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Porsche Panamera 2010


Saturday, April 11, 2009

Porsche Panamera 2010



The Porsche Panamera is a four-door, four-seat luxury sedan, set to be launched in 2009. It will be front-engined and rear wheel drive, with four-wheel drive available on top versions.
At launch, the Panamera will have three engine choices - a 3.6 L V6 found in the 2008 facelifted Cayenne with 300 hp (224 kW; 304 PS) in the base Panamera, a 4.8 L V8 with 405 hp (302 kW; 411 PS) in the Panamera S and Panamera 4S], and a turbocharged 4.8 L V8 with approximately 500 hp (373 kW; 507 PS) in the Panamera Turbo. There is even a hybrid version in the pipeline. Rumors suggest that the V-10 engine from Porsche's limited-run Carrera GT supercar may be offered as well, although this is still extremely unlikely given the expense of manufacturing the engine and that Porsche does not currently have a facility capable of producing a suitable number of the V-10 engines per year. It is also rumored that the V-12 diesel from the Audi Q7 may be used in the Panamera. US models include engine start/stop system. Turbo version includes active aerodynamics with a multi-stage, adjustable rear spoiler. The Panamera is being marketed as a sedan, however this is technically inaccurate. It is in fact a five-door hatchback, complete with a wide-opening rear liftgate and more trunkroom than a typical sedan. Hatchbacks, especially in America, are considered down-market, so Porsche has chosen to use the term sedan to better compete with true sedans such as the Mercedes-Benz S-Class and the Maserati Quattroporte. While the hatchback design adds greater utility through more cargo room, it has led to criticism that car is ugly and has an oversized rear end. Transmission European models use 6-speed manual gearbox on the rear-drive, normally aspirated model. All US models, as well as all-wheel drive and turbo models, use 7-speed PDK transmission. Handling Porsche Traction Management includes fully-controlled all-wheel drive. PTM is standard on both the Panamera 4S and the Panamera Turbo. Optional Sports Chrono Packages includes a Sport Plus button, which includes tighter damping and air springs and drops the car body by 25 mm (0.98 in). The final assembly of the vehicles will take place in Leipzig. Engines will be assembled in Stuttgart, and the car's painted body will come from the Volkswagen facility in Hannover. The Panamera is generally considered to be the long-awaited fruit of their 989 concept from the late 1980s; some argue that it also presents itself as a successor to the 2-doored 928, but there may be plans to develop a new 928 too. It will be marketed as a direct competitor to automobiles such as the Mercedes-Benz CLS63 AMG, Aston Martin Rapide, Lamborghini Estoque and Maserati Quattroporte and (to a lesser degree) a less expensive alternative to vehicles such as the Bentley Continental GT and Ferrari 612 Scaglietti.It will be produced in the new plant at Leipzig alongside the Cayenne. The vehicle has been caught testing at the Nürburgring and the original sketches are a little more sleek than the taped up model spied testing. Artist renderings of the car already distributed by Porsche show a low-slung, four-door sports car with narrow side windows and flowing lines. However spy shots of the Porsche Panamera testing at the Nürburgring show a more blunt car than the artists renderings. Recent artist impressions paint a car with a very similar front to the 911 and Boxster. At a topping out ceremony at the Leipzig Production Plant, Porsche announced the expansion of their Leipzig plant to include a Panamera production facility. The new facility will measure 25,000 square meters, plus a logistics center with an area of 23,500 square meters. The exterior of the assembly building will be ready by September 2007 making way for the installation of the assembly equipment for the new model series. Porsche will also unveil its second generation hybrid powertrain for the Cayenne and Panamera families around this time. 2008 will see the first assembly of the Panamera line. Production is to start in April 2009, one month after its debut in the Shanghai Motor Show in China. Porsche will keep production rate at around 20,000 cars per year.

Saturday, October 4, 2008

Nokia's Touchscreen 5800 XpressMusic



Armed with a roomy touch display, stereo speakers, and—eventually—a year's worth of free music, Nokia's long-awaited touchscreen phone (formerly known as "The Tube") will make its debut in London today. Can it compete with the iPhone and T-Mobile's Google-powered G1?
First, let's cover the specs: Measuring 4.4 by 2 by 0.6 inches, the 3G- and Wi-Fi-enabled 5800 (set for global release by the end of the year, but not in North America until the "early part" of 2009) is more or less the same size as the iPhone 3G and the G1, although at 3.8 ounces, it's significantly lighter than both of its touchscreen competitors (the iPhone is about 4.8 ounces, while the G1 weighs in at a hefty 5.6 ounces).So, how's the 5800's 3.2-inch touchscreeen? I haven't had a chance to try it in person, but the Symbian-powered display looks (from the press images, at least) reasonably sleek—somewhere between the clunkier interface on the G1 and the iPhone's eye-popping UI. No multitouch (so no "pinch"-type gestures), mind you, but the 5800 has an accelerometer that lets you turn the phone sideways for a virtual, landscape-oriented QWERTY keypad. You'll also be able to enter text using a half-size, portrait QWERTY keypad (with a stylus, if you like), T9 text prediction, or handwriting recognition.
Nokia promises a couple of key one-touch interface features, including a "Contacts Bar" that gives you quick access to your "favorite" four contacts, along with a "Media Bar" that'll let you tap into your music, videos, and images. Not bad, although I'd also like to see a status/alerts toolbar like the G1's.




As its name implies, the 5800 XpressMusic is more about tunes than productivity, so don't expect out-of-the-box support for BlackBerry or Exchange servers (although this being a Symbian phone, there's nothing stopping third parties from filling the void). Instead, the 5800 comes with stereo speakers, support for stereo Bluetooth headsets, a 3.5mm headset jack (which doubles as a TV-out port), and up to 16GB of microSD memeory expansion for your tunes.The 5800 will also support Nokia's much-touted "Comes with Music" service, which will let you download all the free tunes you can stand—but just for 12 months, with a helping of DRM on the side. (CNET has details on all the restrictions right here.) Also, keep in mind that the cost of all those "free" tunes will be passed along via an inflated price tag for upcoming "Comes with Music" handsets (the Nokia N95 and 5310 XpressMusic phones will also be getting "Comes with Music" support), although Nokia reps didn't have details on how big the surcharge will be. Still, the music catalog looks to be pretty solid, with all four of the major labels (as well as some indies) signed on.
Back to the 5800 itself: The phone also comes with a 3.2MP camera, complete with Carl Zeiss optics, a dual LED flash, and video recording (up to 30fps). GPS and Nokia Maps are included for navigation. Sorry, gamers—no N-Gage support on the 5800, at least for now.




Nokia hasn't released U.S. pricing details—or carriers, if any—for the 5800 yet. (Since the 5800 is a GSM handset, it'll only work with GSM-based carriers such as AT&T and T-Mobile.) In Europe, however, the phone (minus "Comes with Music," for now) will sell for 279 euros, or about US$385—not bad, considering the sky-high price tag of Nokia's N-series beauties.
How does the 5800 XpressMusic stack up with the iPhone and the G1? Well, hard to say until I see the phone itself in action—and especially whether the 5800's touch interface measures up to the two touch heavyweights.
My initial impression? I'm a bit underwhelmed, frankly; it's almost as if Nokia is wading cautiosly into the touchscreen pool with the 5800. What I'm really waiting for is a full-on, touchscreen Nseries handset, complete with a revamped interface designed specifically for touch. In any case, I'm reserving any final judgement until I get an actual unit in for review. (Update: Gizmodo just published a quick hands-on report, and so far, the touchscreen sounds pretty lackluster: "On the prototype we played with briefly, it's much harder to get touches to register, and far less accurate than the iPhone's capacitive screens. The 5800 packs a built-in stylus for this reason—you'll be using it a lot."
By Ben Patterson

Monday, September 15, 2008

THE MILE jeddah tower


Exploring urban issues facing 21st century, The Mile High Tower offers a fresh perspective on an idea that has been debated by architects for a century"1 mile =1600 M.
Exploding land values, growing populations and expanding economies are placing extraordinary burdens on many culturally rich, but land deprived Asian regions. In response to these pressures we have proposed a vertical city. In conceiving the tower as a vertical city, the design team has integrated technological, architectural and urban planning strategies into a single structure that breathes with urban complexity. The scale of the building and the scope of the program force the reevaluation of current skyscraper precedents for form, purpose, infrastructure, transportation, structure, and sustainability.
Architecture and engineering have traditionally treated structure as static—the building frame was constructed to be strong and heavy enough to resist all anticipated loads. The Mile High Tower proposes a lighter, dynamic structural system that actively responds to forces placed upon it. Controlled by wind detecting sensors, stabilizing aileron-like fins run the length of the tower frame and modulate their position to control resonant motion and building drift.
The separation of the structural frame and the building envelope enhances the quality of the interior space by providing an abundance of natural light and ventilation. Equipped with wind generators, photovoltaic panels, a heliostat, and sewage treatment facilities, the tower attains a high degree of sustainability with minimal environmental impact.
Approaching the tower as a theoretical project has proven liberating, freeing the design team to seek new solutions to technical problems, to find creative approaches outside the present financial climate, and to implement environmentally sustainable strategies that will enhance the next generation of ultra-high rise buildings. Our paradigm is the human body. This near-future tower incorporates structural and climatic systems that, like the human body, respond dynamically and efficiently to forces placed upon them.
Pickard Chilton company have done the skyscraper design, plus other specialized engineering firms for structural, infrastructure and traffic design, cost and time planning!!
Facts:
This "monster" is not standing alone, there is two other towers connected to it at the hight of 170 M by two bridges. ( these two towers will give this huge tower some kind of stability.Kingdom holding group retained HOK to do the master plan for the project and the soil test in the location,and they approved a super tall in the project.Estimates that the total investment potential that will be generated by this project will be in excess of SR 55 billion:
-around 15 % from that number for the super tall land mark ,around SR 8 billion= $ 2 billion.
-SR 400 million for the water canal(5 Km) around the project land "from the red sea on the west to the Abhur creek on the south of the project location"and the result for that is a new island on the north of abhur creek well change the map of Jeddah,and it will help the natural life in abhur creek.
SR 42 billion "$ 11 billion" several commercial towers, residential units, retail space, office space, a beach resort, hotels and an education campus.

Friday, September 12, 2008

LHC: Large Hadron Collider


Why the LHC


A few unanswered questions...
The LHC was built to help scientists to answer key unresolved questions in particle physics. The unprecedented energy it achieves may even reveal some unexpected results that no one has ever thought of!
For the past few decades, physicists have been able to describe with increasing detail the fundamental particles that make up the Universe and the interactions between them. This understanding is encapsulated in the Standard Model of particle physics, but it contains gaps and cannot tell us the whole story. To fill in the missing knowledge requires experimental data, and the next big step to achieving this is with LHC.


Newton's unfinished business...

What is mass?
What is the origin of mass? Why do tiny particles weigh the amount they do? Why do some particles have no mass at all? At present, there are no established answers to these questions. The most likely explanation may be found in the Higgs boson, a key undiscovered particle that is essential for the Standard Model to work. First hypothesised in 1964, it has yet to be observed.
The ATLAS and CMS experiments will be actively searching for signs of this elusive particle.


An invisible problem...

What is 96% of the universe made of?
Everything we see in the Universe, from an ant to a galaxy, is made up of ordinary particles. These are collectively referred to as matter, forming 4% of the Universe. Dark matter and dark energy are believed to make up the remaining proportion, but they are incredibly difficult to detect and study, other than through the gravitational forces they exert. Investigating the nature of dark matter and dark energy is one of the biggest challenges today in the fields of particle physics and cosmology.
The ATLAS and CMS experiments will look for supersymmetric particles to test a likely hypothesis for the make-up of dark matter.


Nature's favouritism...

Why is there no more antimatter?
We live in a world of matter – everything in the Universe, including ourselves, is made of matter. Antimatter is like a twin version of matter, but with opposite electric charge. At the birth of the Universe, equal amounts of matter and antimatter should have been produced in the Big Bang. But when matter and antimatter particles meet, they annihilate each other, transforming into energy. Somehow, a tiny fraction of matter must have survived to form the Universe we live in today, with hardly any antimatter left. Why does Nature appear to have this bias for matter over antimatter?
The LHCb experiment will be looking for differences between matter and antimatter to help answer this question. Previous experiments have already observed a tiny behavioural difference, but what has been seen so far is not nearly enough to account for the apparent matter–antimatter imbalance in the Universe.


Secrets of the Big Bang
What was matter like within the first second of the Universe’s life?
Matter, from which everything in the Universe is made, is believed to have originated from a dense and hot cocktail of fundamental particles. Today, the ordinary matter of the Universe is made of atoms, which contain a nucleus composed of protons and neutrons, which in turn are made of quarks bound together by other particles called gluons. The bond is very strong, but in the very early Universe conditions would have been too hot and energetic for the gluons to hold the quarks together. Instead, it seems likely that during the first microseconds after the Big Bang the Universe would have contained a very hot and dense mixture of quarks and gluons called quark–gluon plasma.
The ALICE experiment will use the LHC to recreate conditions similar to those just after the Big Bang, in particular to analyse the properties of the quark-gluon plasma.


Hidden worlds…
Do extra dimensions of space really exist?
Einstein showed that the three dimensions of space are related to time. Subsequent theories propose that further hidden dimensions of space may exist; for example, string theory implies that there are additional spatial dimensions yet to be observed. These may become detectable at very high energies, so data from all the detectors will be carefully analysed to look for signs of extra dimensions.


How the LHC works
The LHC, the world’s largest and most powerful particle accelerator, is the latest addition to CERN’s accelerator complex. It mainly consists of a 27 km ring of superconducting magnets with a number of accelerating structures to boost the energy of the particles along the way.
Inside the accelerator, two beams of particles travel at close to the speed of light with very high energies before colliding with one another. The beams travel in opposite directions in separate beam pipes – two tubes kept at ultrahigh vacuum. They are guided around the accelerator ring by a strong magnetic field, achieved using superconducting electromagnets. These are built from coils of special electric cable that operates in a superconducting state, efficiently conducting electricity without resistance or loss of energy. This requires chilling the magnets to about ‑271°C – a temperature colder than outer space! For this reason, much of the accelerator is connected to a distribution system of liquid helium, which cools the magnets, as well as to other supply services.
Thousands of magnets of different varieties and sizes are used to direct the beams around the accelerator. These include 1232 dipole magnets of 15 m length which are used to bend the beams, and 392 quadrupole magnets, each 5–7 m long, to focus the beams. Just prior to collision, another type of magnet is used to 'squeeze' the particles closer together to increase the chances of collisions. The particles are so tiny that the task of making them collide is akin to firing needles from two positions 10 km apart with such precision that they meet halfway!
All the controls for the accelerator, its services and technical infrastructure are housed under one roof at the CERN Control Centre. From here, the beams inside the LHC will be made to collide at four locations around the accelerator ring, corresponding to the positions of the particle detectors.


The LHC experiments
The six experiments at the LHC are all run by international collaborations, bringing together scientists from institutes all over the world. Each experiment is distinct, characterised by its unique particle detector.
The two large experiments, ATLAS and CMS, are based on general-purpose detectors to analyse the myriad of particles produced by the collisions in the accelerator. They are designed to investigate the largest range of physics possible. Having two independently designed detectors is vital for cross-confirmation of any new discoveries made.
Two medium-size experiments, ALICE and LHCb, have specialised detectors for analysing the LHC collisions in relation to specific phenomena.
Two experiments, TOTEM and LHCf, are much smaller in size. They are designed to focus on ‘forward particles’ (protons or heavy ions). These are particles that just brush past each other as the beams collide, rather than meeting head-on
The ATLAS, CMS, ALICE and LHCb detectors are installed in four huge underground caverns located around the ring of the LHC. The detectors used by the TOTEM experiment are positioned near the CMS detector, whereas those used by LHCf are near the ATLAS detector.


LHC Computing Grid
The Large Hadron Collider will produce roughly 15 petabytes (15 million gigabytes) of data annually – enough to fill more than 1.7 million dual-layer DVDs a year!
Thousands of scientists around the world want to access and analyse this data, so CERN is collaborating with institutions in 33 different countries to operate a distributed computing and data storage infrastructure: the LHC Computing Grid (LCG).
Data from the LHC experiments is distributed around the globe, with a primary backup recorded on tape at CERN. After initial processing, this data is distributed to eleven large computer centres – in Canada, France, Germany, Italy, the Netherlands, the Nordic countries, Spain, Taipei, the UK, and two sites in the USA – with sufficient storage capacity for a large fraction of the data, and with round-the-clock support for the computing grid.
These so-called “Tier-1” centres make the data available to over 120 “Tier-2” centres for specific analysis tasks. Individual scientists can then access the LHC data from their home country, using local computer clusters or even individual PCs.
The LCG collaborates closely with the other CERN grid projects:
The LHC Computing Grid has been the driving force behind the European multi-science grid Enabling Grids for E-SciencE (EGEE), which continues to grow in size and diversity of usage. EGEE currently involves more than 240 institutions in 45 countries, supporting science in more than 20 disciplines, including bioinformatics, medical imaging, education, climate change, energy, agriculture and more.
CERN openlab: The LCG project also works with industry, in particular through the CERN openlab, where leading IT companies are testing and validating cutting-edge grid technologies using the LCG environment.


The safety of the LHC
The Large Hadron Collider (LHC) can achieve an energy that no other particle accelerators have reached before, but Nature routinely produces higher energies in cosmic-ray collisions. Concerns about the safety of whatever may be created in such high-energy particle collisions have been addressed for many years. In the light of new experimental data and theoretical understanding, the LHC Safety Assessment Group (LSAG) has updated a review of the analysis made in 2003 by the LHC Safety Study Group, a group of independent scientists.
LSAG reaffirms and extends the conclusions of the 2003 report that LHC collisions present no danger and that there are no reasons for concern. Whatever the LHC will do, Nature has already done many times over during the lifetime of the Earth and other astronomical bodies. The LSAG report has been reviewed and endorsed by CERN’s Scientific Policy Committee, a group of external scientists that advises CERN’s governing body, its Council.
The following summarizes the main arguments given in the LSAG report. Anyone interested in more details is encouraged to consult it directly, and the technical scientific papers to which it refers.


Cosmic rays
The LHC, like other particle accelerators, recreates the natural phenomena of cosmic rays under controlled laboratory conditions, enabling them to be studied in more detail. Cosmic rays are particles produced in outer space, some of which are accelerated to energies far exceeding those of the LHC. The energy and the rate at which they reach the Earth’s atmosphere have been measured in experiments for some 70 years. Over the past billions of years, Nature has already generated on Earth as many collisions as about a million LHC experiments – and the planet still exists. Astronomers observe an enormous number of larger astronomical bodies throughout the Universe, all of which are also struck by cosmic rays. The Universe as a whole conducts more than 10 million million LHC-like experiments per second. The possibility of any dangerous consequences contradicts what astronomers see - stars and galaxies still exist.


Microscopic black holes
Nature forms black holes when certain stars, much larger than our Sun, collapse on themselves at the end of their lives. They concentrate a very large amount of matter in a very small space. Speculations about microscopic black holes at the LHC refer to particles produced in the collisions of pairs of protons, each of which has an energy comparable to that of a mosquito in flight. Astronomical black holes are much heavier than anything that could be produced at the LHC.
According to the well-established properties of gravity, described by Einstein’s relativity, it is impossible for microscopic black holes to be produced at the LHC. There are, however, some speculative theories that predict the production of such particles at the LHC. All these theories predict that these particles would disintegrate immediately. Black holes, therefore, would have no time to start accreting matter and to cause macroscopic effects.
Although stable microscopic black holes are not expected in theory, study of the consequences of their production by cosmic rays shows that they would be harmless. Collisions at the LHC differ from cosmic-ray collisions with astronomical bodies like the Earth in that new particles produced in LHC collisions tend to move more slowly than those produced by cosmic rays. Stable black holes could be either electrically charged or neutral. If they had electric charge, they would interact with ordinary matter and be stopped while traversing the Earth, whether produced by cosmic rays or the LHC. The fact that the Earth is still here rules out the possibility that cosmic rays or the LHC could produce dangerous charged microscopic black holes. If stable microscopic black holes had no electric charge, their interactions with the Earth would be very weak. Those produced by cosmic rays would pass harmlessly through the Earth into space, whereas those produced by the LHC could remain on Earth. However, there are much larger and denser astronomical bodies than the Earth in the Universe. Black holes produced in cosmic-ray collisions with bodies such as neutron stars and white dwarf stars would be brought to rest. The continued existence of such dense bodies, as well as the Earth, rules out the possibility of the LHC producing any dangerous black holes.


Strangelets
Strangelet is the term given to a hypothetical microscopic lump of ‘strange matter’ containing almost equal numbers of particles called up, down and strange quarks. According to most theoretical work, strangelets should change to ordinary matter within a thousand-millionth of a second. But could strangelets coalesce with ordinary matter and change it to strange matter? This question was first raised before the start up of the Relativistic Heavy Ion Collider, RHIC, in 2000 in the United States. A study at the time showed that there was no cause for concern, and RHIC has now run for eight years, searching for strangelets without detecting any. At times, the LHC will run with beams of heavy nuclei, just as RHIC does. The LHC’s beams will have more energy than RHIC, but this makes it even less likely that strangelets could form. It is difficult for strange matter to stick together in the high temperatures produced by such colliders, rather as ice does not form in hot water. In addition, quarks will be more dilute at the LHC than at RHIC, making it more difficult to assemble strange matter. Strangelet production at the LHC is therefore less likely than at RHIC, and experience there has already validated the arguments that strangelets cannot be produced.


Vacuum bubbles
There have been speculations that the Universe is not in its most stable configuration, and that perturbations caused by the LHC could tip it into a more stable state, called a vacuum bubble, in which we could not exist. If the LHC could do this, then so could cosmic-ray collisions. Since such vacuum bubbles have not been produced anywhere in the visible Universe, they will not be made by the LHC.


Magnetic monopoles
Magnetic monopoles are hypothetical particles with a single magnetic charge, either a north pole or a south pole. Some speculative theories suggest that, if they do exist, magnetic monopoles could cause protons to decay. These theories also say that such monopoles would be too heavy to be produced at the LHC. Nevertheless, if the magnetic monopoles were light enough to appear at the LHC, cosmic rays striking the Earth’s atmosphere would already be making them, and the Earth would very effectively stop and trap them. The continued existence of the Earth and other astronomical bodies therefore rules out dangerous proton-eating magnetic monopoles light enough to be produced at the LHC.


Reports and reviews
Studies into the safety of high-energy collisions inside particle accelerators have been conducted in both Europe and the United States by physicists who are not themselves involved in experiments at the LHC. Their analyses have been reviewed by the expert scientific community, which agrees with their conclusion that particle collisions in accelerators are safe. CERN has mandated a group of particle physicists, also not involved in the LHC experiments, to monitor the latest speculations about LHC collisions.
Download the Comments on claimed risks from metastable black holes
Download the Statement from the Executive Board of the Division of Particles and Fields of the American Physical Society (APS)
Download this summary of the LSAG report. Translations are available in the following languages : fr de el es it jp no pl ru.
Download the LSAG report (2008)
Download the specialist report published in Europe (2003)
Download the specialist report published in the United States(1999)
Download expert comment on speculations raised by Professor Otto Roessler about the production of black holes at the LHC
Download further expert comment on speculations raised by Professor Otto Roessler about the production of black holes at the LHC
Download another independent assessment of the safety of black hole scenarios at the LHC


Facts and figures
The largest machine in the world...
The precise circumference of the LHC accelerator is 26 659 m, with a total of 9300 magnets inside. Not only is the LHC the world’s largest particle accelerator, just one-eighth of its cryogenic distribution system would qualify as the world’s largest fridge. All the magnets will be pre‑cooled to -193.2°C (80 K) using 10 080 tonnes of liquid nitrogen, before they are filled with nearly 60 tonnes of liquid helium to bring them down to -271.3°C (1.9 K).


The fastest racetrack on the planet...
At full power, trillions of protons will race around the LHC accelerator ring 11 245 times a second, travelling at 99.99% the speed of light. Two beams of protons will each travel at a maximum energy of 7 TeV (tera-electronvolt), corresponding to head-to-head collisions of 14 TeV. Altogether some 600 million collisions will take place every second.


The emptiest space in the Solar System...
To avoid colliding with gas molecules inside the accelerator, the beams of particles travel in an ultra-high vacuum – a cavity as empty as interplanetary space. The internal pressure of the LHC is 10-13 atm, ten times less than the pressure on the Moon!


The hottest spots in the galaxy, but even colder than outer space...
The LHC is a machine of extreme hot and cold. When two beams of protons collide, they will generate temperatures more than 100 000 times hotter than the heart of the Sun, concentrated within a minuscule space. By contrast, the 'cryogenic distribution system', which circulates superfluid helium around the accelerator ring, keeps the LHC at a super cool temperature of -271.3°C (1.9 K) – even colder than outer space!


The biggest and most sophisticated detectors ever built...
To sample and record the results of up to 600 million proton collisions per second, physicists and engineers have built gargantuan devices that measure particles with micron precision. The LHC's detectors have sophisticated electronic trigger systems that precisely measure the passage time of a particle to accuracies in the region of a few billionths of a second. The trigger system also registers the location of the particles to millionths of a metre. This incredibly quick and precise response is essential for ensuring that the particle recorded in successive layers of a detector is one and the same.


The most powerful supercomputer system in the world...
The data recorded by each of the big experiments at the LHC will fill around 100 000 dual layer DVDs every year. To allow the thousands of scientists scattered around the globe to collaborate on the analysis over the next 15 years (the estimated lifetime of the LHC), tens of thousands of computers located around the world are being harnessed in a distributed computing network called the Grid.


LHC Milestones
Journey to a new frontier
The LHC accelerator was originally conceived in the 1980s and approved for construction by the CERN Council in late 1994. Turning this ambitious scientific plan into reality proved to be an immensely complex task.
Civil engineering work to excavate underground caverns to house the huge detectors for the experiments started in 1998. Five years later, the last cubic metre of ground was finally dug for the whole project.
Numerous state-of-the-art technologies were pushed even further to meet the accelerator's exacting specifications and unprecedented demands.
Anticipating the colossal amount of data the LHC's experiments would produce (nearly 1% of the world’s information production rate), a new approach to data storage, management, sharing and analysis was created in the LHC Computing Grid project.
For more than a decade, building the LHC had been a dream for many who have worked hard to bring it to completion. Finally we can retell the story of this adventure in a journey, from a dream to a reality…

From CERN

Wednesday, September 10, 2008

NASA's Shuttle and Rocket Missions



A variety of vehicles, launch sites on both U.S. coasts, shifting dates and times... the NASA Launch Schedule is easy to decipher by checking out our Launch Schedule 101 that explains how it all works! Updated -- September 5 - 11:30 a.m. EDT Legend: + Targeted For * No Earlier Than (Tentative) ** To Be Determined


2008 Launches


Date: October +Mission: TacSat-3Launch Vehicle: Orbital Sciences Minotaur Rocket Launch Site: Wallops Flight Facility - Goddard Space Flight Center Launch Time: ** -->Description: NASA will support the Air Force launch of the TacSat-3 satellite, managed by the Air Force Research Laboratory's Space Vehicles Directorate. TacSat-3 will demonstrate the capability to furnish real-time data to the combatant commander. NASA Ames will fly a microsat and NASA Wallops will fly the CubeSats on this flight in addition to providing the launch range. Date: Oct. 5 Mission: IBEX Launch Vehicle: Orbital Sciences Pegasus XL Rocket Launch Site: Reagan Test Site, Kwajalein Atoll Launch Window: 12:41 to 12:48 p.m. EDT Description: IBEX's science objective is to discover the global interaction between the solar wind and the interstellar medium and will achieve this objective by taking a set of global energetic neutral atom images that will answer four fundamental science questions. Date: Oct. 10 + Mission: STS-125 Launch Vehicle: Space Shuttle AtlantisLaunch Site: Kennedy Space Center Launch Pad 39A Launch Time: 12:33 a.m. EDT Landing Site: Kennedy Space Center's Shuttle Landing Facility Landing Date and Time: Oct. 20 + Description: Space Shuttle Atlantis will fly seven astronauts into space for the fifth and final servicing mission to the Hubble Space Telescope. During the 11-day flight, the crew will repair and improve the observatory's capabilities through 2013. Date: Nov. 12 + Mission: STS-126Launch Vehicle: Space Shuttle EndeavourLaunch Site: Kennedy Space Center - Launch Pad 39A Launch Time: 8:43 p.m. EST Landing Site: Kennedy Space Center's Shuttle Landing Facility Landing Date and Time: Nov. 27 + Description: Space Shuttle Endeavour launching on assembly flight ULF2, will deliver a Multi-Purpose Logistics Module to the International Space Station.


2009 Launches


Date: 2009 Mission: Ares I-X Test Flight Launch Vehicle: Ares I-X Launch Site: Kennedy Space Center - Launch Pad 39B Description: The Ares I-X test flight is NASA's first test flight for the Agency's new Constellation launch vehicle -- Ares I. The Ares I-X flight will provide NASA with an early opportunity to test and prove flight characteristics, hardware, facilities and ground operations associated with the Ares I. Date: Jan. 15 Mission: OCO Launch Vehicle: Orbital Sciences Taurus Rocket Launch Site: Vandenberg Air Force Base - Launch Pad SLC 576-E Launch Time: ** -->Description: The Orbiting Carbon Observatory is a new Earth orbiting mission sponsored by NASA's Earth System Science Pathfinder Program. Date: Jan. 23 * Mission: STSS Demonstrators Program - Missile Defense AgencyLaunch Vehicle: United Launch Alliance Delta II Launch Site: Cape Canaveral Air Force Station - Launch Complex 17, Pad A Launch Time: ** -->Description: STSS Demonstrators Program is a midcourse tracking technology demonstrator and is part of an evolving ballistic missile defense system. STSS is capable of tracking objects after boost phase and provides trajectory information to other sensors and interceptors. To be launched by NASA for the Missile Defense Agency. Date: Feb. 4 Mission: NOAA-N Prime Launch Vehicle: United Launch Alliance Delta II Launch Site: Vandenberg Air Force Base - Launch Pad SLC-2 Launch Time: ** -->Description: NOAA-N Prime is the latest polar-orbiting satellite developed by NASA/Goddard Spaceflight Center for the National Oceanic and Atmospheric Administration (NOAA). NOAA uses two satellites, a morning and afternoon satellite, to ensure every part of the Earth is observed at least twice every 12 hours. NOAA-N will collect information about Earth's atmosphere and environment to improve weather prediction and climate research across the globe. Date: Feb. 10 * Mission: GOES-OLaunch Vehicle: United Launch Alliance Delta IV Launch Site: Cape Canaveral Air Force Station - Launch Complex 37 Launch Time: -->Description: NASA and the National Oceanic and Atmospheric Administration (NOAA) are actively engaged in a cooperative program, the multi-mission Geostationary Operational Environmental Satellite series N-P. This series will be a vital contributor to weather, solar and space operations, and science. Date: Feb. 12 + Mission: STS-119Launch Vehicle: Space Shuttle DiscoveryLaunch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Discovery launching on assembly flight 15A, will deliver the fourth starboard truss segment to the International Space Station. Date: March 2 * Mission: LRO/LCROSS Launch Vehicle: United Launch Alliance Atlas V Launch Site: Cape Canaveral Air Force Station - Launch Complex 41 Launch Time: ** -->Description: LRO will launch with the objectives to finding safe landing sites, locate potential resources, characterize the radiation environment and test new technology. The Lunar CRater Observing and Sensing Satellite mission is seeking a definitive answer about the presence or absence of water ice in a permanently shadowed crater at either the Moon's North or South Pole. Date: April 10 Mission: KeplerLaunch Vehicle: United Launch Alliance Delta II Launch Site: Cape Canaveral Air Force Station - Launch Complex 17 - Pad 17-B Launch Time: ** -->Description: The Kepler Mission, a NASA Discovery mission, is specifically designed to survey our region of the Milky Way galaxy to detect and characterize hundreds of Earth-size and smaller planets in or near the habitable zone. Date: April 30 Mission: STSS ATRR - Missile Defense AgencyLaunch Vehicle: United Launch Alliance Delta II Launch Site: Vandenberg Air Force Base - Launch Pad SLC-2 Launch Time: ** -->Description: STSS ATRR serves as a pathfinder for future launch and mission technology for the Missile Defense Agency. To be launched by NASA for the MDA. Date: May 15 + Mission: STS-127Launch Vehicle: Space Shuttle Endeavour Launch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Endeavour will deliver the exposed facility of Japan's Kibo laboratory to the International Space Station. Date: June 15 Mission: Glory Launch Vehicle: Orbital Sciences Taurus Rocket Launch Site: Vandenberg Air Force Base - Launch Pad SLC 576-E Launch Time: ** -->Description: The Glory Mission will help increase our understanding of the Earth's energy balance by collecting data on the properties of aerosols and black carbon in the Earth's atmosphere and how the Sun's irradiance affects the Earth's climate. Date: July 30 + Mission: STS-128 Launch Vehicle: Space Shuttle Atlantis Launch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Atlantis will use a Multi-Purpose Logistics Module to carry experiment and storage racks to the International Space Station. Date: Sept. 15 * Mission: Mars Science Laboratory Launch Vehicle:
Launch Site:
Launch Time: ** -->Description: The Mars Science Laboratory is a rover that will assess whether Mars ever was, or is still today, an environment able to support microbial life and to determine the planet's habitability. Date: Oct. 15 + Mission: STS-129Launch Vehicle: Space Shuttle DiscoveryLaunch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Discovery will deliver components including two spare gyroscopes, two nitrogen tank assemblies, two pump modules, an ammonia tank assembly and a spare latching end effector for the station's robotic arm to the International Space Station. Date: November + Mission: WISE Launch Vehicle:
Launch Site:
Launch Time: ** -->Description: The Wide-field Infrared Survey Explorer (WISE) will survey the entire sky in the mid-infrared with far greater sensitivity than any previous mission or program ever has. The WISE survey will consist of over a million images, from which hundreds of millions of astronomical objects will be catalogued. Date: Dec. 10 + Mission: STS-130Launch Vehicle: Space Shuttle Endeavour Launch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Endeavour will deliver the final connecting node, Node 3, and the Cupola, a robotic control station with six windows around its sides and another in the center that provides a 360-degree view around the International Space Station.


2010 Launches


Date: Mission: SDO Launch Vehicle: United Launch Alliance Atlas V Launch Site: Cape Canaveral Air Force Station - Launch Complex 41 Launch Time: ** -->Description: The first Space Weather Research Network mission in the Living With a Star (LWS) Program of NASA. Date: Feb. 11 + Mission: STS-131Launch Vehicle: Space Shuttle AtlantisLaunch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Atlantis will carry a Multi-Purpose Logistics Module filled with science racks that will be transferred to laboratories of the International Space Station. Date: April 8 + Mission: STS-132Launch Vehicle: Space Shuttle DiscoveryLaunch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Discovery mission will carry an integrated cargo carrier to deliver maintenance and assembly hardware, including spare parts for space station systems. In addition, the second in a series of new pressurized components for Russia, a Mini Research Module, will be permanently attached to the bottom port of the Zarya module. Date: May 31 + Mission: STS-133Launch Vehicle: Space Shuttle Endeavour Launch Site: Kennedy Space Center - Launch Pad 39A Launch Time: ** -->Description: Space shuttle Endeavour will deliver critical spare components including antennas and gas tanks to the International Space Station.

Sunday, September 7, 2008

The Cigar Manufacturing Process


The making of a premium hand-rolled cigar is a complicated, time consuming and highly skilled process. In some factories, human hands may touch a cigar leaf more than 40 times by the time the process is completed!What goes into cigars? The cigar making process is the key to assessing the quality of a specific cigar.In making a handmade cigar, two to four filler leaves (depending on the size and strength of the cigar) are laid end to end and rolled into the two halves of the binder leaves, making up what is called the "bunch". Great skill is required to make sure that the filler is evenly distributed so that the cigar will draw properly. Wooden molds are used into which the filler blend (rolled into the binder) is pressed by the "bunchers", with a mechanical press then used to complete the process. In the Havana factory, the same person who eventually adds the wrapper does the bunching. The practice is slightly different in, for instance, the factories of the Dominican Republic, where specialist bunchers work in teams with specialist wrapper rollers. In both systems, the result is that each roller has a supply of ready molded fillers, prepared for what is being made on that day, at his or her work bench.Surplus filler is trimmed from the end to form a round top. A wrapper leaf is then selected, the remaining stalk is stripped off the binder, and the wrapper is trimmed to the right size (using the central part of the leaf, placed upside-down, to avoid having any veins showing) with an oval steel blade called a chaveta.The cylinder of tobacco in its binder (the "bunch") is now laid at an angle across the wrapper, which is then stretched as necessary and wound carefully around the binder, overlapping at each turn, until it is stuck down using a tiny drop of colorless and flavorless tragacanth vegetable gum. The cigar is then rolled; applying gentle pressure, with the flat part of the steel blade to make sure its construction is even. Next, a small round piece of wrapper (about the size of a small coin) is cut out from the trimmings on hand to form the cap, which is stuck in place. In the case of cigars such as the Montecristo Especial, twisting the end of the wrapper seals the closed end. This is a version of what is known as the "flag" method of capping a cigar, a highly skilled process in which the wrapper itself is smoothed down to form the cap. The flag method is only used on the best handmade cigars, and never on machine-made. Finally, the open end is guillotined to the correct length.The construction of a cigar is a crucial factor in how well you enjoy it. If it is under-filled, it will draw easily, but burn fast, and get hot and harsh as a result. If it is over-filled, it will be difficult to draw on, or "plugged". Good cigars have to be consistent. That relies on skill, quality control, and the resources (reserves of suitable leaf, essentially) to guarantee that this year's cigars are the same as last year's, even if there is a bad harvest.

Friday, September 5, 2008

Saudi Arabia's Construction Boom


RABIGH, Saudi Arabia — The alarm bell sounded the end of the lunch break here one November afternoon, and suddenly thousands of workers — on foot, on bicycles and in buses — streamed in, seemingly from out of nowhere, and jolted this huge construction site to life.Amid a forest of cranes, towers and beams rising from the desert, more than 38,000 workers from China, India, Turkey and beyond have been toiling for two years in unforgiving conditions — often in temperatures exceeding 100 degrees — to complete one of the world's largest petrochemical plants in record time. By the end of the year, this massive city of steel at the edge of the Red Sea will take its place as a cog of globalization: plastics produced here will be used to make televisions in Japan, cell phones in China and thousands of other products to be sold in the United States and Europe. Construction costs at the plant, which spreads over eight square miles, have doubled to $10 billion because of shortages in materials and labor. The amount of steel being used is 10 times the weight of the Eiffel Tower."I've worked on many big things in my life, but I've never worked on anything this big," an American project manager mused during a bus tour of the project, called Petro Rabigh, a joint venture of the state-run oil company Saudi Aramco and Sumitomo Chemical of Japan. Size isn't the only consideration. The project is Saudi Arabia's boldest bet yet that this oil-rich kingdom can transform itself into an industrial powerhouse. The plant is part of a $500 billion investment program to build new cities, create millions of jobs and diversify the economy away from petroleum exports over the next two decades."The Saudi economy was in idle mode for 20 years," said John Sfakianakis, the chief economist at SABB, formerly known as the Saudi British Bank, who is based in Riyadh, the Saudi capital. "Today, the feeling here is, 'We've won the lottery; let's not waste it.'"The kingdom's lofty economic goals would have been unthinkable without the surge in energy prices that has filled the coffers of oil producers. Oil prices have quadrupled since 2002 and reached $100 a barrel in New York this month. Persian Gulf countries earned $1.5 trillion in oil revenue from 2002 to 2006, twice as much as in the previous five-year period, according to the Institute of International Finance, a global association of banks that is based in Washington. As the top exporter, Saudi Arabia has been the main beneficiary.Despite all the recent headlines about Middle East investors bailing out troubled American banks like Citigroup, a growing share of today's petrodollars are staying at home to finance megaprojects like Petro Rabigh, analysts say. That money is financing the biggest economic boom in a generation, helping to build not only the high-rises of Dubai, where the world's tallest tower is going up, but also telecommunications networks, roads and universities throughout the Middle East. Abu Dhabi is planning to spend close to $1 billion for a new museum with the help of the Louvre, in Paris. Dubai's latest grandiose idea is to build a small-scale replica of the French city of Lyon, complete with residential housing, a museum, a culinary school and a soccer club.
In Saudi Arabia, Riyadh looks like a boom town: sprawling over 40 miles, it is teeming with shopping malls, electronics stores and luxury boutiques. But while times are good today, many Saudis realize that their country is locked in a race against time to create industries that produce more than just oil in order to keep a young and growing population employed. The kingdom, which has a population of 24.5 million, including nearly 7 million foreigners, has what one analyst called a "human time bomb." About 40 percent of Saudis are under 15, and because the country has one of the world's highest birth rates, the population is expected to reach nearly 40 million by 2025. "It has been a social, and therefore a political, imperative of the Saudi government to develop the economy and to create employment opportunities," said Timothy S. Gray, the chief executive of HSBC Saudi Arabia.That could well mean that higher oil prices are here to stay. One paradox of modern-day Saudi Arabia is that while it seeks to reduce the importance of petroleum to its economy, it needs those exports more than ever.To be sure, the region's economies are too small to absorb all the oil riches on their own. Too much money is chasing too few assets, analysts say, forcing oil producers to invest some of their revenue abroad and diversify their holdings, either through opaque state-owned investment funds or through direct private investments. Last year, for example, a fund controlled by the government of Abu Dhabi bought a stake in Citigroup for $7.5 billion, while another run by Dubai's ruler bought a large share in Sony, the Japanese consumer electronics giant. Sabic, a major Saudi petrochemical company, bought the plastics division of General Electric for $11.6 billion, and the Kuwait Petroleum Corporation bought half of Dow Chemical's commodity-plastics unit for $9.5 billion. In recent weeks, other big banks plagued by losses from the mortgage crisis, like Merrill Lynch and Morgan Stanley, have raised tens of billions of dollars from a variety of Middle Eastern and Asian funds, including ones from Kuwait or Saudi Arabia.
According to data compiled by Bloomberg News, overseas investments by Persian Gulf countries reached a record $75 billion in 2007. Arms deals, a time-worn way of recycling petrodollars, remain popular in the region; the United States is pushing for a $20 billion weapons sale to Saudi Arabia, for example. But while oil-rich states are still buying American Treasury bonds or military hardware from the West, analysts say the more significant trend is for a growing share of their investments to be pumped into local projects. "The vision is to turn the kingdom into a major industrial power by 2020," said Jean-François Seznec, a professor at Georgetown University who is a specialist in industrial policies in the Persian Gulf. "A billion dollars here and a billion there, and soon you’re talking about real money."Projects like Petro Rabigh, Mr. Seznec said, will allow Saudi Arabia to become one of the top three chemical producers in the world within a few years. Unlike Kuwait or Abu Dhabi, Saudi Arabia does not have a sovereign fund responsible for investing the country's petroleum riches. Ali Al-Naimi, the kingdom's energy minister and one of the grand architects of Saudi industrial policy, summed up the country's goals at the dedication ceremony for Petro Rabigh in 2006."I would like to highlight the fact that the Petro Rabigh project is part of a bigger picture," Mr. Naimi said at the time. "This strategy includes expanding the base of the Saudi economy, diversifying national income sources, attracting international investments and reaping the direct and indirect benefits that these types of projects will accrue to the Saudi citizen.” The trend to modernize and develop the economy is not entirely new, of course. Saudi Arabia has been trying to diversify itself for over two decades. It famously tried to make the desert bloom in the 1970s and ’80s by investing heavily in water desalinization plants and growing crops. But a long period of low oil prices, from the mid-1980s through the 1990s, stalled much of its effort. The government still relies on petroleum exports for 90 percent of its revenue; oil sales account for half of the country’s gross domestic product. The current level of oil prices has given the country's industrialization strategy a new spring, allowing the government to improve its finances while investing in large infrastructure projects. The Saudi G.D.P. has doubled in the last five years. Not counting oil, economic growth has been 4 percent to 6 percent a year since 2002. Oil has not been the only engine of growth. The country’s private sector has also thrived and now accounts for 45 percent of the economy, compared with just 20 percent about 20 years ago. Since the 1990s, the share of private Saudi money invested at home has doubled, and now represents about 20 percent of total holdings, according to SABB."There is a lot of money looking for investment opportunities," said Mr. Gray at HSBC.The financial turnaround has been spectacular. In 1999, the Saudi government's debt amounted to 120 percent of G.D.P. That number has dropped to less than 20 percent as the government paid back its obligations and put its finances in order.Last year, the government recorded a budget surplus of $48 billion, five times the surplus of 2003. This year, it has built its biggest budget to date around a conservative estimate of oil prices of $45 a barrel; that will almost certainly yield a substantial surplus at the end of the year. All of that is a far cry from the 1990s, when oil averaged $20 a barrel, thanks mostly to Saudi concerns at the time to keep oil prices low. One of the most noticeable illustrations of the industrialization push is a plan championed by King Abdullah, the 83-year-old Saudi monarch, to build six new cities throughout the country — including the King Abdullah Economic City on the western coast, near the city of Rabigh; the Knowledge Economic City, near Medina; and the Prince Abdulaziz bin Mousaed Economic City, in the north. The intent is to create industrial centers that double as housing and commercial hubs for the country's young and growing population. The Saudi Arabian General Investment Authority, a government agency, expects these cities to add $150 billion to the country’s G.D.P. by 2020, create one million new jobs and be home to as many as five million people. Drawings of these new towns depict a cross of the futuristic "Blade Runner" and traditional Arabic design. But the new cities are also expected to become new industrial centers that focus on four main sectors: petrochemicals, aluminum, steel and fertilizers. According to SABB, these cities together will have four times the geographical area of Hong Kong, three times the population of Dubai, and an economic output equal to Singapore's. Other plans include building four refineries, two petrochemical plants and a modern graduate-level university with an endowment of $10 billion. The frenzied growth of the economy has had some serious downsides. Inflation has been rampant in the last year; food prices and rents have risen sharply. Traffic jams in Riyadh and other Saudi cities have become a constant affliction, while real estate values have soared and the construction sector is strained by a lack of workers. The stock market, meanwhile, has yet to recover from its collapse two years ago. From 2000 to early 2006, the local Tadawul stock index surged from 2,000 points to a peak of 19,870, a return of almost 900 percent. But the overvalued market went into a panicky free fall that caused it to lose two-thirds of its value in a matter of months.After being flat for most of 2007, the market has recovered in the last quarter, gaining more than 40 percent. Still, its value is only about half that of its peak two years ago.One reason for the partial rebound was anticipation of the sale of shares in Petro Rabigh earlier this month. For the first time, Saudi investors had a chance to buy a major asset linked to Aramco. The initial public offering, for 25 percent of Petro Rabigh, raised $1.23 billion and was the largest stock sale in Saudi history. The stock is expected to begin trading at the end of the month. The project itself is still about a year away from completion. Once in operation, it will produce 2.4 million tons of plastics a year. This venture, along with dozens of other megaprojects, will firmly anchor Saudi Arabia as one of the world’s top suppliers of chemical products as well as oil."Saudi Aramco has a vision of itself as Exxon Mobil," Mr. Seznec of Georgetown said, "except much bigger." From The New York Times on the Web (c) The New York Times Company.

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