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User: macsaver |
UV-klub Heidelberg - 24.11.2007 Ed Davenport (London, Gumption Recordings) Residents: Eddie Zarook, Casio Casino, Neville Attree, 212fahrenheit Visual Support by treiblicht Tags: Minimal Gumption Recordings Heidelberg UV-klub Eddie Zarook Casio Casino treiblicht Ed Davenport |
User: macsaver |
UV-klub Heidelberg - 24.11.2007 Another UV-klub Video Tags: UV-klub Heidelberg Eddie Zarook Casio Casino treiblicht Neville Attree LoFi Gumption 212fahrenheit |
User: macsaver |
UV-klub Heidelberg - 22.07.07 Eddie Zarook and Casio Casino (aka Steffen Neuert) have been quietly plying their particular brand of minimal house, deep techno, tech house, electronica, acid and electronic trickery at the UV club in Heidelberg for a good, few years now. What struck me on my first visit earlier this year, apart from the unique location, was the extraordinary vibe running through the diverse, expectant crowd -- it's been a long time since i've seen people actually dancing into a club. If you've already heard their debut release on LoFi, then you know what the fuss is about. Haluzengenic and The Gap are two tracks that achieve the difficult task of inducing dancefloor mayhem while remaining credible pieces of sonic exploration. It's a successful fusion that will continue to bare fruit in the future and is no doubt the result of their previous musical incarnations. Steffen's involvement with electronic production didn't start until he arrived in Heidelberg 12 years ago. At the time he was immersed in the indie scene, being far from impressed with the state of German techno. However Dirk Mantei, the owner of his local record store slowly turned him on to the ‚good side' of electronic dance music and the purchase of studio equipment including a (now sadly defunkt) Roland R8 also helped shape a new musical perspective. Since then, collaborations with fellow Heidelberger Lopazz have been a constant feature of his career along with the ground-breaking project Bergheim 34, through which Steffen successfully managed to meld his love of Krautrock and Detroit minimal techno, presenting electronic music in a live band context, long before the more recent, cliched attempts of today's electro clashers. Around the same time, Eddie was starting out on his own musical journey that initially embraced those ‚gods of rock' Led Zep and Hendrix. After relocating to Germany from Iran in 1989, he studied guitar, eventually graduating with flying colours from music school in Cologne. He settled in Heidelberg in 1998 and a year later his growing fascination with electronic music prompted him to start Djing. Typically, the pair first met in the Vinyl Only record store in 1999 where their shared love of techno classics, especially the minimal sound, led to the idea to start producing together. Their energy was such that, almost immediately, the UV club was born and it's a tribute to their belief and enthusiasm that the club is still rocking packed crowds six years later. Steffen (aka Casio Casino) was already playing around the world with his project Bergheim 34 in the U.S.A, with Sad Rockets all over Europe. Eddie Zarook has been rocking clubs from New York to St. Petersburg. But still both of them are playing in Heidelberg: You got to rock the block before you rock the land!!! (written by Neville Attree 2006) Tags: Heidelberg Minimal Techno Club Eddie Zarook Casio Casino 212fahrenheit Neville Attree treiblicht Karlstorbahnh |
User: 8otion8 |
212 / Fahrenheit When the youth group got too large 212 Student Ministries had to seperate the high school and mid school into two different services and this was the video to promote that. Tags: church youth ministry |
User: xxxFAHRENHEIT212xxx |
FAHRENHEIT 212 Oktober 2006 Tags: FAHRENHEIT 212 |
User: adamcoffing |
Fahrenheit Intro Dance (212 Student Ministries) This was a dance that all the team leaders came up with to intro Fahrenheit, our Middle School Service. It was mostly to create hype for the night! Tags: Fahrenheit Dance 212 Student Leaders Intro High School Musical |
User: Antivanilla |
Fahrenheit 212 - Part One Don't judge me people, this was made in sixth grade. And this is the best dam home movie EVER. Tags: Michael Brienza is P.O.E. |
User: Antivanilla |
Fahrenheit 212 - Part 2 Part two. Don't judge me. Unless you love it, then feel free to judge. Tags: Michael Brienza is P.O.E. |
User: 8otion8 |
212 Student Ministries This is just a little promo video advertising the entire 212 Student Ministires, Depth (college), 212 (high school), and Fahrenheit (mid school.) Tags: church youth ministry |
User: MelodyOfVision |
Krakatoa: The Last Days, Clip 6 - Pyroclastic Surge From the BBC docu-drama, "Krakatoa: The Last Days." The movie is also known as "Krakatoa: Volcano of Destruction" and aired on Discovery Channel. The movie brings to life the journals and recollections of four witnesses who survived the cataclysmic eruption of Krakatoa in August of 1883. The Beijerinck (Beyerinck) family, along with 3,000 Ketimbang survivors, had settled further inland. They survived a tsunami and the destructive ear-shattering force of Krakatoa's explosions. They thought the worst had past, but one more is about to strike. A pyroclastic surge is a fluid mass of turbulent gas and rock fragments which is ejected during volcanic eruptions and are similar to pyroclastic flows except that it has a higher proportion of gas to rock particles. Pyroclastic flows can generate pyroclastic surges. Because a pyroclastic surge is "lighter" than a pyroclastic flow, it can travel much faster at speeds of 350 mph carrying massive destructive kinetic energy and can actually climb higher ground. Pyroclastic surges can be "hot" containing gas and steam at temperatures above 100 degrees Celsius (212 degrees Fahrenheit) to as much as 800 degrees Celsius(1472 degrees Fahrenheit). They can also be "cold" with temperatures below 100 degrees Celsius. Aside the temperature factor, both hot and cold pyroclastic surges can still be lethal, depending on the type of gases they carry. Hot pyroclastic surges can cross significant bodies of water on a cushion of superheated steam just as it occurred in the Ketimbang area of Sumatra. If you would like to read Johanna Beijerinck's in-depth account of her family's survival through this volcanic catastrophe, please visit: Survivor Diary -- Johanna Beyerinck http://dsc.discovery.com/convergence/krakatoa/diaries/johanna.html --- Tags: Krakatoa The Last Days Volcano Of Destruction 1883 Pyroclastic Surge Flows BBC Discovery Channel Johanna Beijerinck |
User: inventorr77 |
Boiling Water Without Heat - Vapor Pressure Experiment An eye opening video that shows that water doesn't need to be heated (or even hot) to boil? Sure... we know from science class that water boils at 212 degrees Fahrenheit at sea-level but what about under a vacuum? Watch this. The venturi siphon pump I used can be purchased here: Nalgene* Aspirator Vacuum Pump 09-960-2 from Fisher Scientific. Nalgene Vacuum Pump Polypro S41381 Vendor No.:6140-0010EMD see: https://www.fishersci.com/wps/portal/PRODUCTDETAIL?productId=694608&catalogId=29104&brCategoryId=null&fromCat=yes&fromSearch=null Tags: boiling water vacuum vapor pressure |
User: nightwo1f |
ssc2007-19v1_full This artist's animation begins by showing a dark and dusty corner of space where little visible light can escape. The animation then transitions to an infrared view taken by NASA's Spitzer Space Telescope, revealing an embryonic star with dramatic jets. This infrared portrait gives us a rare look at what our own solar system looked like billions of years ago. Stars form out of spinning clouds, or envelopes, of gas and dust. As the envelopes flatten and collapse, jets of gas stream outward and a swirling disk of planet-forming material takes shape around the forming star. Eventually, the envelope and jets disappear, leaving a newborn star with a suite of planets. This process takes millions of years. The Spitzer image shows a developing sun-like star, called L1157, that is only thousands of years old (for comparison, our solar system is around 4.5 billion years old). Why is the young system only visible in infrared light? The answer has to do with the fact that stars are born in cocoons of dust that block visible light. But the heat, or infrared light, of an object can be detected through the dust. In Spitzer's infrared view of L1157, the star itself is hidden but its envelope is visible in silhouette as a thick black bar. While Spitzer can peer through this region's dust, it cannot penetrate the envelope itself. Hence, the envelope appears black. The thickest part of the envelope can be seen as the black line crossing the giant jets. This L1157 portrait provides the first clear look at stellar envelope that has begun to flatten. The color white shows the hottest parts of the jets, with temperatures around 100 degrees Celsius (212 degrees Fahrenheit). Most of the material in the jets, seen in orange, is roughly zero degrees on the Celsius and Fahrenheit scales. The reddish haze all around the picture is dust. The white dots are other stars, mostly in the background. L1157 is located 800 light-years away in the constellation Cepheus. The Spitzer image was taken by the telescope's infrared array camera. Infrared light of 8 microns is colored red; 4.5-micron infrared light is green; and 3.6-micron infrared light is blue. The visible-light picture is from the Palomar Observatory-Space Telescope Science Institute Digitized Sky Survey. Blue visible light is blue; red visible light is green, and near-infrared light is red. Tags: aviation space |
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