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Kristin Cavallari Shows Off Her Long Legs in a Red Mini Skirt and Nude High Heels on the Red Carpet

February 11, 2012 By WebGlitzer

Kristin Cavallari has amazing legs. They are on full display in a short red dress and ever present Christian Louboutin nude pumps as she makes her way down the red carpet.Toned and fit, her long legs are a sight to behold. Well done.

Kristin Cavallari legsKristin Cavallari legsKristin Cavallari legs

HOLLYWOOD, CA – FEBRUARY 08: Actress Kristin Cavallari attends the ‘This Means War’ Los Angeles premiere held at Grauman’s Chinese Theatre on February…

Source: Best Celebrity Legs in High Heels

Filed Under: Celebrity, Sexy Legs Tagged With: high heels, mini skirt

Ashanti is Curvy and Leggy in a Revealing Dress and High Heels on the Red Carpet

February 10, 2012 By WebGlitzer

Ashanti shows off her impressive curves and shapely legs as she makes her way down the red carpet for a movie premiere. The short and low-cut dress is quite revealing displaying her beautiful cleavage and sexy legs. And of course she has mounted herself in the ever peasant Christian Louboutin platform nude pumps. She’s a pretty woman with eye-popping curves and  a style that indicates she enjoys the attention her sex appeal brings.

Ashanti legsAshanti legs

NEW YORK, NY – FEBRUARY 07: Ashanti attends the “Safe House” premiere at the SVA Theater on February 7, 2012 in New York City. (Photo by Jamie Images)…

Source: Best Celebrity Legs in High Heels

Filed Under: Celebrity

Galactic Views (22)

February 10, 2012 By WebGlitzer

←
SPACE WATCH

Portrait of a Doomed Asteroid
NASA – A new study provides a possible explanation of mysterious X-ray flares detected by the Chandra K-ray Observatory for several years in the region of Sagittarius A*, or Sgr A**. The study suggests a cloud around Sgr A*, a supermassive black hole at the center of our Milky Way Galaxy, which contains hundreds of trillions of asteroids and comets that have been stripped from their parent stars. The flares occur when asteroids of six miles or larger in radius are consumed by the black hole. An asteroid that undergoes a close encounter with another object, such as a star or planet, can be thrown into an orbit headed towards Sgr A*. If the asteroid passes within about 100 million miles of the black hole, roughly the distance between the Earth and the sun, it is torn into pieces by the tidal forces from the black hole. These fragments would then be vaporized by friction as they pass through the hot, thin gas flowing onto Sgr A*, similar to a meteor heating up and glowing as it falls through Earth’s atmosphere. A flare is produced and eventually the remains of the asteroid are swallowed by the black hole. Image Credit: Illustrations: NASA/CXC/M.Weiss

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This entry was posted in Nature, Science, SPACE WATCH and tagged Asteroid, Atmosphere of Earth, Black hole, Earth, Milky Way, NASA, Sagittarius A*, Space, Supermassive black hole. Bookmark the permalink.

Source: the Net economy

Filed Under: Photos

Rose McGowan Blisters the Runway in a Leggy Display of Red

February 10, 2012 By WebGlitzer

Rose McGowan has great legs in high heels. The woman has a nice body and from what I can tell spends time maintaining those toned stems from frequent gym visits. I simply wish she would stop pumping her face full of poison. I realize that celebs have it in their thick heads that a no lines, no wrinkles, is somehow a beautiful thing as women age. But dammit, you people look ridiculous. Your faces look like masks and completely fake. Enjoy your gorgeous body and take age on with class and dignity and not syringes and scalpels.

Rose McGowan legsRose McGowan legs

NEW YORK, NY – FEBRUARY 08: Actress Rose McGowan walks on the runway wearing a Donna Karen design at The Heart Truth’s Red Dress Collection 2012 Show…

Source: Best Celebrity Legs in High Heels

Filed Under: Celebrity

Galactic Views (21)

February 9, 2012 By WebGlitzer

←
SPACE WATCH

Remnant of a Supernova
NASA – Vital clues about the devastating ends to the lives of massive stars can be found by studying the aftermath of their explosions. In its more than twelve years of science operations, NASA’s Chandra X-ray Observatory has studied many of these supernova remnants sprinkled across the galaxy.

The latest example of this important investigation is Chandra’s new image of the supernova remnant known as G350.1-0.3. This stellar debris field is located some 14,700 light years from the Earth toward the center of the Milky Way.

Evidence from Chandra and from ESA’s XMM-Newton telescope suggest that a compact object within G350.1+0.3 may be the dense core of the star that exploded. The position of this likely neutron star, seen by the arrow pointing to “neutron star” in the inset image, is well away from the center of the X-ray emission. If the supernova explosion occurred near the center of the X-ray emission then the neutron star must have received a powerful kick in the supernova explosion.

Data suggest this supernova remnant, as it appears in the image, is 600 and 1,200 years old. If the estimated location of the explosion is correct, this means the neutron star has been moving at a speed of at least 3 million miles per hour since the explosion.

Another intriguing aspect of G350.1-0.3 is its unusual shape. Many supernova remnants are nearly circular, but G350.1-0.3 is strikingly asymmetrical as seen in the Chandra data in this image (gold). Infrared data from NASA’s Spitzer Space Telescope (light blue) also trace the morphology found by Chandra. Astronomers think that this bizarre shape is due to stellar debris field expanding into a nearby cloud of cold molecular gas.

The age of 600-1,200 years puts the explosion that created G350.1-0.3 in the same time frame as other famous supernovas that formed the Crab and SN 1006 supernova remnants. However, it is unlikely that anyone on Earth would have seen the explosion because of the obscuring gas and dust that lies along our line of sight to the remnant.

These results appeared in the April 10, 2011 issue of The Astrophysical Journal. Image Credits: X-ray: NASA/CXC/SAO/I. Lovchinsky et al; IR: NASA/JPL-Caltech

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Source: the Net economy

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Galactic Views (21)

February 9, 2012 By WebGlitzer

←
SPACE WATCH

Remnant of a Supernova
NASA – Vital clues about the devastating ends to the lives of massive stars can be found by studying the aftermath of their explosions. In its more than twelve years of science operations, NASA’s Chandra X-ray Observatory has studied many of these supernova remnants sprinkled across the galaxy.

The latest example of this important investigation is Chandra’s new image of the supernova remnant known as G350.1-0.3. This stellar debris field is located some 14,700 light years from the Earth toward the center of the Milky Way.

Evidence from Chandra and from ESA’s XMM-Newton telescope suggest that a compact object within G350.1+0.3 may be the dense core of the star that exploded. The position of this likely neutron star, seen by the arrow pointing to “neutron star” in the inset image, is well away from the center of the X-ray emission. If the supernova explosion occurred near the center of the X-ray emission then the neutron star must have received a powerful kick in the supernova explosion.

Data suggest this supernova remnant, as it appears in the image, is 600 and 1,200 years old. If the estimated location of the explosion is correct, this means the neutron star has been moving at a speed of at least 3 million miles per hour since the explosion.

Another intriguing aspect of G350.1-0.3 is its unusual shape. Many supernova remnants are nearly circular, but G350.1-0.3 is strikingly asymmetrical as seen in the Chandra data in this image (gold). Infrared data from NASA’s Spitzer Space Telescope (light blue) also trace the morphology found by Chandra. Astronomers think that this bizarre shape is due to stellar debris field expanding into a nearby cloud of cold molecular gas.

The age of 600-1,200 years puts the explosion that created G350.1-0.3 in the same time frame as other famous supernovas that formed the Crab and SN 1006 supernova remnants. However, it is unlikely that anyone on Earth would have seen the explosion because of the obscuring gas and dust that lies along our line of sight to the remnant.

These results appeared in the April 10, 2011 issue of The Astrophysical Journal. Image Credits: X-ray: NASA/CXC/SAO/I. Lovchinsky et al; IR: NASA/JPL-Caltech

Related articles
  • Galactic Views (18) (theneteconomy.wordpress.com)
  • Galactic Views (15) (theneteconomy.wordpress.com)

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Source: the Net economy

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Victoria’s Secret Angels Are Leggy in Silver Mini Dresses and High Heels

February 9, 2012 By WebGlitzer

Lindsay Ellingson, Adriana Lima, and Doutzen Kroes play around with their undies as they pose for the cameras in mini dresses and high heels which show off their impossible lingerie model bodies. These women are pretty but seem so completely brainless standing around with panties and brassieres draped over their half-dressed figures. It’s interesting watching these women in various states of undress while one of their own, Kylie Bisutti, decided to quit modeling lingerie for all but her husband.

Victoria's Secret Angels Victoria's Secret Angels legs

NEW YORK, NY – FEBRUARY 08: (L-R) Models Lindsay Ellingson, Adriana Lima, and Doutzen Kroes attend the Victoria’s Secret Angels Valentine’s Day Event D…

Source: Best Celebrity Legs in High Heels

Filed Under: Celebrity

Connected Cars: How to Accelerate Mainstream Adoption

February 9, 2012 By WebGlitzer

Steve Tengler is a user experience (UX) director at Altia, Inc. He spent over 20 years in automotive design at OnStar, Nissan and Ford.

Every so often, the media tells us about an automotive manufacturer on the cusp of delivering wireless, cooperative systems. The reader immediately thinks of Knight Rider, and wanders through a fantasy of connected car heaven.

However, this type of news is often miles from accurate; connected car offerings in the near-to-distant future are a different reality. This article examines the delays behind that “nearly done” automotive technology, and analyzes the value of our research dollars.

In 2005, several automakers introduced cooperative, wireless systems at the Intelligent Transportation Society World Congress in the parking lot of the San Francisco Giants’s then SBC Park. Messages were sent vehicle-to-vehicle and vehicle-to-infrastructure via dedicated short-range communications (DSRC) or, as it would later be renamed, “IEEE 802.11p (5.9 GHz).”

Most of the applications were safety-related systems that offered a seemingly futuristic understanding of position, speed and road conditions. But that was six long years ago – so, what has changed? Apart from the Giants stadium name-change, not much. Technology is no closer to the marketplace. Let’s explore why.


The “Co” in Cooperation


If you’ve heard the saying “the second mouse gets the cheese,” then you understand the fate of the first mouse — snap! Similarly, no company has succumbed to the lure of the first-to-market-cheese since each has foreseen the trap: producing a cooperative system with no cooperation.

Let’s imagine you are a leading automotive manufacturer that holds 20% of the U.S. market. That market is projected to reach 14 million vehicles in 2012. Considering there are over 250 million vehicles on the road, you could potentially communicate with 1.1% of the vehicles after just one year, assuming you installed the $ 200-$ 300 worth of equipment on all of your vehicles.

The first customer to purchase a wireless device creates the equivalent of a tree falling in an unoccupied forest. How satisfied will he or she be? If there’s no one else with whom to communicate, then not very satisfied at all. And how differentiating will that system be when all other automotive companies introduce systems that communicate the same information as your breakthrough device? Again, not at all. The moral to this story? In this case, being first has few rewards.


The Technology Hurdles


There are still four hiccups in the technology that, surprisingly, don’t make it to the media all that often.

  • Security: If someone hacks into the system, there needs to be a means of crime identification and removal (e.g. law enforcement, disabling hardware, ignoring false broadcasts, etc.). Otherwise, Joe Hacker could ease his commute by diverting traffic or creating city-wide chaos. However, this level of security management requires a backhaul system to a centralized certificate authority (someone who manages the system). At one point, the government considered making this a series of installed roadside or intersection locations, but that was too expensive and fraught with state-to-state complications. The individual OEMs could seek an embedded or accommodated cellular connection (e.g. OnStar or SYNC), but those require cuts in penetration, depending on the actions of the customer, who could cancel his OnStar subscription, forget to connect, or turn on a Bluetooth cellphone. So, right now there’s no easy one-size-fits-all solution to security.
  • Positioning: Any semi-autonomous system currently provides lane positioning by white-line monitoring (i.e. lane markers), but according to AASHTO, the likelihood of a lane departure fatality is twice as high in rural areas, where lane markings are less common and also tend to have inferior lighting and snow removal. To overcome that challenge, the vehicle must have highly accurate, autonomous positioning. This can only be achieved with one of several expensive solutions.
  • Packet Collisions: Imagine being on the floor of the stock market — lots of people screaming, no one can effectively hear everyone all at once. During the initial phases of cooperative research on platooning done by the automotive manufacturers, this is exactly what the investigations determined. In congested multi-lane highway situations, each vehicle would be trying to broadcast its location, but no one would be able to “hear” it. Therefore, platooning would not be successfully (or safely) achieved.
  • Intelligence: As artfully described by Hotchkiss in “Understanding the Human Part of the User Experience,” we humans are unbelievably adept decision-makers. Replacing us for even simple, predictable tasks like chess has taken decades and serious processing power. Driving is a complex task that requires thousands of decisions and reactions every mile. Implementing humans’ complex, dynamic decisions and observations to create an autonomous system is an enormous task.

The Business Case


How does the automotive manufacturer make a profit on these cooperative, non-differentiating systems? How can an automotive manufacturer easily charge for the hardware? If infrastructure must be supplied, how is it governed?

The question of collective business was mentioned by The National Highway Traffic Safety Administration (NHTSA) at the 2011 Transportation Research Board’s annual meeting, despite nearly a decade of investigations into cooperative technology. Until a means of making money is clearly delineated, no companies will be lining up to platoon, regardless of the societal benefits.

The solution occasionally proposed is that Wi-Fi could provide the accident avoidance systems, along with non-safety Internet connectivity at intersections. This plan is fraught with technological issues (the latency to join the intersection group — known as association timing — is too great) as well as business issues. Who pays to install Wi-Fi at millions of intersections? If the government gets that bill, how does it avoid competing with the private sector? Regardless of public or private, how does today’s car count on the infrastructure 10 years from today? Who co-pays for maintenance? Maybe Google will provide free Wi-Fi, or maybe it will fizzle like some of the company’s other beta releases.


Some Potential Solutions


Now, we’re not expecting a Jetsons-type car, but a few key companies could help realize basic wireless functionality. The solutions, though, require the following strategic elements.

  • Creative User Experience: To differentiate from the cooperative systems competition, the user experience (UX) must be unique in some fashion. For safety systems such as intersection collision avoidance and platooning, it is actually undesirable to have non-standard interfaces, since a common warning is more likely to elicit a common reaction. To differentiate, the OEM must create non-safety applications with unique UXs that provide value using the same technology. Be it a local chat room, an automated license plate game, or a quasi-classified information exchange, the human-machine interface that provides the unique customer experience in a safe manner will justify or subsidize the costs.
  • Sleeping with the Enemy: Entering the market via only one OEM is insufficient, but co-launching the system with one or two other vehicle manufacturers could easily result in 50-60% market penetration. This would require a coordinated launch, which is difficult enough with one OEM across multiple vehicle platforms, but is especially challenging between competitors. As crazy as it sounds, GM and Toyota have already discussed the opportunity, but reportedly struck no deal for co-distribution. Some OEMs are awaiting a mandate from the U.S. government that requires companies to install DSRC equipment, but that’s the best way to arrive last to the party with little to no differentiation.
  • The Alpha and the Omega: To launch the system, the vehicle and the infrastructure must exist first. The only ways for an automaker to ensure this is to either use something existing or provide the enabler on its own. Be it an embedded cellular system (e.g. Lexus Enform, GM OnStar) or an integration solution (e.g. Ford SYNC), the backhaul must attach to a privately-run security system. Otherwise, the design is fraught with risks that no manufacturer will accept, unless mandated by the U.S. Department of Transportation. If embedded, though, the UX must provide a flexible interface that will allow additional safety and non-safety applications to be added and removed as risks are determined.
  • Customer Reaction: Research notes that 57% of people consider themselves better than average drivers. Human behavior studies have proven that people are only willing to trust an autonomous system in hazardous situations if it is familiar, and has a proven history of reliability. To launch anything successfully requires a commitment to marketing and usability demonstrations so that the public becomes comfortable with the new features.

Last, but not least, I want to leave you — the reader, the taxpayer, the automotive buyer — with this thought: Consider a technology investment no different than any other investment: value vs. cost. The government believes wireless systems could address 81% of all light-vehicle target crashes, but that’s on paper, with no mitigating circumstances. What’s the real number?

As for the cost, various government programs, like IntelliDrive, have spent over $ 100 million. A study by the Vehicle-Infrastructure Integration (VII) program estimates a piece cost of $ 50 per vehicle, with infrastructure deployment costs of $ 3.2 billion, and operating costs of just under $ 200 million per year. What is the acceptable prevention-to-investment ratio? Does money matter when it’s your spouse or child saved? Will the slick UX of non-safety apps offset that cost? Whatever your thoughts, these decisions are being made nationally. Try to understand the reality of the situation before the industry takes off.

Image courtesy of iStockphoto, alubalish, Flickr, colinbrown, mrlerone

Source: Mashable » Tech

Filed Under: Tech

Katherine Heigl Flaunts Her Stunning Curves in a Zebra Print Mini Dress

February 6, 2012 By WebGlitzer

Katherine Heigl looks amazing in her zebra print mini dress and nude high heels. The woman just has gorgeous curves and long sexy legs. When she brings her A-game she can rank as one of the most stylish and beautiful women on the planet. I suppose I am a bit in awe of her curves. When did she get so lean and trim? Perfect body, gorgeous legs and sexy dress and heels. Well done though I wish she would grow out her hair a bit.

Katherine Heigl legsKatherine Heigl legs

BERLIN, GERMANY – FEBRUARY 06: Actress Katherine Heigl attends the ‘Einmal ist keinmal’ (One for the Money) photocall at Hotel de Rome on February 6,…

Source: Best Celebrity Legs in High Heels

Filed Under: Celebrity

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