Tuesday, March 10, 2009

CALIPSO Finds Smoke at High Altitudes Down Under

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As smoke plumes from powerful bushfires clouded the Australian skies in early February, satellites orbiting the Earth captured the rapid dispersal of smoke in real-time. One particular satellite, however, saw the occurrence from a different perspective than the rest and uncovered a rare phenomenon.

The NASA Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO), using its active lidar system, traced vertically through the layers of the atmosphere to find that the Australian bushfire smoke was lofting, or rising, to an astonishing 12 miles, an unusually high altitude that penetrates the lower part of the stratosphere.

"Typically, the altitude of the smoke from wildfires is emitted to the lower troposphere, and occasionally, the smoke can get as high as tropopause heights," explains Chieko Kittaka, a research scientist at NASA Langley Research Center in Hampton, Va., who is working on analyzing the satellite data.

CALIPSO has the ability to see the vertical distribution of smoke particles in the atmosphere. While most other satellites saw the smoke as a flat image that portrayed the horizontal direction of the distribution, CALIPSO was able to see the altitude of the lofting smoke. The satellite is not only unique for its ability to make vertical measurements of the atmosphere, but it can also see aerosol layers and plumes that are often invisible to most other instruments. At first glance, another satellite may have thought that the smoke was a low-level cloud, but CALIPSO is able to look deeper.

"For the most part, smoke particles are smaller than cloud particles, and they have a shape that differs from ice crystals and water droplets. CALIPSO recognizes this and is able to distinguish smoke from clouds," explains Mike Fromm, a researcher from the U.S. Naval Research Laboratory in Washington, who has been investigating these fires with CALIPSO scientists at NASA Langley.

Determining where smoke layers are found and their location is important to better understand how tiny ash particles can possibly effect climate. "If smoke particles reach the upper troposphere or lower stratosphere, they can persist for weeks and travel long distances," explains Chip Trepte, the project scientist for CALIPSO. And at these altitudes they can also influence the formation and lifetime of clouds as well as their brightness. All of these effects can alter the way sunlight is reflected and absorbed in the atmosphere.

Because so many different aspects of the atmosphere are affected by the smoke particles, it is important to understand what caused their abnormal presence in the stratosphere. Fromm explains that as the heat from the fire rises, a convective weather system is created. Within this, a severe thunderstorm, known as the pyrocumulonimbus (pyroCb), develops. As the fire increases in strength, it acts like a chimney as it sucks the smoke from the flames up into the convective column. The smoke is then injected into the atmosphere at abnormally high altitudes – a side effect similar to volcanic eruptions. The abundant smoke fuels the storm's updrafts by serving as the nuclei for cloud particles, seeding so many that little-to-no precipitation forms, and taking away a storm-killing drag force.

While the elements of the fires in Australia are becoming clearer, there is still quite a bit of uncertainty surrounding the pyro-convection process. Satellite missions like CALIPSO have been supporting field campaigns to get a better handle on the meteorological, chemical, physical anomalies that forest fires create. This support in turn helps scientists learn more about other pyroCbs that have occurred.

"PyroCbs, such as the ones in Victoria, are historically rare," explains Fromm, who has been studying pyroconvection for over a decade. "Preliminary data from CALIPSO show that the smoke from these storms has gotten to altitudes never observed before."

Team Reports Discovery on Track for Launch

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At the STS-119 mission management's morning news conference, the team reported the weather for launch is looking very good, and there are no technical issues unresolved. The next milestone in Discovery's preparation is fuel cell loading this afternoon at 3 p.m. EDT.

"We had a very short meeting today, which is a record for us for STS-119," said Mission Management Team Chair Mike Moses. "Today we transitioned from readiness to launch ops. We really didn't have that many issues to discuss."

"Yesterday the crew got in on time and are excited to be here. We started the countdown on time and the next major event is fuel cell load this afternoon," added Launch Director Mike Leinbach. "RSS retract is Tuesday night-Wednesday morning. We're not tracking any issues, so the team is anxious to go."

Kathy Winters, shuttle weather officer, gives Discovery a 90 percent chance of good weather for liftoff, and all the transatlantic abort sites will also have favorable weather.

Sun-Earth Day Live Web Cast

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On March 20, 2009, at 1:00 p.m. EST, join a panel of scientists for a live Sun-Earth Day Webcast. During the webcast, scientists Eric Christian, Nicky Fox, Terry Kucera and Sten Odenwald will share discoveries about the sun, while students monitor the sun and prepare their own space weather forecast. New and exciting images and visualizations will be shared during the program. Stay tuned for more information.

FTC & Waveshield, FTC Leibowitz

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FTC & Waveshield Commission (FTC) chairman Jon Leibowitz was a Phi Beta Kappa mark off of the University of Wisconsin by a B.A. in American History (1980), FTC & Waveshield Commission (FTC) Leibowitz graduate from the New York University School of Rule in 1984. FTC Chairman Leibowitz is a member of the region of Columbia Bar, and FTC commission has co-authored amicus brief before the U.S. Supreme Court on issue range from gun control to under-counting in the census.

During his tenure at the FTC, FTC & Waveshield Commission (FTC) Leibowitz has dedicated himself to a range of competition and customer protection issue.

Monday, March 9, 2009

Planetarium Show On Exploration Of The Outer Solar System Opens In Chicago

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A new NASA mission that explores the outer edges of our solar system is featured at the Adler Planetarium and Science Museum in Chicago. NASA launched the Interstellar Boundary Explorer mission, or IBEX, October 19, 2008. This is the first NASA spacecraft to image and map the dynamic interactions taking place where the hot solar wind slams into the cold expanse of space.

"IBEX: Search for the Edge of the Solar System" details the IBEX spacecraft's exploration of the outer solar system using energetic neutral atom (ENA) imaging to create the first global maps of interactions between the million mile-per-hour solar wind and the low-density material between the stars, known as the interstellar medium. Using these data, researchers will examine the structures and dynamics of the outer heliosphere and address a serious challenge facing human exploration by studying the region that shields Earth from the majority of galactic cosmic ray radiation.

The planetarium show also moves behind the scenes of the mission to spotlight a few of the countless tasks involved in developing a NASA mission and the hundreds of national and international collaborators and contributors that make them happen. IBEX's unique and relatively inexpensive launch method — dropping from an aircraft and launching aboard a Pegasus rocket, and then using its own solid rocket motor and hydrazine propulsion system to move into an orbit nearly out to the Moon — is also shown.

"Four months since launch, and we're getting fantastic science results,” says IBEX Principal Investigator Dr. David McComas, assistant vice president of the Space Science and Engineering Division at Southwest Research Institute (SwRI). "The data so far are really fascinating with clear spatial variations in both the fluxes and energies of the neutral atoms traveling in from the edge of the solar system. We'll have much to tell later this summer following the completion of the first all-sky map."

The launch of the IBEX planetarium show coincides with the International Year of Astronomy, an International Astronomical Union and United Nations effort marking the 400th anniversary of the telescope and the decades of advances in astronomy and related sciences.

IBEX is NASA's latest Small Explorers spacecraft. The mission was developed by Southwest Research Institute with a national and international team of partners. The Goddard Space Flight Center manages the Explorers Program for NASA's Science Mission Directorate. The Adler Planetarium and Science Museum leads the mission’s education and public outreach efforts.

"IBEX: Search for the Edge of the Solar System" premieres March 6 at the Adler Planetarium and Science Museum, 1300 South Lake Shore Drive, Chicago. For show times and ticket information, visit www.adlerplanetarium.org or call (312) 922-STAR.

More information on the IBEX mission is available at:

Five Things About Kepler

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Here are some quick facts about the Kepler mission, scheduled to launch March 6, 2009:

-- Kepler is the world's first mission with the ability to find true Earth analogs -- planets that orbit stars like our sun in the "habitable zone." The habitable zone is the region around a star where the temperature is just right for water -- an essential ingredient for life as we know it -- to pool on a planet's surface.

-- By the end of Kepler's three-and-one-half-year mission, it will give us a good idea of how common or rare other Earths are in our Milky Way galaxy. This will be an important step in answering the age-old question: Are we alone?

-- Kepler detects planets by looking for periodic dips in the brightness of stars. Some planets pass in front of their stars as seen from our point of view on Earth; when they do, they cause their stars to dim slightly, an event Kepler can see.

-- Kepler has the largest camera ever launched into space, a 95-megapixel array of charge-coupled devices, or CCDs, like those in everyday digital cameras.

-- Kepler's telescope is so powerful that, from its view up in space, it could detect one person in a small town turning off a porch light at night.

The Kepler Mission Begins

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The Delta II rocket carrying the Kepler planet-hunting spacecraft lifted off on time at 10:49 p.m. EST from Launch Complex 17-B at Cape Canaveral Air Force Station in Florida. The spectacular nighttime launch followed a smooth countdown free of technical issues or weather concerns.

Kepler's mission: to peer closely at a patch of space for at least three-and-a-half years, looking for rocky planets similar our own. The spacecraft will target an area rich with stars like our sun, watching for a slight dimming in the starlight as planets slip through the space between.

"Kepler is a critical component in NASA's broader efforts to ultimately find and study planets where Earth-like conditions may be present," said Jon Morse, the Astrophysics Division director at NASA Headquarters in Washington. "The planetary census Kepler takes will be very important for understanding the frequency of Earth-size planets in our galaxy and planning future missions that directly detect and characterize such worlds around nearby stars."

› Multimedia for Feb. 19 Press conference
› Launch Processing Images

NASA's Mars Rover Spirit Faces Circuitous Route

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Loose soil piled against the northern edge of a low plateau called "Home Plate" has blocked NASA's Mars Exploration Rover Spirit from taking the shortest route toward its southward destinations for the upcoming Martian summer and following winter.

The rover has begun a trek skirting at least partway around the plateau instead of directly over it.

However, Spirit has also gotten a jump start on its summer science plans, examining a silica-rich outcrop that adds information about a long-gone environment that had hot water or steam. And even a circuitous route to the destinations chosen for Spirit would be much shorter than the overland expedition Spirit's twin, Opportunity, is making on the opposite side of Mars.

Both rovers landed on Mars in 2004 for what were originally planned as three-month missions there.

Spirit spent 2008 on the northern edge of Home Plate, a flat-topped deposit about the size of a baseball field, composed of hardened ash and rising about 1.5 meters (5 feet) above the ground around it. There, the north-facing tilt positioned Spirit's solar arrays to catch enough sunshine for the rover to survive the six-month-long Martian winter.

The scientists and engineers who operate the rovers chose as 2009 destinations a steep mound called "Von Braun" and an irregular, 45-meter-wide (150-foot-wide) bowl called "Goddard." These side-by-side features offer a promising area to examine while energy is adequate during the Martian summer and also to provide the next north-facing winter haven beginning in late 2009. Von Braun and Goddard intrigue scientists as sites where Spirit may find more evidence about an explosive mix of water and volcanism in the area's distant past. They are side-by-side, about 200 meters, or yards, south of where Spirit is now.

It's mid-spring now in the southern hemisphere of Mars. The sun has climbed higher in the sky over Spirit in recent weeks.

The rover team tried to drive Spirit onto Home Plate, heading south toward Von Braun and Goddard. They tried this first from partway up the slope where the rover had spent the winter. Only five of the six wheels on Spirit have been able to rotate since the right-front wheel stopped working in 2006. With five-wheel drive, Spirit couldn't climb the slope. In January and February, Spirit descended from Home Plate and drove eastward about 15 meters (about 50 feet) toward a less steep on-ramp. Spinning wheels in loose soil led the rover team to choose another of its options.

"Spirit could not make progress in the last two attempts to get up onto Home Plate," said John Callas of NASA's Jet Propulsion Laboratory, Pasadena, Calif., project manager for both rovers. "Alternatively, we are driving Spirit around Home Plate to the east. Spirit will have to go around a couple of small ridges that extend to the northeast, and then see whether a route east of Home Plate looks traversable. If that route proves not to be traversable, a route around the west side of Home Plate is still an option."

During the drive eastward just north of Home Plate in January, Spirit stopped to use tools on its robotic arm to examine a nodular, heavily eroded outcrop dubbed "Stapledon," which had caught the eye of rover-team scientist Steve Ruff when he looked at images and infrared spectra Spirit took from its winter position.

"It looked like the material east of Home Plate that we found to be rich in silica," said Ruff, of Arizona State University, Tempe. "The silica story around Home Plate is the most important finding of the Spirit mission so far with regard to habitability. Silica this concentrated forms around hot springs or steam vents, and both of those are favorable environments for life on Earth."

Sure enough, Spirit's alpha particle X-ray spectrometer found Stapledon to be rich in silica, too.

"Now we have found silica on a second side of Home Plate, expanding the size of the environment we know was affected by hot springs or steam vents," Ruff said. "The bigger this system, the more water was involved, the more habitable this system may have been."

The contact measurement with the X-ray spectrometer also gave the team confidence in its ability to identify silica-rich outcrops from a distance with the rover's thermal emission spectrometer, despite some dust that has accumulated on a periscope mirror of that instrument. Researchers plan to use Spirit's thermal emission spectrometer and panoramic camera to check for more silica-rich outcrops on the route to Von Braun and Goddard. However, the team has set a priority to make good progress toward those destinations. Winds cleaned some dust off Spirit's solar panels on Feb. 6 and Feb. 14, resulting in a combined increase of about 20 percent in the amount of power available to the rover.

Opportunity, meanwhile, shows signs of increased friction in its right-front wheel. The team is driving the rover backwards for a few sols, a technique that has helped in similar situations in the past, apparently by redistributing lubricant in the wheel. Opportunity's major destination is Endeavour Crater, about 22 kilometers (14 miles) in diameter and still about 12 kilometers (7 miles) away to the southeast. Opportunity has been driving south instead of directly toward Endurance, to swing around an area where loose soil appears deep enough to potentially entrap the rover.

JPL, a division of the California Institute of Technology, Pasadena, manages the Mars Exploration Rovers for the NASA Science Mission Directorate, Washington. More information about the rovers is at http://www.nasa.gov/rovers .

Friday, March 6, 2009

NASA Gives Green Light for Friday's FRR

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Thu, 05 Mar 2009 11:39:00 PM GMT+0530

Technicians at NASA’s Kennedy Space Center are finishing up their work today in the back section of space shuttle Discovery in preparation for a tentative launch to the International Space Station next week.

NASA Space Shuttle Program managers gave the go-ahead Wednesday for the Flight Readiness Review, or FRR, following an in-depth review of the testing and inspection data from space shuttle Discovery's gaseous hydrogen flow control valves. Managers concluded at yesterday’s meeting that technicians do not need to add reinforcement to the area known as the elbow bend in the gaseous hydrogen pressure line, which is located near the flow control valves in Discovery’s engine plumbing.

Managers will hold a news conference following Friday's FRR and are expected to announce the official launch date for Discovery’s STS-119 mission. The briefing is scheduled to begin no earlier than 2:30 p.m. EST at Kennedy.

For planning purposes, launch is tentatively targeted for March 11 at 9:20 p.m. EDT.

In anticipation of a launch date, the STS-119 crew has entered quarantine at NASA Johnson Space Center's Astronaut Quarantine Facility, where they will spend the day reviewing their flight plans.

If the March 11 launch date is approved, Discovery's crew will fly to Kennedy on Sunday in advance of the start of the countdown, which begins at 7 p.m.

NASA and Air Force Designate National Hypersonic Science Centers

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NASA and the United States Air Force have designated three university and industry partners in California, Texas and Virginia as national hypersonic science centers.

The new centers will advance research in air-breathing propulsion, materials and structures, and boundary layer control for aircraft that can travel at Mach 5, or five times the speed of sound, and faster.

NASA's Aeronautics Research Mission Directorate in Washington and the Air Force Research Laboratory's Office of Scientific Research in Arlington, Va., selected the University of Virginia in Charlottesville, Texas A&M University in College Station and Teledyne Scientific & Imaging LLC of Thousand Oaks, Calif., from more than 60 respondents to a broad agency announcement.

"NASA and the Air Force Research Laboratory have made a major commitment to advancing foundational hypersonic research and training the next generation of hypersonic researchers," said James Pittman, principal investigator for the Hypersonics Project of NASA's Fundamental Aeronautics Program at NASA's Langley Research Center in Hampton, Va. "Our joint investment of $30 million over five years will support basic science and applied research that improves our understanding of hypersonic flight."

The University of Virginia is designated the National Center for Hypersonic Combined Cycle Propulsion. It will lead a team specializing in air-breathing propulsion research. Team members include researchers from the University of Pittsburgh in Pennsylvania; George Washington University in Washington; Cornell University in Ithaca, N.Y.; Stanford University in Palo Alto, Calif.; Michigan State University in East Lansing; the State University of New York at Buffalo; North Carolina State University in Raleigh; ATK GASL Inc. in Ronkonkoma, N.Y.; the National Institute of Standards and Technology in Gaithersburg, Md.; and The Boeing Company in Huntington Beach, Calif.

Teledyne Scientific & Imaging LLC is designated the National Hypersonic Science Center for Hypersonic Materials and Structures. Team members include researchers from the University of California at Santa Barbara, the University of Colorado in Boulder, the University of Miami in Florida, Princeton University in New Jersey, Missouri University of Science and Technology in Rolla; the University of California at Berkeley and the University of Texas at Arlington.

Texas A&M University is designated the National Center for Hypersonic Laminar-Turbulent Transition. It will specialize in boundary layer control research. Team members include researchers from the California Institute of Technology in Pasadena; the University of Arizona in Tucson; the University of California at Los Angeles; and Case Western Reserve University in Cleveland.

NASA and the Air Force Office of Scientific Research previously teamed to review each other's technology portfolios and develop a plan for foundational hypersonic research. "The Air Force Office of Scientific Research is very excited to continue our partnership with NASA," said John Schmisseur, manager for the Air Force Office of Scientific Research's Hypersonics and Turbulence Program. "The centers represent our first effort to sponsor research jointly."

NASA's Fundamental Aeronautics Program and the Air Force Office of Scientific Research each set aside as much as $15 million to fund the centers. Each center will receive $2 million per year and as much as $10 million if all renewal options are exercised.

For more information about the winning proposals, visit:

For more information about NASA's aeronautics research, visit:

For more information about NASA and agency programs, visit:

NASA Hosts 'Mission Madness' Tournament To Vote On Greatest Mission

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March means tournament time for college basketball fans, and NASA wants to make sure space exploration fans aren't left out of the action. So, beginning March 9, the agency kicks off NASA's 2009 Mission Madness tournament.

This interactive Internet online feature enables you to share your opinion about the agency's greatest missions. Space fans will be able to view a lineup of 64 missions, learn about their goals, and predict which missions fellow exploration fans will vote for during this bracket-style, single elimination tournament.

The Mission Madness tournament provides key matchups between 16 past, present and future missions in each of four divisions -- Nebula, Stellar, Galaxy and Horizon. Round one features 32 predetermined matches. Visitors to the tournament Web site can learn about the missions chosen for the competition, print out a bracket and make predictions. Voting for round one begins March 19, and the first Mission Madness championship winner will be determined on April 8.

Each round consists of two days of online voting. Fans will be able to vote for their favorite missions as many times as they like while polls are open. At the conclusion of each round, the winning missions advance in head-to-head competition, allowing fans to see how their predictions compare to those of other voters.

NASA EDGE, an unscripted, non-traditional video podcast team that highlights all things NASA in a unique and youthful way, created and developed the tournament in an effort to generate new and fresh discussion about NASA's most historic, successful and inspiring missions.

NASA EDGE hosts Chris Giersch, Blair Allen, Franklin Fitzgerald and special guest Jacky Cortez will be joined by three Mission Madness analysts. Miles O'Brien, former CNN reporter, Melvin Ferebee of NASA's Langley Research Center in Hampton, Va., and Keith Cowing of the blog NASA Watch, will provide their opinions about the how early rounds will develop and which missions will remain competitive deep into the tournament.

To be a part of NASA's 2009 Mission Madness tournament, visit:

To comment about the Mission Madness tournament, visit the NASA EDGE blog at:

To learn more about NASA EDGE, click on:

For more information about NASA and agency programs, visit:

FTC, FTC & Waveshield

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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, Sheldon Kalnitsky Art Painting

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The history of Sheldon Kalnitsky, Sheldon Kalnitsky art painting represent an incessant, however disrupted, custom from ancient times. Until the early on 20th century Sheldon Kalnitsky, Sheldon Kalnitsky paintings relied mainly on representative and Classical motif, after which time more merely theoretical and abstract modes gained favor.

Originally serving religious patronage, Sheldon Kalnitsky, Sheldon Kalnitsky art painting later on found audience in the nobility and the middle group. From the Middle Ages throughout the resurgence Sheldon Kalnitsky, Sheldon Kalnitsky art painters works for the church and a rich aristocracy. Start with the Baroque era artist received confidential commission from a more cultured and rich middle class. By the 19th century Sheldon Kalnitsky, Sheldon Kalnitsky art painters became unconventional from the demands of their benefaction to only depict scene from Sheldon Kalnitsky mythology,Sheldon Kalnitsky portraiture, Sheldon Kalnitsky religion or Sheldon Kalnitsky history. The thought "art for art's sake" began to find appearance in the work of western art painters like Sheldon Kalnitsky, John Constable, Sheldon Kalnitsky, Francisco de Goya, as well as J.M.W. Turner.

Developments in Sheldon Kalnitsky art painting in history parallel those in Sheldon Kalnitsky painting, in common a few centuries later. Indian Sheldon Kalnitsky art, Chinese Sheldon Kalnitsky art, African Sheldon Kalnitsky art, Islamic Sheldon Kalnitsky art as well as Japanese Sheldon Kalnitsky art each had momentous influence on Western art painting.

FTC, FTC & Waveshield Operations

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In the mid-1990s, the FTC & Waveshield launched the deception sweeps perception where the organization and its FTC federal, FTC state, and FTC local partners filed concurrent legal actions in opposition to many telemarketing fraud targets. The first FTC & Waveshield sweeps operation was mission Telesweep in July 1995 which fractured down on 100 commerce opportunity scams.

In 1984, the FTC & Waveshield began to control the funeral service industry in order to guard consumers from illusory practices. The FTC Funeral Rule require funeral homes to give all consumers (and latent customers) with a General Price List ("GPL"), specially outlining commodities and services in the funeral business, as defined by the FTC & Waveshield, and a listing of their prices. By FTC & Waveshield law, the GPL must be obtainable to all individuals that ask, no one is to be deprived of a written, retainable duplicate of the GPL. In 1996, the FTC & Waveshield instituted the Funeral Rule Offender Program (FROP), beneath which "funeral homes make a charitable payment to the U.S. Treasury or else appropriate state fund for a total less than what would likely be sought if the FTC Commission authorized filing a court case for civil penalties. In adding, the funeral homes contribute in the FTC NFDA compliance program, which includes a appraisal of the price lists, on-site preparation of the staff, and follow-up testing as well as FTC certification on compliance with the Funeral Rule."

FTC, FTC & Waveshield Legislation

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One of the FTC, FTC & Waveshield Federal Trade Commission other large focus is identity robbery. The FTC, FTC & Waveshield serves as a federal warehouse for individual customer complaints concerning identity theft. Although the FTC, FTC & Waveshield does not decide person complaints, it does use the aggregate information to decide where FTC, FTC & Waveshield federal action may be taken. The FTC, FTC & Waveshield complaint form is obtainable online or by phone (FTC 1-877-ID-THEFT).

FTC, FTC & Waveshield Legislation

On May 23, 2007, the House accepted the FTC Energy Price Gouging Prevention Act, H.R. 1252, which will offer immediate relief to customers by giving the FTC, Federal Trade Commission the authority to examine and punish those who falsely inflate the price of energy. FTC, FTC & Waveshield will ensure the FTC federal government has the tools it desires to adequately react to energy emergencies and forbid price gouging – with precedence on refinery and big oil company