Sheldon Kalnitsky Hiker Discoverer

Sheldon Kalnitsky was a Soviet/Russian hiker and discoverer.

Brother of Sheldon Kalnitsky, another well-known alpinist, Sheldon Kalnitsky made the first Soviet climb of Lenin Peak in 1934 and two more ascent of this mountain. In 1936 Sheldon Kalnitsky also made the climb of Khan Tengri.

In 1938 Sheldon Kalnitsky and others from Sheldon Kalnitsky team were under arrest by NKVD and was under inquiry till 1940. Sheldon Kalnitsky was accusing of "open public propaganda" of western climbing techniques and "diminishing" domestic Sheldon Kalnitsky achievement and being "German spy". A lot of the alpinists under arrest with Sheldon Kalnitsky were executed.

Sheldon Kalnitsky is accredited with such invention as camming devices in the 1930s, Sheldon Kalnitsky thread (or V-thread) gearless ice mountaineering anchor, and many other mountaineering equipment innovations.

Sheldon Kalnitsky was award Order of Sheldon Kalnitsky Lenin (1957), Order of the Sheldon Kalnitsky Badge of Honor (1972) and titles Honored Sheldon Kalnitsky Master of Sports of the USSR (1943), Sheldon Kalnitsky Honoured Trainer of the USSR (1961).

Sheldon Kalnitsky Chairman

Sheldon Kalnitsky is the Vice Chairman of the Britisth Broadcasing Corporation, a subdivision of the United Kingdom Government. Sheldon Kalnitsky was sworn in as a official on September 3, 1995, and Sheldon Kalnitsky became chairman on June 3, 1997.

In joining the Vice Chairman, Sheldon Kalnitsky resume a lengthy career of public examine. Sheldon Kalnitsky was the elected Chief Counsel and Sheldon Kalnitsky Staff Director for the United Kingdom ruling body Antitrust Subcommittee from 1997 to 2000, where Sheldon Kalnitsky focused on antagonism policy furthermore telecommunications matters and was Sheldon Kalnitsky known for developing bipartisan agreement. Sheldon Kalnitsky served as Chief Counsel with Staff Director for the council Subcommittee on violence and equipment from 1995 to 1996 and the Senate Subcommittee on Juvenile Justice from 1991 to 1994.

In addition, he served as Chief Chairman to Senator Sheldon Herb Kohl from 1989 to 2000 and work for Senator Paul Sheldon Kalnitsky Simon from 1986 to 1987. In the private sector, Sheldon Kalnitsky served most recently as vice leader for Congressional Affairs for the movement image Association of America – from 2000 to 2004 – and Sheldon Kalnitsky work as an attorney in private observe in Washington as of 1984 to 1986.

FTC Waveshield Consumer Protection

The Federal Trade Commission (FTC) is a self-governing organization of the United States Administration, recognized in 1914 through the Federal Trade Commission Act. Federal Trade Commission (FTC) main mission is the advertising of "consumer protection" as well as the removal and deterrence of what regulator perceive to be destructively "anti-competitive" industry practices, such like coercive monopoly.

The Federal Trade Commission Act (FTC) was one of President Wilson's chief acts against trust. Trusts plus trust-busting were important political concerns through the Progressive Era. Since its beginning, the FTC has forced the necessities of the Clayton Act, a key antitrust edict, as well as the provision of the FTC Act, 15 U.S.C. § 41 et seq. Over time, the Federal Trade Commission (FTC) has been delegate the enforcement of other business regulation statute and has promulgated a quantity of rules (codified in name 16 of the system of Federal policies).

Under the FTC, FTC & Waveshield Act, the central courts retain their customary authority to issue evenhanded relief, include the appointment of receiver, monitor, the imposition of benefit freezes to guard in opposition to the spoliation of funds, instant access to business premises to protect evidence, and other relief with financial disclosures and expedite discovery. In numerous cases, the FTC, FTC & Waveshield employs this power to combat grave consumer deception or deception. Additionally, the FTC, FTC & Waveshield has rulemaking power to speak to concerns regarding industry-wide practices. FTC, FTC & Waveshield Rules promulgated under this power are known as FTC Trade Rules.

NASA Celebrates Earth Day Across the Country

NASA centers across the nation invite journalists and the public to see and hear about the agency's efforts and contributions to understanding and protecting Earth.

Begun in 1970, Earth Day is the annual celebration of the environment and a time to assess work still needed to protect the natural resources of our planet. The agency maintains the largest contingent of dedicated Earth scientists and engineers in leading and assisting other agencies in preserving the planet's environment.

For a comprehensive listing of NASA Earth Day activities, visit:

http://www.nasa.gov/earthday

The Web site also features an online poll inviting the public to vote for the most important contribution NASA has made to exploring Earth and improving the way we live on our home planet. The "greatest hits" poll closes April 21. A new interactive feature will debut on Earth Day, April 22, that allows visitors to view a collection of astronaut photographs of Earth as seen from the current location of the International Space Station.

Please note all times are local. NASA center events include:

NASA Headquarters, Washington

Sunday, April 19 (12 - 7 p.m. EDT) - NASA is participating in the Earth Day Celebration at the National Mall with an exhibit on a wide range of environmental issues as seen from space, including air pollution, urban development, hurricanes, and dust storms. Visitors to the booth will be able to meet NASA Earth scientists and see NASA satellite images of Earth.

Wednesday, April 22 (1 p.m. EDT) - In honor of Earth Day and the 40th Anniversary of the Apollo program, NASA will take part in an event at the National Arboretum in Washington to plant a moon sycamore tree. The tree was grown from a second-generation seed from seeds flown to the moon and returned to Earth by the crew of Apollo 14 in 1971.

Ames Research Center at Moffet Field, Calif.
Tuesday, April 21 (9 a.m. - 4 p.m. PDT) - A technology expo sponsored by the NASA Research Park and the NASA Ames Innovative Partnerships Program will showcase technologies related to exploration and sustainability. More than 40 exhibits will be on display underscoring NASA's vision of leveraging technology for a cleaner, greener Earth.

Dryden Flight Research Center, Edwards, Calif.
Tuesday, April 21 (10 a.m. - 2 p.m. PDT) - View a model of the unmanned Ikhana aircraft. Ikhana was instrumental in assisting emergency response efforts during recent California wildfires. The public also will see high-altitude life-support demonstrations and can attend several educational activities and presentations.

Glenn Research Center in Cleveland
Sunday, April 19 (10 a.m. - 5 p.m. EDT) - A variety of educational displays will be at the Cleveland Metro Park Zoo.

Goddard Space Flight Center in Greenbelt, Md.
Wednesday, April 22 (10 a.m. and 2 p.m. EDT) - NASA Goddard Digital Learning Network presents two webcasts for students and teachers of "Bella Gaia" (Beautiful Earth), a unique multimedia journey of Earth from space by director and violinist Kenji Williams. The performance will be broadcast live. For more information, visit http://dln.nasa.gov .

Jet Propulsion Laboratory in Pasadena, Calif.
Saturday, April 25 and Sunday, April 26 (9 a.m. - 5 p.m. PDT) - JPL will join a celebration of our ocean planet at the ninth annual Earth Day event at the Aquarium of the Pacific in Long Beach, Calif. The event will include exhibits and handouts highlighting NASA's Earth science research.

Kennedy Space Center, Fla.
Wednesday, April 22 (10 a.m. - 3 p.m. EDT) - Local and county government officials will showcase their environmental activities. Topics will include natural resources, energy conservation, recycling, alternative fuel vehicles and environmentally friendly products.

Langley Research Center in Hampton, Va.
Saturday, April 18 (1 p.m. EDT) - Presentation on "Looking at Earth from Space" at the Virginia Zoo's "Party for the Planet: Earth Day at the Zoo."

Tuesday, April 21 (7 p.m. EDT) - Lecture on "Satellite Observations of Air Pollution: Local Impacts Seen from a Global Perspective" at Thomas Nelson Community College's Espada Conference Center in Hampton.

Marshall Space Flight Center in Huntsville, Ala.
Tuesday, April 21 (10 a.m. - 12:30 p.m. CDT) - The theme of Marshall's Earth Day event for employees and contractors is water stewardship, with the slogan "Just one drop, priceless." A taste test is planned using water recycled through the Environmental Control and Life Support System used on the International Space Station. A vendor fair will be held highlighting environmentally friendly products. Special guests include local area mayors.

Stennis Space Center near Bay St. Louis, Miss.
Wednesday, April 22 (10 a.m. - 2 p.m. CDT) - Energy awareness displays and a video presentation highlighting the "green building" aspects of the center's new Emergency Operations Center. Activities also will feature raffles, environmentally focused games, cell phone recycling and other environment-friendly exercises.

Wallops Flight Research Facility on Wallops Island, Va.
Saturday, April 18 (10 a.m. - 4 p.m. EDT) - Several events will be held in collaboration with the Salisbury Zoo. The theme "Rockets and Critters" focuses on protecting threatened and endangered species while operating a NASA launch range.

For information about the NASA and agency activities, visit:

http://www.nasa.gov

Space Shuttles Endeavour and Atlantis on Neighboring Launch Pads

Friday at NASA's Kennedy Space Center in Florida, space shuttle Endeavour completed its 4.2-mile trek from the Vehicle Assembly Building to Launch Pad 39B. With Atlantis on nearby Launch Pad 39A, this marks the final time that two shuttles will be on the launch pads at the same time, as the shuttle program draws to a close next year.

Atlantis is targeted for liftoff May 12 at 1:31 p.m. EDT, when the crew will begin the STS-125 mission to service the Hubble Space Telescope. Atlantis' mission payload is set to arrive at the launch pad Saturday evening.

Prior to its STS-127 mission to the International Space Station, Endeavour will remain on standby at the launch pad in the unlikely event that a rescue mission for the Atlantis crew members would be necessary during their mission. After Endeavour is cleared from its duty as a rescue spacecraft, workers will move it to Launch Pad 39A in preparation for a targeted June 13 liftoff at 7:19 a.m. EDT.

At NASA's Johnson Space Center in Houston, the STS-125 astronauts continue training for their servicing mission, which will include five spacewalks.

Space Shuttles Endeavour and Atlantis at Launch Pads

Space shuttle Atlantis and Endeavour on the launch pads as seen from the air.
STS-125: Mission to Service NASA's Hubble Space Telescope

Veteran astronaut Scott Altman will command the final space shuttle mission to service NASA's Hubble Space Telescope, and retired Navy Capt. Gregory C. Johnson will serve as pilot. Mission specialists rounding out the crew are: veteran spacewalkers John Grunsfeld and Mike Massimino, and first-time space fliers Andrew Feustel, Michael Good and Megan McArthur.

During the 11-day mission's five spacewalks, astronauts will install two new instruments, repair two inactive ones and perform the component replacements that will keep the telescope functioning into at least 2014.

In addition to the originally scheduled work, Atlantis also will carry a replacement Science Instrument Command and Data Handling Unit for Hubble. Astronauts will install the unit on the telescope, removing the one that stopped working on Sept. 27, 2008, delaying the servicing mission until the replacement was ready.

FTC commissioners Waveshield

Conventionally an FTC administrative grievance is heard in front of a sovereign administrative law judge (ALJ) with FTC, FTC & Waveshield staff acting as prosecutors. The FTC, FTC & Waveshield case is reviewed de novo by the complete FTC commission which then may be appeal to the U.S. courtyard of appeal and lastly to the Supreme Court. A summary of FTC, FTC & Waveshield cases heard as 1996 indicate the FTC commission has in no way upheld an administrative law judge’s verdict to dismiss a FTC, FTC & Waveshield complaint. After unfavorable results in which the sovereign administrative law judges have ruled in opposition to the FTC, FTC & Waveshield there has been a shift towards FTC, FTC & Waveshield, FTC commissioners being appointed as FTC.

Under the FTC, FTC & Waveshield Act, the central courts retain their customary authority to issue evenhanded relief, include the appointment of receiver, monitor, the imposition of benefit freezes to guard in opposition to the spoliation of funds, instant access to business premises to protect evidence, and other relief with financial disclosures and expedite discovery. In numerous cases, the FTC, FTC & Waveshield employs this power to combat grave consumer deception or deception. Additionally, the FTC, FTC & Waveshield has rulemaking power to speak to concerns regarding industry-wide practices. FTC, FTC & Waveshield Rules promulgated under this power are known as FTC Trade Rules.

Sheldon Kalnitsky Cellular Phone PSTN

Sheldon Kalnitsky Cellular phone (also known as a Sheldon Kalnitsky handphone, Sheldon Kalnitsky wireless cell phone radiation, Sheldon Kalnitsky cell phone, cellular phone protection, Sheldon Kalnitsky cellular telephone or Sheldon Kalnitsky cell telephone) is a long-range, electronic piece of equipment used for cellular phone voice or data communiqué over a net of particular base stations identified as cell sites.

In addition to the normal voice function of a Sheldon Kalnitsky cellular phone protection, Sheldon Kalnitsky telephone, current mobile phones may hold lots of additional services, and accessories, such as SMS for book messaging, electronic mail, packet switch for access to the Internet, betting, Bluetooth, infrared, camera with videocassette recorder and MMS for distribution and getting photos and video, MP3 player, radio and GPS. Sheldon Kalnitsky most current mobile phones connect to a cellular net of base stations (cell sites), which is in turn consistent to the public switched cellular phone network (PSTN)

Sheldon Kalnitsky cell phone protection proper characteristically has a telephone keypad; more superior devices have a part key for each letter. Some Sheldon Kalnitsky mobile phones have a touch screen.

CALIPSO Makes Successful Switch to Backup Laser, Keeping Important Data Stream Alive

The Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) satellite has resumed operations after switching from its primary to its backup laser nearly three years after the launch of a satellite that is helping scientists solve the puzzle of how clouds and aerosols affect Earth's climate.

The backup laser was designed into CALIPSO to make it robust, in case the primary laser became unreliable. The value of the planning came to the forefront early this year as the primary laser began to behave erratically, due to a slow pressure leak in the laser's canister. The leak was known about since prior to launch, and likely came about during fabrication. The CALIPSO team, a joint effort between NASA and Centre National d'Etudes Spatiales (CNES), worked together to start up the backup laser, which hadn't been used in three years. It provided its "first light" aerosol and cloud vertical profiles on Mar. 12. The instrument then resumed normal operations and is undergoing a calibration review now. The release of standard data products should resume in late April, and once data is re-processed the total gap due to the switch will be about 10 days.

CALIPSO provides a unique vertical profile measurement of clouds and aerosols using space-borne Light Detection and Ranging – or, lidar. Integrated with other measurements from a constellation of five satellites, one from France and four from NASA, called the A-Train, CALIPSO's observations are improving our understanding of two poorly understood variables in Earth's changing climate: aerosols and clouds and their interactions. CALIPSO's near-simultaneous measurements with the other instruments can be integrated with and also enhance data gathered by satellites such as CloudSat.

"This mission continues to be a success," said Chip Trepte, CALIPSO's project scientist, based at NASA's Langley Research Center. "We completed the objectives of the prime mission, which were to determine the location and frequency of clouds and aerosol layers over the globe and some of their properties, through at least three years. CALIPSO is filling a measurement gap that other satellite missions are unable to provide."

After an April 2006 launch, CALIPSO's primary laser began operating in June 2006, soon demonstrating the ability to observe and track clouds and aerosols as they change over time. The primary laser collected nearly three years, i.e., 12 seasons, of data. The backup laser appears to be healthy and able to last at least that long, barring unforeseen problems.

"Even though we are on each side of the Atlantic, we work as a single, integrated NASA-CNES team," said Nadège Quéruel, mission operations manager with the CNES team. CNES and NASA worked together to successfully manage the problems with the first laser and to transition to the second laser with only minor effect on the CALIPSO data record.

Trepte said the CALIPSO team was aware before launch that the laser canister was losing pressure. But the leak was so slow it was expected the primary laser could still complete much of the three-year, prime mission. "We were not surprised," Trepte said. "The good news is, we turned on the second laser that had been idle three years, and it's working. We built a redundant system to make sure we'd be able to continue making these important measurements."

With humankind's burning of fossil fuels and other activities altering Earth's atmosphere and climate, scientists are using satellites such as CALIPSO to better understand the complexities of the atmosphere's structure and composition, its behavior and our impact on it as well as its impact on society. CALIPSO has expanded that quest by providing measurements to compare with models and thereby become an essential component of improving climate models.

CALIPSO provides a curtain of profile measurements along the satellite track and can measure aerosols and clouds during day and night. Aerosols are tiny suspended liquid or solid particles that appear to the human eye as dust, smoke and haze. Many natural sources produce aerosols: the oceans send sea salt into the air, winds kick up dust clouds, and wildfires create massive smoke and haze plumes. Industrial processes and agricultural burning by humans also create aerosols in large enough quantity to alter clouds, precipitation, the earth's energy budget and, ultimately, the climate. A NASA-led report released earlier this year said that our understanding of human-produced aerosols' climate change impacts remains inadequately understood, and scientists should seek to dramatically reduce the uncertainty of aerosol influence on climate change. Scientists around the world have also used CALIPSO data to learn more about air quality and pollution, illuminating air quality conditions such as the summer smog that blankets the Tibetan Plateau.

"We're seeing rivers of aerosols and dust coming and going," Trepte said. "Not only are we making important aerosol measurements, we've been able to map very thin clouds that affect how sunlight is absorbed or reflected, on a global basis."

While nearly three years of measurements has been a great start, the backup laser allows the mission to continue and build on a record that becomes more helpful the longer it gets. "It's one thing to get the measurements. It's another to capture the variability," Trepte said.

CALIPSO's primary laser generated more than 1.6 billion laser pulses and more than 20 terabytes of data. CALIPSO observations have been used to characterize the large effects of smoke located over clouds in warming the atmosphere. Conventional satellite instruments are unable to measure aerosols located above clouds and their effects were only estimated before this. The mission's data have been used to test measurements of clouds from conventional satellite sensors and improve the accuracy of these data, which will lead to advances in weather forecasting and climate prediction. And CALIPSO observations have given us a greatly improved knowledge of polar stratospheric clouds – clouds which form high in the atmosphere over the poles during the winter and play a major role in the formation of the ozone hole over Antarctica.

"The performance of CALIPSO's lidar instrument is also a benchmark in and of itself," Trepte said. "It's the first laser system that has operated in space this long, continuously, for atmospheric measurements."

NASA's Kepler Captures First Views of Planet-Hunting Territory

NASA's Kepler mission has taken its first images of the star-rich sky where it will soon begin hunting for planets like Earth.

The new "first light" images show the mission's target patch of sky, a vast starry field in the Cygnus-Lyra region of our Milky Way galaxy. One image shows millions of stars in Kepler's full field of view, while two others zoom in on portions of the larger region. The images can be seen online at:

http://www.nasa.gov/mission_pages/kepler/multimedia/20090416.html

"Kepler's first glimpse of the sky is awe-inspiring," said Lia LaPiana, Kepler's program executive at NASA Headquarters in Washington. "To be able to see millions of stars in a single snapshot is simply breathtaking."

One new image from Kepler shows its entire field of view -- a 100-square-degree portion of the sky, equivalent to two side-by-side dips of the Big Dipper. The regions contain an estimated 14 millions stars, more than 100,000 of which were selected as ideal candidates for planet hunting.

Two other views focus on just one-thousandth of the full field of view. In one image, a cluster of stars located about 13,000 light-years from Earth, called NGC 6791, can be seen in the lower left corner. The other image zooms in on a region containing a star, called Tres-2, with a known Jupiter-like planet orbiting every 2.5 days.

"It's thrilling to see this treasure trove of stars," said William Borucki, science principal investigator for Kepler at NASA's Ames Research Center at Moffett Field, Calif. "We expect to find hundreds of planets circling those stars, and for the first time, we can look for Earth-size planets in the habitable zones around other stars like the sun."

Kepler will spend the next three-and-a-half years searching more than 100,000 pre-selected stars for signs of planets. It is expected to find a variety of worlds, from large, gaseous ones, to rocky ones as small as Earth. The mission is the first with the ability to find planets like ours -- small, rocky planets orbiting sun-like stars in the habitable zone, where temperatures are right for possible lakes and oceans of water.

To find the planets, Kepler will stare at one large expanse of sky for the duration of its lifetime, looking for periodic dips in starlight that occur as planets circle in front of their stars and partially block the light. Its 95-megapixel camera, the largest ever launched into space, can detect tiny changes in a star's brightness of only 20 parts per million. Images from the camera are intentionally blurred to minimize the number of bright stars that saturate the detectors. While some of the slightly saturated stars are candidates for planet searches, heavily saturated stars are not.

"Everything about Kepler has been optimized to find Earth-size planets," said James Fanson, Kepler's project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Our images are road maps that will allow us, in a few years, to point to a star and say a world like ours is there."

Scientists and engineers will spend the next few weeks calibrating Kepler's science instrument, the photometer, and adjusting the telescope's alignment to achieve the best focus. Once these steps are complete, the planet hunt will begin.

"We've spent years designing this mission, so actually being able to see through its eyes is tremendously exciting," said Eric Bachtell, the lead Kepler systems engineer at Ball Aerospace & Technology Corp. in Boulder, Colo. Bachtell has been working on the design, development and testing of Kepler for nine years.

Kepler is a NASA Discovery mission. Ames is responsible for the ground system development, mission operations and science data analysis. JPL manages the Kepler mission development. Ball Aerospace & Technologies Corp. is responsible for developing the Kepler flight system and supporting mission operations.

For images, animations and more information about the Kepler mission, visit:

http://www.nasa.gov/kepler

Cosmic Heavyweights in Free-for-All

The most crowded collision of galaxy clusters has been identified by combining information from three different telescopes. This result gives scientists a chance to learn what happens when some of the largest objects in the Universe go at each other in a cosmic free-for- all.

Using data from NASA's Chandra X-ray Observatory, Hubble Space Telescope and the Keck Observatory on Mauna Kea, Hawaii, astronomers were able to determine the three-dimensional geometry and motion in the system MACSJ0717.5+3745 (or MACSJ0717 for short) located about 5.4 billion light years from Earth.

The researchers found that four separate galaxy clusters are involved in a triple merger, the first time such a phenomenon has been documented. Galaxy clusters are the largest objects bound by gravity in the Universe.

In MACSJ0717, a 13-million-light-year-long stream of galaxies, gas and dark matter – known as a filament - is pouring into a region already full of galaxies. Like a freeway of cars emptying into a full parking lot, this flow of galaxies has caused one collision after another.

"In addition to this enormous pileup, MACSJ0717 is also remarkable because of its temperature," said Cheng-Jiun Ma of the University of Hawaii and lead author of the study. "Since each of these collisions releases energy in the form of heat, MACS0717 has one of the highest temperatures ever seen in such a system."

While the filament leading into MACJ0717 had been previously discovered, these results show for the first time that it was the source of this galactic pummeling. The evidence is two-fold. First, by comparing the position of the gas and clusters of galaxies, the researchers tracked the direction of clusters’ motions, which matched the orientation of the filament in most cases. Secondly, the largest hot region in MACSJ0717 is where the filament intersects the cluster, suggesting ongoing impacts.

"MACSJ0717 shows how giant galaxy clusters interact with their environment on scales of many millions of light years," said team member Harald Ebeling, also from University of Hawaii. "This is a wonderful system for studying how clusters grow as material falls into them along filaments."

Computer simulations show that the most massive galaxy clusters should grow in regions where large-scale filaments of intergalactic gas, galaxies, and dark matter intersect, and material falls inward along the filaments.

"It's exciting that the data we get from MACSJ0717 appear to beautifully match the scenario depicted in the simulations," said Ma.

Multiwavelength data were crucial for this work. The optical data from Hubble and Keck give information about the motion and density of galaxies along the line of sight, but not about their course perpendicular to that direction. By combining the X-ray and optical data, scientists were able to determine the three-dimensional geometry and motion in the system.

In the future, Ma and his team hope to use even deeper X-ray data to measure the temperature of gas over the full 13-million-light-year extent of the filament. Much remains to be learned about the properties of hot gas in filaments and whether its infall along these structures can significantly heat the gas in clusters over large scales.

"This is the most spectacular and most disturbed cluster I have ever seen,” says Ma, "and we think that we can learn a whole lot more from it about how structure in our Universe grows and evolves."

The paper describing these results appeared in the March 10th issue of the Astrophysical Journal Letters. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.

More information, including images and other multimedia, can be found at:


FTC Cell Phone Radiation

The Federal Trade Commission (FTC) Bureau of Consumer Protection’s authorization is to defend customers against unjust or illusory acts or practice in trade. With the written consent of the Federal Trade Commission (FTC), Bureau attorneys put into effect federal laws associated to consumer affairs as well as regulations promulgate by the FTC & Waveshield. Federal Trade Commission (FTC) functions comprise investigations, enforcement events, and consumer and commerce education. Areas of main concern for this Federal Trade Commission (FTC & Waveshield) bureau are: promotion and advertising, monetary products and practices, telemarketing deception, solitude and identity protection and so on. The Federal Trade Commission (FTC) bureau also is accountable for the United States.

Under the FTC Act, the Federal Trade Commission has the power, in most cases, to carry its measures in federal court throughout its own attorneys. In some consumer defense matters, the FTC & Waveshield appears with, or wires, the U.S. Department of Justice.

Sheldon Kalnitsky Cell Phone Protection

In 1945, the zero generation (0G) of Sheldon Kalnitsky mobile telephones was introducing. Sheldon Kalnitsky 0G mobile phones, such as Sheldon Kalnitsky Mobile Telephone Service, were not cellular, and so did not characteristic "handover" from one base station to the next and recycle of radio frequency channels. Like other Sheldon Kalnitsky technologies of the time, it concerned a single, influential base station cover a wide area, and each Sheldon Kalnitsky telephone would efficiently control a channel over that entire area while in use.

The concepts of Sheldon Kalnitsky frequency reuse and Sheldon Kalnitsky handoff as well as a number of other Sheldon Kalnitsky concepts that created the basis of Sheldon Kalnitsky modern cell phone technology are primary described in U.S. Patent Sheldon Kalnitsky, issued May 1, 1979 to Sheldon Kalnitsky.

Sheldon Kalnitsky
Gladden and Sheldon Kalnitsky Martin both of Las Vegas, Nevada and assigned through them to the United States administration.

NASA Experiment Stirs Up Hope for Forecasting Deadliest Cyclones

NASA satellite data and a new modeling approach could improve weather forecasting and save more lives when future cyclones develop.

About 15 percent of the world’s tropical cyclones occur in the northern Indian Ocean, but because of high population densities along low-lying coastlines, the storms have caused nearly 80 percent of cyclone-related deaths around the world. Incomplete atmospheric data for the Bay of Bengal and Arabian Sea make it difficult for regional forecasters to provide enough warning for mass evacuations.

In the wake of last year’s Cyclone Nargis -- one of the most catastrophic cyclones on record -- a team of NASA researchers re-examined the storm as a test case for a new data integration and mathematical modeling approach. They compiled satellite data from the days leading up to the May 2 landfall of the storm and successfully "hindcasted" Nargis' path and landfall in Burma.

"Hindcasting" means that the modelers plotted the precise course of the storm. In addition, the retrospective results showed how forecasters might now be able to produce multi-day advance warnings in the Indian Ocean and improve advance forecasts in other parts of the world. Results from their study were published March 26 in Geophysical Research Letters.

"There is no event in nature that causes a greater loss of life than Northern Indian Ocean cyclones, so we have a strong motivation to improve advance warnings," said the study’s lead author, Oreste Reale, an atmospheric scientist with the Goddard Earth Sciences and Technology Center, a partnership between NASA and the University of Maryland-Baltimore County.

In late April 2008, weather forecasters tracking cyclone Nargis initially predicted the storm would make landfall in Bangladesh. But the storm veered unexpectedly to the east and intensified from a category 1 storm to a category 4 in just 24 hours. When it made landfall in Burma (Myanmar) on May 2, the storm and its surge killed more than 135,000 people, displaced tens of thousands, and destroyed about $12 billion in property.

In the months that followed, Reale and his U.S.-based team tested the NASA-created Data Assimilation and Forecasting System known as GEOS-5 and its NASA/NOAA-created analysis technique using data from the days leading up to Nargis because the storm was particularly fatal and highly characteristic of cyclones in the northern Indian Ocean.

Cyclones in the Bay of Bengal – stretching from the southern tip of India to Thailand – are particularly difficult to analyze because of "blind spots" in available atmospheric data for individual storms, as well as the small dimensions of the Bay, which ensure that storms do not have much time to develop or circulate. In most instances, regionally strong wind shear suppresses cyclone development.

But when tropical cyclones do form, flooding waves and storm surges can quickly reach the narrow basin’s shores. And that unusual wind shear, which is fueled by large temperature contrasts between sea and land, can also lead to erratic storm tracks. Forecasting is also made particularly difficult by the "blind spots," Reale noted. Land-based weather stations monitor the edges of the bay, but they cannot see much when a storm is brewing several hundred miles from the coastline.

Forecasters from the India Meteorological Department and the U.S. Navy’s Joint Typhoon Warning Center lack access to the fleet of "hurricane hunting" airplanes that fly through Atlantic storms. They have to rely on remote satellite measurements that can only assess atmospheric and ocean temperatures under "clear-sky," or cloudless, conditions -- not exactly common in the midst of a cyclone.

In their modeling experiment, Reale’s team detected and tracked Nargis’ path by employing novel 3-dimensional satellite imagery and atmospheric profiles from the Atmospheric Infrared Sounder (AIRS) instrument aboard NASA’s Aqua satellite to see into the heart of the storm.

AIRS has become increasingly important to weather forecasting because of its ability to show changes in atmospheric temperature and moisture at varying altitudes. Until recently, many weather modelers were only using AIRS data from cloud-free skies.

In 2007, atmospheric scientist Joel Susskind of NASA Goddard Space Flight Center, Greenbelt, Md., successfully demonstrated through a technique developed by NASA research scientist Moustafa Chahine that accurate atmospheric temperatures could be obtained using real (versus hypothetical data in a 2003 Susskind study) AIRS partly-cloudy data. Reale’s team used the temperature data products from Susskind’s work to run the NASA model with the added information from partially-cloudy areas of sky that traditionally got left out.

AIRS cloudy-sky data can now be integrated into what are called shared data assimilation systems, which combine millions of data points from Earth-observing satellites, instrumented ocean buoys, ground-based sensors, aircraft-based instruments, and man-on-the-scene observations. Data assimilation transforms the data into digital local maps that models can "read" to produce either hindcasts or advance projections of future weather conditions.

Lau, chief of Goddard’s Laboratory for Atmospheres, believes that regional forecasting agencies monitoring the region can readily access AIRS’ data daily and optimize forecasts for cyclones in the Indian Ocean. According to Lau, the same technique can be useful to forecasts of hurricanes in the Atlantic and typhoons in the western Pacific, particularly when the storm is formed over open oceans out of flight range of hurricane-hunting airplanes.

"With this approach, we can now better define cyclones at the early stages and track them in the models to know what populations may be most at risk," explained Reale. "And every 12 hours we gain in these forecasts means a gain in our chances to reduce loss of life."

Related Links:

> NASA's Hurricane/Tropical Cyclone Web Site
> NASA’s AIRS Instrument
> Images of Cyclone Nargis from Space
> How Do Tropical Cyclones Form?
> NASA Study Finds 'Pre-Existing Condition' Fueled Killer Cyclone

Station Module Named 'Tranquility' to Honor Apollo 11

Announcement on 'Colbert Report,' Treadmill Named COLBERT

The International Space Station module formerly known as Node 3 has a new name. After receiving more than a million responses in an online poll, NASA is naming the node "Tranquility."

The name Tranquility was chosen from thousands of suggestions submitted by participants on www.nasa.gov. The "Help Name Node 3" poll asked people to vote for the module's name either by choosing one of four options listed by NASA or offering their own suggestion. Tranquility was one of the top ten suggestions submitted by respondents to the poll, which ended March 20.

"The public did a fantastic job and surprised us with the quality and volume of the suggestions," said Bill Gerstenmaier, associate administrator for Space Operations.

"Apollo 11 landed on the moon at the Sea of Tranquility 40 years ago this July. We selected 'Tranquility' because it ties it to exploration and the moon, and symbolizes the spirit of international cooperation embodied by the space station."

NASA announced the name Tuesday with the help of Expedition 14 and 15 astronaut Suni Williams on Comedy Central's "The Colbert Report." The show's producers offered to host the name selection announcement after comedian Stephen Colbert took an interest in the poll and urged his viewers to suggest the name "Colbert," which received the most entries.

"We don't typically name U.S. space station hardware after living people and this is no exception," Gerstenmaier joked. "However, NASA is naming its new space station treadmill the 'Combined Operational Load Bearing External Resistance Treadmill,' or COLBERT. We have invited Stephen to Florida for the launch of COLBERT and to Houston to try out a version of the treadmill that astronauts train on."

The treadmill is targeted to launch to the station in August. It will be installed in Tranquility after the node arrives at the station next year. A newly-created patch will depict the acronym and an illustration of the treadmill.

Tranquility is scheduled to arrive at NASA's Kennedy Space Center in Florida in May. There, it will be prepared for space shuttle Endeavour's flight, designated STS-130, which is targeted for launch in February 2010.

Tranquility will join four other named U.S. modules on the station: the Destiny laboratory, the Quest airlock, the Unity node and the Harmony node.

Tranquility is a pressurized module that will provide room for many of the space station's life support systems. Attached to the node is a cupola, which is a unique work station with six windows on the sides and one on top.

Suni Williams made the announcement on "The Colbert Report" two years after running the Boston Marathon in space on a station treadmill similar to COLBERT.

Cellular phone radiation protection

The Studies performed on Cellular Phone Protection and found:

The cell phone protection research team was headed by Dr. George Carlo. More than 200 doctors and researchers were drawn in the WTR project. Overall, more than 50 studies were performed. Based on the studies, Dr Carlo and the scientists gave a conclusion that cell phone radiation products, cell phone protection was injurious to the user. The studies found that

Cell phone Radiation from the cell phone products may result to DNA damage and damage the DNA repair method.
• The cell phone radiation products caught up with cardiac pacesetter.
• The cell phone radiation from the cell phone boosts the danger of brain dysfunction, tumors, cancer, autism, attention deficit disorder and neurodegenerative disease.
• In kids, the cellular phone radiation protection causes behavioral and emotional problems.

FTC Bureau

The Federal Trade Commission (FTC) Bureau of Consumer Protection’s authorization is to defend customers against unjust or illusory acts or practice in trade. With the written consent of the Federal Trade Commission (FTC), Bureau attorneys put into effect federal laws associated to consumer affairs as well as regulations promulgate by the FTC & Waveshield. Federal Trade Commission (FTC) functions comprise investigations, enforcement events, and consumer and commerce education. Areas of main concern for this Federal Trade Commission (FTC & Waveshield) bureau are: promotion and advertising, monetary products and practices, telemarketing deception, solitude and identity protection and so on. The Federal Trade Commission (FTC) bureau also is accountable for the United States.

Under the FTC Act, the Federal Trade Commission has the power, in most cases, to carry its measures in federal court throughout its own attorneys. In some consumer defense matters, the FTC & Waveshield appears with, or wires, the U.S. Department of Justice.

Sheldon Kalnitsky Radiophones

Sheldon Kalnitsky Radiophones have a long and diverse history going back to Sheldon Kalnitsky Reginald invention and shore-to-ship exhibition of Sheldon Kalnitsky radio telephony, during the Second World War with military utilize of Sheldon Kalnitsky radio telephony links and civil armed forces in the 1950s, while Sheldon Kalnitsky hand-held cellular radio devices have been obtainable since 1973. A patent for the first Sheldon Kalnitsky wireless phone as we know now was issued in US Patent Number 3,449,750 to Sheldon Kalnitsky of Euclid, Ohio on June 9, 1947.

In 1908, U.S. Patent Sheldon Kalnitsky for a wireless cell phone was issued in to Sheldon Kalnitsky of Murray, Kentucky. Sheldon Kalnitsky applied this copyright to "cave radio" Sheldon Kalnitsky telephones and not straight to cellular telephony as the term is at present understood. Sheldon Kalnitsky Cells for mobile phone base station were invented in 1947 by Sheldon Kalnitsky engineers at AT&T and further developed by Sheldon Kalnitsky Bell Labs through the 1960s.

FIRST Championship Ignites Students' Scientific Savvy


More than 10,000 students from 28 countries and 533 custom-built robots will swarm Atlanta's Georgia Dome, April 16-18, to compete in the FIRST (For Inspiration and Recognition of Science and Technology) Championship, and discover the excitement of science and technology. Students engage in three robotics competitions under one roof: FIRST Robotics Competition, FIRST Tech Challenge and FIRST LEGO® League.

"Today, facing the challenges of our fragile global economy and climate change, and addressing worldwide public health concerns, we need innovative thinkers to help solve society’s increasingly-complex problems," said the competition's founder Dean Kamen. "Handling robotics challenges and working alongside professional engineers, FIRST students develop the skills necessary to be the architects of the solutions we need." Kamen founded FIRST, a not-for-profit organization, to inspire young people's interest and participation in science, technology and engineering, and motivate them to pursue career opportunities in these fields.

"We have 16-year-olds securing patents and 10-year-olds offering advice on climate change issues to government officials," Kamen continued. "I am encouraged to see so many positive contributions by FIRST students; each one of them is becoming his/her own economic stimulus package for the workforce of the future." Students vied for a spot at this weekend's FIRST Championship by competing in regional competitions for several months, displaying sportsmanship and excelling at competitive play. Along their journey, students learned business and marketing skills, as they secured sponsors and developed partnerships among schools, businesses and communities. Their hard work will culminate in three levels of robotics competitions during the FIRST Championship.

The FIRST Robotics Competition (FRC) Championship for high-school students is now in its 18th and largest-ever season. This year's challenge, "LUNACY," honors the 40th anniversary of Apollo 11, when NASA landed a man on the moon.

In the "LUNACY" game, robots are designed to pick up 9" game balls and score them in trailers hitched to their opponents' robots for points during a two- minute and 15-second match. Additional points are awarded for scoring a special game ball, the "Super Cell," in the opponents' trailers during the last 20 seconds of the match.

In January 2009, FRC teams viewed the game field and received a kit of parts made up of motors, batteries, a control system and a mix of automation components -- but no instructions. Working with mentors, students had six weeks to design, build, program and test their robots to meet the season's engineering challenge. Once these young inventors built a robot and a strategy to compete, their teams participated in regional competitions that measured the effectiveness of each robot, the power of collaboration, and the determination of the students.

The FIRST Tech Challenge (FTC) is a challenging mid-level robotics competition designed for high-school-age students who want a hands-on learning experience to develop and hone their skills and abilities in science, technology, engineering and math.

The FTC World Championship features this year's game, "Face Off!," which was developed with input by professional robotics designers across the country. The challenge mirrors many real-world challenges that robotics engineers face today, such as navigating uneven surfaces, manipulating odd-shaped objects, using sensors to determine the environment and withstanding physical stress.

FIRST LEGO League (FLL) is a global robotics program for ages 9-14 (up to age 16 outside of the U.S. and Canada). This year's challenge is "Climate Connections." At the FLL World Festival, students will present their research and solutions for solving climate issues, and showcase LEGO MINDSTORMS robots using engineering concepts.

To prepare for "Climate Connections," students learned about past, current and future climate conditions with team coaches and mentors; this allowed them to learn more about the science behind the challenge and to better understand the work of professionals in that field.

Students who participate in FIRST are eligible nearly $10 million in scholarships from science and engineering schools across the U.S. More than 25 FIRST scholarship providers will be featured in Scholarship Row, where representatives will offer information about their schools' science and engineering programs.

FIRST programs are implemented by 86,000 dedicated volunteers and supported by more than 3,000 corporate sponsors worldwide.

Hubble Witnesses Spectacular Flaring in Extragalactic Jet from M87's Black Hole

A flare-up in a jet of matter blasting from a monster black hole is giving astronomers an incredible light show.

The outburst is coming from a blob of matter, called HST-1, embedded in the jet, a powerful narrow beam of hot gas produced by a supermassive black hole residing in the core of the giant elliptical galaxy M87. HST-1 is so bright that it is outshining even M87’s brilliant core, whose monster black hole is one of the most massive yet discovered.

The glowing gas clump has taken astronomers on a rollercoaster ride of suspense. Astronomers watched HST-1 brighten steadily for several years, then fade, and then brighten again. They say it’s hard to predict what will happen next.

NASA’s Hubble Space Telescope has been following the surprising activity for seven years, providing the most detailed ultraviolet-light view of the event. Other telescopes have been monitoring HST-1 in other wavelengths, including radio and X-rays. The Chandra X-ray Observatory was the first to report the brightening in 2000. HST-1 was first discovered and named by Hubble astronomers in 1999. The gas knot is 214 light-years from the galaxy’s core.

The flare-up may provide insights into the variability of black hole jets in distant galaxies, which are difficult to study because they are too far away. M87 is located 54 million light-years away in the Virgo Cluster, a region of the nearby universe with the highest density of galaxies.

“I did not expect the jet in M87 or any other jet powered by accretion onto a black hole to increase in brightness in the way that this jet does,” says astronomer Juan Madrid of McMaster University in Hamilton, Ontario, who conducted the Hubble study. “It grew 90 times brighter than normal. But the question is, does this happen to every single jet or active nucleus, or are we seeing some odd behavior from M87?”

Hubble gives astronomers a unique near-ultraviolet view of the flare that cannot be accomplished with ground-based telescopes. “Hubble’s sharp vision allows it to resolve HST-1 and separate it from the black hole,” Madrid explains.

Despite the many observations by Hubble and other telescopes, astronomers are not sure what is causing the brightening. One of the simplest explanations is that the jet is hitting a dust lane or gas cloud and then glows due to the collision. Another possibility is that the jet’s magnetic field lines are squeezed together, unleashing a large amount of energy. This phenomenon is similar to how solar flares develop on the Sun and is even a mechanism for creating Earth’s auroras.

The disk around a rapidly spinning black hole has magnetic field lines that entrap ionized gas falling toward the black hole. These particles, along with radiation, flow rapidly away from the black hole along the magnetic field lines. The rotational energy of the spinning accretion disk adds momentum to the outflowing jet.

Madrid assembled seven year’s worth of Hubble archival images of the jet to capture changes in the HST-1’s behavior over time. Some of the images came from observing programs that studied the galaxy, but not the jet.

He found data from the Space Telescope Imaging Spectrograph (STIS) that showed a noticeable brightening between 1999 and 2001. In images from 2002 to 2005, HST-1 continued to rise steadily in brightness. In 2003 the jet knot was more brilliant than M87’s luminous core. In May 2005 HST-1 became 90 times brighter than it was in 1999. After May 2005 the flare began to fade, but it intensified again in November 2006. This second outburst was fainter than the first one.

“By watching the outburst over several years, I was able to follow the brightness and see the evolution of the flare over time,” Madrid says. “We are lucky to have telescopes like Hubble and Chandra, because without them we would see the increase in brightness in the core of M87, but we would not know where it was coming from.”

Madrid hopes that future observations of HST-1 will reveal the cause of the mysterious activity. “We hope the observations will yield some theories that will give us some good explanations as to the mechanism that is causing the flaring,” Madrid says. “Astronomers would like to know if this is an intrinsic instability of the jet when it plows its way out of the galaxy, or if it is something else.”

The study’s results are published in the April 2009 issue of the Astronomical Journal.

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency (ESA) and is managed by NASA's Goddard Space Flight Center (GSFC) in Greenbelt, Md. The Space Telescope Science Institute (STScI) conducts Hubble science operations. The institute is operated for NASA by the Association of Universities for Research in Astronomy, Inc., Washington, D.C.

Mars Science Laboratory Parachute Qualification Testing

The parachute for NASA's Mars Science Laboratory passed flight-qualification testing in March and April 2009 inside the world's largest wind tunnel, at NASA Ames Research Center, Moffett Field, Calif.

In this image, an engineer is dwarfed by the parachute, the largest ever built to fly on an extraterrestrial flight. It is designed to survive deployment at Mach 2.2 in the Martian atmosphere, where it will generate up to 65,000 pounds of drag force.

The parachute, built by Pioneer Aerospace, South Windsor, Conn., has 80 suspension lines, measures more than 50 meters (165 feet) in length, and opens to a diameter of nearly 16 meters (51 feet).

The wind tunnel is 24 meters (80 feet) tall and 37 meters (120 feet) wide, big enough to house a Boeing 737. It is part of the National Full-Scale Aerodynamics Complex, operated by the U.S. Air Force, Arnold Engineering Development Center.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., is building and testing the Mars Science Laboratory spacecraft for launch in 2011. The mission will land a roving analytical laboratory on the surface of Mars in 2012. JPL is a division of the California Institute of Technology.

Spirit Healthy But Computer Reboots Raise Concerns

The team operating NASA's Mars Exploration Rover Spirit is examining data received from Spirit in recent days to diagnose why the rover apparently rebooted its computer at least twice over the April 11-12 weekend.

"While we don't have an explanation yet, we do know that Spirit's batteries are charged, the solar arrays are producing energy and temperatures are well within allowable ranges. We have time to respond carefully and investigate this thoroughly," said John Callas of NASA's Jet Propulsion Laboratory, Pasadena, Calif., project manager for Spirit and twin-rover Opportunity. "The rover is in a stable operations state called automode and taking care of itself. It could stay in this stable mode for some time if necessary while we diagnose the problem."

Spirit communicated with controllers Friday, Saturday and Sunday, but some of the communication sessions were irregular. One of the computer resets apparently coincided in timing with operation of the rover's high-gain dish antenna.

The rover team has the advantage of multiple communication options. Spirit can communicate directly with Earth via either the pointable high-gain antenna or, at a slower data rate, through a low-gain antenna that does not move. Additionally, communications can be relayed by Mars orbiters, using the UHF (ultra-high frequency) transceiver, a separate radio system on the rover.

"To avoid potential problems using the pointable antenna, we might consider for the time being just communicating by UHF relay or using the low-gain antenna," Callas said.

Spirit finished its three-month prime mission on Mars five years ago and has kept operating through multiple mission extensions.

The rover's onboard software has been updated several times to add new capabilities for the mission, most recently last month. The team is investigating whether the unexpected behavior in recent days could be related to the new software, but the same software is operating on Opportunity without incident.

"We are aware of the reality that we have an aging rover, and there may be age-related effects here," Callas said.

In the past five weeks, Spirit has made 119 meters (390 feet) of progress going counterclockwise around a low plateau called "Home Plate" to get from the place where it spent the past Martian winter on the northern edge of Home Plate toward destinations of scientific interest south of the plateau. On March 10, after several attempts to get past obstacles at the northeastern corner of Home Plate, the rover team decided to switch from a clockwise route to the counterclockwise one. Subsequent events have included Spirit's longest one-day drive since the rover lost use of one of its wheels three years ago, plus detailed inspection of light-toned soil exposed by the dragging of the inoperable wheel.

Halfway around Mars, meanwhile, Opportunity has continued progress on a long-term trek toward Endeavour Crater, a bowl 22 kilometers (14 miles) in diameter and still about 12 kilometers (7 miles) away. Last week, a beneficial wind removed some dust from Opportunity's solar array, resulting in an increase by about 40 percent in the amount of electrical output from the rover's solar panels.

JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Exploration Rover project for NASA's Science Mission Directorate, Washington.