Jin Kazama
Xitizen-X,video tourney T5DR(AUG2K7)
Video2 dari tourney T5DR di Xitizen-X yg bulan Agustus kemaren..
diupload kesini... (baru sebagian)
http://www.youtube.com/profile?user=andymrb


Link dari video2 ini bakal dipost di TZ...
Tapi, kalau loe keberatan videonya loe dipost di TZ,(karena nga pede atau apa gitu.)
please kasih tau disini.....


Nanti gw bakal ngepost video2 nya kayak dulu lagi...

Dulu waktu ngepost link2 nya video tourney @ Kentang's.
gw cuma masukin beberapa video ke playlist.
trus playlistnya itu gw post di TZ...

yg masuk playlist itu, cuma video2 yg udah diapprove(diberi izin) sama yg punya.



btw, ini report tourneynya
http://indotekken.com/forum/showthread.php?t=880


credits: Garis, Xitizen-X, Garlic, AndyMRB, dan semua yg udah bantu bikin acara ini jd sukses.

By Lizanias

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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: July 3, 2004New pictures of Saturn's enigmatic moon Titan, taken by cameras aboard the Cassini probe that are capable of penetrating the thick smog-like haze that blankets the frigid world, show strange looking surface features and a deck of methane clouds the size of Arizona. But so far, the instruments have not detected reflections from the surfaces of lakes or small seas of liquid hydrocarbons many scientists believe must form in the ultra-cold environment. Piercing the ubiquitous layer of smog enshrouding Titan, this combination of images from the Cassini visual and infrared mapping spectrometer reveals an exotic surface covered with a variety of materials in the southern hemisphere. Image: NASA/JPL/University of Arizona.But like the sun glint off rivers and lakes visible from airplanes on Earth, the reflections in question can only be seen in a small region of Titan, about 1 percent of the visible surface, based on the relative positions of the sun and Cassini."If we go by 30 times and we haven't seen it, we're going to start getting worried," said Kevin Baines, a member of Cassini's Visual Infrared Mapping Spectrometer team. "But I'd say so far, just going by once, it may have been that the specular reflection point was a continent, a dry area."So the planet could have plenty of liquids and we just got faked out. We don't know," he said in a telephone interview. "It's just 1 percent of the planet, we shouldn't reach any conclusions from that."Cassini's first flyby of Titan, the day after the craft braked into orbit around the ringed planet, was at a distance of more than 200,000 miles. In October, the nuclear-powered probe will pass within just 745 miles of Titan and "we really expect to get a great view then," said Elizabeth Turtle, a member of the Cassini imaging team. A mosaic of Titan's south polar region acquired as Cassini passed by at a range of 339,000 kilometers (210,600 miles) on July 2. These images were acquired through special filters designed to see through the thick haze and atmosphere. The surface features become more blurry toward the limb, where the light reflected off the surface must pass through more atmosphere before reaching the camera. The bright spots near the bottom represent a field of clouds near the south pole. Image: NASA/JPL/Space Science Institute.In the meantime, "I can't tell you how excited I am to be able to show you the images we've got of Titan," she said at a news conference today. "These are just spectacular. It's our first good look at Titan and Titan hasn't disappointed us. It's different from anything we've ever seen before."Using filters to look through specific spectral "windows" in the hazy atmosphere, "we're seeing surface features as small as 10 to 20 kilometers (six to 12 miles) across," Turtle said. "This is 10 times better than what we saw during approach. It's a huge improvement."A mosaic made up of the best pictures from Cassini's long-distance flyby show a broad region of Titan's surface stretching from just above its equator to the moon's south pole. A large dark feature vaguely resembling the letter H on its side was visible at the top of the mosaic. The equatorial zones below were dominated by brighter areas while a large deck of clouds was prominent near the south pole.Drifting some nine miles up in Titan's thick nitrogen atmosphere, the clouds clearly moved and changed shape in pictures shot over a five-hour period."These are dynamical clouds and a meteorologically interesting part of the planet where storms might be happening," said Baines. "There's speculation that it may even be associated with a feature on the ground, so we may have some wind motion lifting up air, methane moisture-laden air, to the point where it can condense out and form clouds."Titan's atmosphere is made up primarily of nitrogen with small levels of methane and molecular hydrogen. Nitrogen and methane combine in the atmosphere but the action of sunlight, even at Saturn's distance, causes the compounds to disassociate and hydrocarbons fall to the surface.Based on a variety of lines of evidence, including a surface temperatures as low as -292 degrees Fahrenheit, scientists believe those hydrocarbons must exist in liquid form, as lakes or large pools. It's also possible Titan is more like a giant sponge, with liquids filling cavities in the materials making up its surface. Shown here is a blowup of a region of Titan imaged on July 2, 2004. This image was taken at a distance of 339,000 kilometers (210,600 miles) and shows brightness variations on the surface of Titan and a bright field of clouds near the south pole. The field of clouds is 450 kilometers (280 miles) across and is the about the size of Arizona. Features as small as 10 kilometers (6 miles) can be discern. Image: NASA/JPL/Space Science InstituteBased on Cassini's initial, long-distance flyby, the questions remain open. But scientists were nonetheless disappointed not to catch that tell-tale glint on the mission's first try."The simulations I've done indicate that if the surface liquid is calm and not roughed up a lot by waves, it would be enormously bright, it would be the brightest thing we would see on Titan," said Bob West, a scientist at the Jet Propulsion Laboratory in Pasadena, Calif. "The calculations also show you can have quite a bit of overlying haze and even with a rough surface, I would have expected to see it by now. And we haven't."Even so, Turtle was elated at what the pictures did show."It's dangerous to start interpreting a brand new surface that we've never seen before, especially on so little sleep," she said. "But we can't really resist. We're seeing surface brightness variations, we're not seeing topographic shading, the same way you would on a cloudy day on Earth, you don't see shadows or anything like that."What we're seeing is just variations in the brightness of the surface. We see some surface features that are circular, others are linear. There are some features that look like they're rather concentric to near the south pole. ... And the sense that we're not just seeing circular blobs all over the place suggests it's not just a heavily cratered body, that there has been geologic activity on Titan."Now, it's anyone's guess as to what that has been, there are quite a lot of candidates, But from these images, we can't say what the geologic activity has been."She said the apparent fuzziness of the surface could be the result of overlying haze, but "we are seeing some fairly fine detail as well."Perhaps not surprisingly, the Cassini data already has forced scientists to change their thinking about the processes going on at the surface."It had been hypothesized that the dark materials on Titan are hydrocarbons that have fallen out of the atmosphere," Turtle said. "There's a lot of methane in the atmosphere and that gets processed and it falls out onto the surface in simple and complex hydrocarbons. It's been hypothesized that the dark areas were regions where that material had accumulated and that the bright areas might actually be cleaner water-ice regions that were perhaps even swept clean by methane rain coming out of the atmosphere."That was the theory until Friday night. Data from the infrared mapping spectrometer, Baines said, indicates "the brighter areas are mixtures of water ice but there's a mixture of other things in it which contributes to the brightness. So we think there are organics that contribute to that brightness. The brighter areas have been contaminated in a sense with organics, the dark areas are more pure water ice."Stay tuned.In other news, Don Gurnett, principal investigator with Cassini's Radio and Plasma Wave Science experiment, played a recording of particles slamming into the spacecraft as it passed through the plane of Saturn's rings.Moving at some 53,000 mph, Cassini crossed the plane between the F and G rings, a region thought to be devoid of large particles that could cause any serious damage. Playing it safe, the spacecraft was oriented with its big dish antenna facing forward to act as a shield.As it turned out, that was probably a good idea. Gurnett said his instrument recorded 680 impacts per second, some 100,000 in all, during the ascending ring plane crossing and a similar number on the other side of Saturn as Cassini flew back down through the plane.The average size of the particles was on the order of a thousandth of a millimeter, about the size of smoke particles. But some were possibly as large as a tenth of a millimeter."When one of these particles comes in and hits the spacecraft, it essentially makes a little explosion," Gurnett said. "Hopefully the particle's not too big so it would go through the spacecraft. ... When that explosion occurs, there's a little puff of gas that's produced, part of it is spacecraft material and part of it the particle. And it's heated to like a hundred thousand degrees. And this puff of gas, which is ionized, when it expands over our (instrument) antenna, some of the charge is collected on the antenna and it makes a voltage pulse."He then played a recording of the impact data, converted into an audio file, which sounded like heavy rain hitting Cassini as it plowed through the ring plane."I would say it was a good thing to have (Cassini's dish) antenna pointed into the direction the particles were arriving," he said. "That was a good move."Additional coverage for subscribers:VIDEO:WATCH SATURDAY'S NEWS CONFERENCE ON TITAN PICTURES VIDEO:WATCH FRIDAY'S SCIENCE NEWS CONFERENCE VIDEO:THURSDAY'S NEWS BRIEFING ON CASSINI'S FIRST PICTURES VIDEO:RING PICTURES ARE PRESENTED WITH EXPERT NARRATION VIDEO:CASSINI RE-DISCOVERS TINY MOONS ATLAS AND PAN VIDEO:CASSINI BOOMING SOUNDS FROM BOW-SHOCK CROSSING VIDEO:CASSINI BEGINS ENGINE FIRING TO ENTER ORBIT VIDEO:BURN ENDS SUCCESSFULLY TO PUT CASSINI IN ORBIT VIDEO:POST-ARRIVAL NEWS CONFERENCE VIDEO:WEDNESDAY'S 12 P.M. EDT CASSINI STATUS BRIEFING VIDEO:A LOOK AT INTERNATIONAL COOPERATION VIDEO:'RING-SIDE CHAT' ABOUT SPACE EXPLORATION VIDEO:AN OVERVIEW OF CASSINI'S RADIO SCIENCE VIDEO:TUESDAY'S CASSINI MISSION OVERVIEW BRIEFING VIDEO:CASSINI'S ARRIVAL AT SATURN EXPLAINED VIDEO:SCIENCE OBJECTIVES FOR CASSINI ORBITER VIDEO:HUYGENS LANDER SCIENCE OBJECTIVES Mars rover collectible patchFree shipping to U.S. addresses!This commemorative patch celebrates NASA's Curiosity rover mission of the Mars Science Laboratory in search of clues whether the Red Planet was once hospitable to life.Gemini 7Gemini 7: The NASA Mission Reports covers this 14-day mission by Borman and Lovell as they demonstrated some of the more essential facts of space flight. Includes CD-ROM.Choose your store: - - - Apollo patchesThe Apollo Patch Collection: Includes all 12 Apollo mission patches plus the Apollo Program Patch. Save over 20% off the Individual price.Choose your store: - - - Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is available from our online.Choose your store: - - - Apollo 9 DVDOn the road to the moon, the mission of Apollo 9 stands as an important gateway in experience and procedures. This 2-DVD collection presents the crucial mission on the voyage to the moon. Choose your store: - - - Gemini 7Gemini 7: The NASA Mission Reports covers this 14-day mission by Borman and Lovell as they demonstrated some of the more essential facts of space flight. Includes CD-ROM.Choose your store: - - - Apollo patchesThe Apollo Patch Collection: Includes all 12 Apollo mission patches plus the Apollo Program Patch. Save over 20% off the Individual price.Choose your store: - - - Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is available from our online.Choose your store: - - - Apollo 9 DVDOn the road to the moon, the mission of Apollo 9 stands as an important gateway in experience and procedures. This 2-DVD collection presents the crucial mission on the voyage to the moon. Choose your store: - - - Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Cassini radar sees flow-like feature across Titan UNIVERSITY OF ARIZONA NEWS RELEASEPosted: November 8, 2004A strikingly bright, lobate feature has turned up in one of Cassini's first radar images of Saturn's moon Titan."It may be something that flowed," Cassini radar team member Ralph Lorenz of the University of Arizona said. "Or it could be something carved by erosion. It's too early to say."But it looks very much like it's something that oozed across the surface.It may be some sort of 'cryovolcanic' flow, an analog to volcanism on Earththat is not molten rock but, at Titan's very cold temperatures, molten ice." This is a synthetic aperture radar image of Titan. Dark regions may represent areas that are smooth, made of radar-absorbing materials, or are sloped away from the direction of illumination. A striking lobate bright feature stretches from upper left to lower right across this image, with connected 'arms' to the east. The fact that the lower (southern) edges of the features are brighter is consistent with the lobate structure being raised above the relatively featureless darker background. Credit: NASA/JPLCassini radar mapped about one percent of Titan's surface during theCassini spacecraft's first close Titan flyby Oct. 26. The radar surveycovered a strip 75 miles wide (120 kilometers) and 1,200 miles (1,960kilometers) long in Titan's northern hemisphere.Cassini was flying about 1,550 miles (2,494 kilometers) above Titan'ssurface, with its radar centered at about 45 degrees north, 30 degreeswest, when it mapped the 90-square-mile (230-square-kilometer) area shownin the new radar image.The Cassini radar team presented the image today at the 86th annual meetingof the American Astronomical Society Division of Planetary Sciences inLouisville, Ky.The radar instrument works by bouncing radio signals off Titan's surfaceand timing their return. The more signal reflected back to thespacecraft, the brighter the imaged area. Turning radio signals intoradar images is time consuming because so many numerical calculations mustbe made. "There's no such thing as a 'raw' radar image," Lorenz said.But two days after the Oct. 26 flyby, Cassini scientists knew that Titan isno impact-crater-pocked dead world, but a much more interesting place.Titan's surface is young -- it's been shaped by dynamic geologicprocessing, Lorenz, Cassini interdisciplinary scientist Jonathan Lunine ofthe University of Arizona, and other Cassini scientists agree.Given this newest image, Lunine said, "Radar has provided the firstevidence for possible young cryovolcanism on Titan's surface. Now ourchallenge is to find out what is flowing, how it works, and theimplications for Titan's evolution."The Cassini-Huygens mission is a cooperative project of NASA, the EuropeanSpace Agency and the Italian Space Agency. The Jet Propulsion Laboratory, adivision of the California Institute of Technology in Pasadena, manages theCassini-Huygens mission for NASA's Science Mission Directorate, Washington,D.C. The Cassini orbiter and its two onboard cameras were designed,developed and assembled at JPL. The radar instrument team is based at JPL,working with team members from the United States and several Europeancountries.Cassini posterJust in time for the Cassini spacecraft's arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12x12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is now available from the Astronomy Now Store.Columbia ReportThe official accident investigation report into the loss of the space shuttle Columbia and its crew of seven. Includes CD-ROM. Choose your store: | | | | 2014 Spaceflight Now Inc.Cassini radar shows diversity on Saturn's moon Titan CASSINI PHOTO RELEASEPosted: October 28, 2004 Credit: NASA/JPLDownload larger image version This radar image of the surface of Saturn's moon Titan was acquired on October 26, 2004, when the Cassini spacecraft flew approximately 1,200 kilometers (745 miles) above the surface and acquired radar data for the first time. It reveals a complex geologic surface thought to be composed of icy materials and hydrocarbons. A wide variety of geologic terrain types can be seen on the image; brighter areas may correspond to rougher terrains and darker areas are thought to be smoother. A large dark circular feature is seen at the western (left) end of the image, but very few features resembling fresh impact craters are seen. This suggests that the surface is relatively young. Enigmatic sinuous bright linear features are visible, mainly cutting across dark areas. The image is about 150 kilometers (93 miles) wide and 250 kilometers (155 miles) long, and is centered at 50 N, 82 W in the northern hemisphere of Titan, over a region that has not yet been imaged optically. The smallest details seen on the image are about 300 meters (186 miles) across. The data were acquired in the synthetic aperture radar mode of Cassini's radar instrument. In this mode, radio signals are bounced off the surface of Titan. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The instrument team is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. Cassini posterJust in time for the Cassini spacecraft's arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12x12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is now available from the Astronomy Now Store.Columbia ReportThe official accident investigation report into the loss of the space shuttle Columbia and its crew of seven. Includes CD-ROM. Choose your store: | | | | 2014 Spaceflight Now Inc.Cassini sails to Saturn 'Flagship mission of our time' BY WILLIAM HARWOOD
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