dust provide a reservoir of raw materials for future star formation.
The 24-micron multiband imaging photometer data (red) shows emission from warm dust heated by the most luminous young stars. The infrared-bright clumpy knots within the spiral arms show where massive stars are being born in giant H II (ionized hydrogen) regions. Studying the locations of these star forming regions with respect to the overall mass distribution and other constituents of the galaxy (e.g., gas) will help identify the conditions and processes needed for star formation.
Edited Spitzer Space Telescope image of the stars Cepheus C and Cepheus B. Inverted grayscale variant.
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.
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.
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
A Soldier assigned to the 3rd Infantry Brigade Combat Team, 25th Infantry Division checks a Manpack radio for an exercise on Aug. 22. The TSM waveform enables multiband and multimode operations. (Photo by Kathryn Bailey, PEO C3T)
Signal University students at Iron Horse University, Fort Carson, CO, receive training on the AN/PSC-5 Multiband Radio. Located at 11 installations inside and outside the United States, Signal University has instructors and training teams who deliver C4ISR training. Its curriculum helps Soldiers prepare for company- and battalion-level field training exercises and obtain specific MOS training. (U.S. Army photo)
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..
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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..
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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..
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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..
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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.
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
via WordPress bit.ly/2DapR1J
Subshock and Evangelos are the curators behind this melodically dynamic psy trance and bass house infused banger. They reworked the song together for Juicy M and the outcome is truly fantastic. Encompassing some serious house vibes and hardcore rhythm, the track coincidentally titled “Psyhaus” was recently released on Spinnin Records. Undoubtably the largest house record label in the world, this is a big release for any artist big or small. No stranger to this genre these two are more so spearheading the bass house style with innovation and ensuring that they keep it fresh as a duo.
The artists sat down to answer some questions over the phone which was a neat experience and a pleasure to get a deeper insight on their story.
How did it feel to get your release signed to Spinnin’ Records?
Evangelos: It felt so good to know that after working hard in that tune for months, tested out so many times and did millions of tweaks to get the perfect mixdown it got signed by the biggest label in the EDM industry. We are also very happy to see the good reactions to this release, we feel like it’s really something fresh!
You’ve been signed to many labels, including Dim Mak, MixMash, and other labels in partnership with Warner Bros. – what advice would you give to producers aiming to get on established labels?
Subshock: Well, we always advice to be patient, work hard and be humble and eventually it will happen, you only need to get noticed by working hard every day. A lot of people says that it is all about connections, which it is true, but not everybody is born having those connections. You need to go out there and network like hell. And of course, it was a matter of working hard on our craft and keep grinding every day and at last, never give up. It took us years for our debut release on Spinnin’ and it definitely didn’t happen overnight!
How did the idea for “JUICY M VS. SUBSHOCK AND EVANGELOS – PSYHAUS” come about?
Evangelos: There is not a really big history here, we are just big fans of Psytrance and Bass House, we play both styles in our shows and we decided to risk a little bit and mix them together. To breakthrough as an artist, we think you should be a bit innovative and just release crazy stuff. This new blend can work really well for our performances and we can’t wait to play it out again. We got some more cooking up as we speak, this year we’ll have lots of music out there, we want to release one track every month like last year!
Did the two of you had solo careers before linking up to form the duo?
Subshock: I started as solo act making dubstep and drum step, under those days I used to release on labels like Excision’s Rottun Records or Dieselboy’s Subhuman and gaining support from big Bass names that helped me tour Europe and North America.
Evangelos: I first started with a partner in a formation called Noiserippers making Dubstep, it was a good time. After some time, we parted ways and went solo under the name Evangelos where I started producing Progressive House. Later I came back to Bass as it satisfies me much more to produce it. When I started I was resident to Zoologico in Madrid, it was the center of Bass/EDM in Spain, that’s where I met Subshock and after doing some b2b sets and doing a couple of tracks we decided to keep going together. Our first collab was “Rebound” and it did really well in Spain, that’s how we knew we were good working together!
Will you be touring in 2019? What have been some of your favorite memories when performing at live events?
Subshock: Yeah of course we will be touring, we are already preparing our second tour around China and getting set some other shows around the globe. We also love to play more in the east part of Europe, people go crazy there!
Well, it always creates really good memories to spend time doing what you love with one of your best buddies you know? But it is also special to see how people are reacting when we play PSYHAUS, they don’t expect the Psytrance part and their faces when it switches is priceless.
Evangelos: Not long ago we were in China and to appear on stage we had to wait for a screen to open and we had to go through it, our intro was playing and people were going crazy, and as we were on stage, Subshock took the pendrive out thinking it belonged to the previous DJ and the music went dead! Now we laugh but at the moment we wanted to dissapear!
What techniques do each of you use to help boost creativity in the studio?
Subshock: We actually started to be a duo also because our workflow in the studio was quite similar but also complementary at the same time, but there is not really a technique. Maybe we could say that the best technique is to combine a lot of hours in the studio with some free time out of it enjoying life with friends and family.
Evangelos: Don’t be afraid to use lots of distorsion, use the buses to mix and control the overall track, be original and take breaks every 3 hours! Oh yeah, and use multiband compression! Also try to do original tracks, experiment and find your own sound. It someone listens to your track and recognizes it as your sound, you are on the right track.
What goals or plans do you have that you guys would like to share for 2019?
Subshock: I think that our main goal for the 2019 is to finally do a tour over the USA but also keep working, risking and give love and fun to those who follow and support us.
Evangelos: We’ve been working hard over 2018 to find our sound and we think we found it, Bass House lets us try lots of things with powerful sounds we love and let us experiment with different BPMs. Before doing a 150 BPMs PSYHAUS track we released a couple of Bass House tracks with the same BPMs and people loved them so we thought it was a good idea to keep the BPMs and give it a twist, expect more like that!
Be sure to follow Subshock and Evangelos if you like their new track Psyhaus!
This article was first published on Your EDM. Source: Juicy M vs. Subshock & Evangelos – Psyhaus [Spinnin Records] [Interview]
Juicy M vs. Subshock & Evangelos – Psyhaus [Spinnin Records] [Interview] published first on soundwizreview.tumblr.com/
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)
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Distribuito in Italia da Reference Laboratory s.r.l.
That's grams, obviously. The spec sheet says 65g, but I did remove a couple of links to size the bracelet.
Really comfortable to wear, this.
[jbm-20250331-q3-022]
Edited Spitzer Space Telescope image of the region around Rho Ophiuchi, showing lots of nebulae and stars.
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.
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
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)
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)