lunes, 31 de marzo de 2014

NASA : Wind Tunnel Testing a Full-Sized Aircraft Tail


Wind Tunnel Testing a Full-Sized Aircraft Tail
NASA recently tested a full-sized tail from a 757 commercial aircraft that was modified and equipped with tiny jets called "sweeping jet actuators" to blow air across the rudder surfaces.
The test vertical tail is an actual 757 tail that came out of an aircraft bone yard in Arizona and was refurbished into a wind tunnel model.
The tunnel hosted the 26-foot 757 tail for a series of tests of an innovative Active Flow Control system that one day might allow airplane builders to design smaller tails, which would reduce weight and drag, and help improve fuel efficiency. The “flow control” comes from the actuators, which are devices that essentially blow air in a sweeping motion along the span of the tail and manipulate that flow of air.
The image was taken inside the National Full-Scale Aerodynamic Complex, a massive wind tunnel located at NASA’s Ames Research Center in Moffett, Ca. In the image, an engineer braces himself against the strong winds in the tunnel as he holds a wand emitting a stream of smoke that’s used to visualize “in flight” air flow across the tail.
Actuator technology will be installed for flight tests on the tail of Boeing’s ecoDemonstrator program 757 flight test aircraft in early 2015 as part of an agreement with NASA.
Image Credit: NASA/Dominic Hart
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

jueves, 13 de marzo de 2014

NASA - Space Communications Antenna Supported Early NASA Missions


Space Communications Antenna Supported Early NASA Missions
This 26 meter (85 foot) antenna operated in Woomera (Island Lagoon), Australia at Deep Space Station (DSS) 41, established in August 1960. The Island Lagoon site was the first deep space station to be established outside the United States and the first Australian antenna NASA built. The station was operated by the Australian Department of Supply and helped support the Ranger and early Mariner missions, as well as communications from the Deep Space Network (DSN) complex in Goldstone, California via a moon bounce. Woomera’s antenna ceased operations in 1972.
Today, the Deep Space Network -- consisting of three sites in Goldstone, California; Madrid, Spain; and Canberra, Australia -- supports space communications for NASA and non-NASA missions that explore the furthest points of our solar system. Each complex currently has a 70 meter (230 foot) antenna, one 34 meter (111 foot) High Efficiency (HEF) antenna, and one or more 34 meter Beam Wave Guide (BWG) antenna. The Deep Space Network is operated 24 hours a day, seven days a week, 365 days per year. To support future mission needs, construction is currently underway in Canberra, Australia to add two new 34 meter BWG antennas, Deep Space Station 35 (DSS-35) and DSS-36 by 2018.
Image Credit: NASA
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

nsf.gov - National Science Foundation - New bilateral pilot opportunity will fund collaborations between US and UK bioscience researchers


Proposals on systems biology, computational biology, bioinformatics and synthetic biology are eligible for consideration for joint US/UK funding
flags of the United States and the United Kingdom
U.S./U.K. research teams may now seek joint U.S./U.K. funding through a simplified mechanism.
Credit and Larger Version
March 4, 2014
A new, two-year pilot opportunity--known as The U.S. NSF/BIO-UK BBSRC Lead Agency Pilot Opportunity--is being formally launched today.
This Pilot opportunity is designed to make it easier for research teams comprised of scientists from the United States and the United Kingdom to manage funding logistics and to simultaneously obtain funding from both countries. It is funded by the U.S. National Science Foundation's (NSF) Directorate for Biological Sciences and the U.K.'s Biotechnology and Biological Sciences Research Council (BBSRC).
This Pilot opportunity will use a simplified, flexible review process that will allow U.S./U.K. research teams to submit a single proposal that will undergo a single review process by only one of the partner agencies. Successful proposals will be funded by both NSF and the BBSRC.
Cora B. Marrett, acting director of NSF, said, "Although NSF has always funded U.S. scientists involved in international collaborations, such collaborations have become increasingly important, partly because of the rapid globalization of research. The many benefits of this Pilot opportunity will include better coordination of funding for U.S./U.K. research teams and increased bilateral awareness of scientific strengths and advancements between the U.S. and U.K. funding agencies."
Jackie Hunter, BBSRC chief executive, said, "Partnerships are vital to U.K. bioscience, offering the opportunity to combine resources and expertise to tackle global challenges. As funders, we are working to reduce some of the barriers encountered by researchers when working with international partners. This pilot is an important step that will help to streamline the collaborative funding process between NSF and BBSRC, making applications easier for those in our community working with the U.S."
The Pilot opportunity was created under a Memorandum of Understanding between NSF and the U.K.'s research councils, which support research partnerships between the two countries. The Pilot opportunity is designed to reduce obstacles that have traditionally been faced by researchers wishing to form international teams. These obstacles include identifying appropriate funding agencies; risking "double jeopardy," where one country's funding agency decides to fund an international team's research proposal, but the partner country does not; and dealing with the different timetables of different funding agencies.
The first step in applying for funding under The Pilot opportunity will be for each research team to select a lead agency based on whether its proposed research would fall more within the scope of NSF'S Directorate for Biological Sciences or that of the BBSRC. Then, each team will submit to its proposed lead agency an Intention to Submit (ITS) that summarizes its proposed research, funding request and other associated information. These documents will be reviewed in August 2014 and August 2015.
Based on each team's ITS, the team's lead agency will determine whether the team will be invited to submit a full proposal. Full proposals will be reviewed in fall 2014 and fall 2015; these reviews will be conducted according to the review criteria of each team's lead agency. Proposals that cover systems biology, computational biology, bioinformatics and synthetic biology (the latter, only for fall 2015 submissions) will be eligible for consideration.
Although the review criteria of NSF and BBSRC are not identical, both agencies' criteria include evaluations by invited reviewers on proposals' scientific or intellectual merit as well as on their broader societal impacts. The decision made by the lead agency on each proposal will be discussed with the partner agency. If a research team receives an award, its U.S. researchers will be funded by NSF, and its U.K. researchers will be funded by the BBSRC.
More information about The U.S. NSF/BIO-UK BBSRC Lead Agency Pilot Opportunity, including submission deadlines, is provided in NSF's Dear Colleague Letter and on the BBSRC's website, which features its Management Plan for the pilot opportunity.
-NSF-
Media Contacts Lily Whiteman, National Science Foundation, (703) 292-8310, lwhitema@nsf.gov
Robert Dawson, Biotechnology and Biological Sciences Research Council of U.K., 01793413204, robert.dawson@bbsrc.ac.uk
Program Contacts James Deshler, National Science Foundation, (703) 292-7871, jdeshler@nsf.gov
The National Science Foundation (NSF) is an independent federal agency that supports fundamental research and education across all fields of science and engineering. In fiscal year (FY) 2014, its budget is $7.2 billion. NSF funds reach all 50 states through grants to nearly 2,000 colleges, universities and other institutions. Each year, NSF receives about 50,000 competitive requests for funding, and makes about 11,500 new funding awards. NSF also awards about $593 million in professional and service contracts yearly.
Useful NSF Web Sites:
NSF Home Page: http://www.nsf.gov
NSF News: http://www.nsf.gov/news/
For the News Media: http://www.nsf.gov/news/newsroom.jsp
Science and Engineering Statistics: http://www.nsf.gov/statistics/
Awards Searches: http://www.nsf.gov/awardsearch/
The National Science Foundation (NSF)
Guillermo Gonzalo Sánchez Achutegui

domingo, 9 de marzo de 2014

ESA : Margarita Island, Venezuela


Situated in the southern Caribbean Sea about 20 km off of mainland Venezuela’s coast, the island comprises two peninsulas linked by a long, narrow strip of land – called an isthmus.
The eastern part of the island is home to most of the island’s residents, while the Macanao peninsula to the west is dominated by a central mountain range.
Between the peninsulas and cut off from the open sea by the isthmus lies the La Restinga lagoon, a national park that appears as a dark green and blue area in this image.
Recognised as a wetland of international importance by the Ramsar Convention, the area features picturesque mangroves and is an important feeding ground for birds such as herons and flamingos. The shallow waters are home to red snappers, sardines and swordfish – among other types of fish – and oysters grow on the mangrove roots.
Japan's ALOS satellite captured this image on 26 June 2010 with its AVNIR-2 Advanced Visible and Near Infrared Radiometer.
ALOS was supported as a Third Party Mission, which means that ESA used its multi-mission ground systems to acquire, process, distribute and archive data from the satellite to its user community.
In April 2011 the satellite abruptly lost power while mapping Japan’s tsunami-hit coastline.
This image is featured on the Earth from Space video programme.
ESA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

ESA : Catching signals from a speeding satellite


Catching signals from a speeding satellite

Upgraded station in Spain
7 March 2014
Soaring high above Earth as they speed through space, satellites are difficult targets to track. Now a new approach developed in Europe is helping ground stations to acquire signals faster and more accurately than ever before.
During launch, a satellite is flung into orbit with tremendous force, attaining speeds of over 28 000 km/h – about 40 times faster than a commercial airliner.
A critical moment is when the satellite separates from its rocket and starts transmitting radio signals. A receiving station on the ground has to be ready and waiting, pointed at precisely the right spot in the sky to catch the transmission, which is a highly focused and narrow beam. And it’s moving fast.
“Traditionally, even the best stations – like ESA’s 15 m and 35 m-diameter dishes – are only sensitive across an arc of just a few degrees,” says Magdalena Martinez de Mendijur, a systems engineer at ESA’s Operations Centre in Germany.
“If the antenna is not pointed perfectly, or if the satellite zips by out of its ‘field of view’ before acquisition, the signal could be missed altogether.”

A cutting-edge difference

SARAS – a Spanish acronym for ‘Fast Acquisition of Satellites and Launchers’ – is a circular array of eight small radio-frequency sensors mounted around the rim of an existing dish antenna.
New antenna array
That’s where SARAS – a Spanish acronym for ‘Fast Acquisition of Satellites and Launchers’ – is making a cutting-edge difference.
The system mounts a circular array of eight small radio-frequency sensors around the rim of an existing dish antenna.
“The signals received by these eight are combined, and the system can estimate the direction of arrival of the incoming radio beam, and the entire dish can be repointed directly at the satellite with great precision and accuracy, even when the incoming signal is weak or distorted,” says Magdalena.
It was fitted to the 15 m dish at ESA’s Space Astronomy Centre in Spain in 2013. Since then, it has been extensively tested, catching signals from missions including CryoSat-2, XMM, GOCE and Swarm.

ESA partners with European industry

“This new approach more than doubles the size of the dish’s window and we can acquire signals from a new satellite in less than 12 seconds,” says Klaus Juergen Schulz, responsible for ground station engineering.
“A future version should improve this to just two seconds.”
SARAS for faster satellite tracking
The technology was developed by Spanish company Isdefe, partly supported by ESA’s General Support Technology Programme, which converts promising engineering concepts into mature products.
The system has been patented in Spain and is being patented in Europe, and will be developed into a full commercial product.
“This is an excellent example of how technology research supported through ESA funding and technical and managerial supervision can be developed by European industry into world-class products and services,” says Juan Miro, Head of ESA’s Ground Systems Engineering department.

Related articles
Deep-space stations gain made-in-Europe hearing boost18 July 2013 Picking up ultra-weak signals from spacecraft exploring deep in our Solar System requires cooling a detector to within a few degrees of absolute zero. Thanks to ESA’s support, the technology is now available in Europe for the first time.
ESA
Guillermo Gonzalo Sánchez Achutegui

NASA : NASA Selects 10 Proposals for Unprecedented Twin Astronaut Study

On March 7, NASA announced the selection of 10 investigations for the study of identical twin astronauts Scott and Mark Kelly and, in doing so, launched human space life science research into a new era. Although NASA’s Human Research Program has been researching the effects of spaceflight on the human body for decades, these 10 investigations will provide NASA with broader insight into the subtle effects and changes that may occur in spaceflight as compared to Earth-based environments. NASA and the National Space Biomedical Research Institute (NSBRI) will jointly manage this ambitious new undertaking.
“We realized this is a unique opportunity to perform a class of novel studies because we had one twin flying aboard the International Space Station and one twin on the ground,” says Craig Kundrot, Ph.D. and deputy chief scientist of NASA’s Human Research Program. “We can study two individuals who have the same genetics, but are in different environments for one year.”
Astronauts Mark Kelly and Scott Kelly are pictured in training
Astronauts Mark Kelly and Scott Kelly are pictured participating in the Joint STS-134, Expedition 25 and Expedition 26 ISS Emergency Scenario training
Image Credit:
NASA
Astronauts Mark Kelly and Scott Kelly at the check-out facility at Ellington Field
Astronauts Mark Kelly (right), STS-124 commander, and Scott Kelly are pictured in the check-out facility at Ellington Field near NASA's Johnson Space Center as the STS-124 crewmembers prepare for a flight to Kennedy Space Center in NASA T-38 trainer jets.
Image Credit:
NASA
Youtube Override:
HRP Twins Study Video
Image Credit:
NASA
 
The investigations, which were picked from a pool of 40 proposals, introduce to space physiology the field of –omics, the integrated study of DNA, RNA, and the entire complement of biomolecules in the human body. Studying human physiology at this fundamental level will provide NASA and the broader spaceflight community with unique information. This is because these tiny components of the human body tell researchers volumes about an individual’s composition and their reaction to stressors like those associated with spaceflight. Investigating the subtle changes – or lack thereof – between the Kelly brothers at this level, after Scott’s year in space and Mark’s year on Earth, could shed light between the nature vs. nurture aspect of the effects of spaceflight on the human body.
The studies will focus on four areas: human physiology, behavioral health, microbiology/microbiome, and molecular or -omics studies. Human physiological investigations will look at how the spaceflight environment may induce changes in different organs like the heart, muscles or brain within the body. Behavioral health investigations will help characterize the effects spaceflight may have on perception and reasoning, decision making and alertness. The microbiology/microbiome investigations will explore the brothers’ dietary differences and stressors to find out how both affect the organisms in the twins’ guts. Lastly, but potentially opening a whole new realm of information about humans exposed to the spaceflight environment are the molecular or -omics investigations. These studies will look at the way genes in the cells are turned on and off as a result of spaceflight; and how stressors like radiation, confinement and microgravity prompt changes in the proteins and metabolites gathered in biological samples like blood, saliva, urine and stool.
Some of the investigations are brand new, some are already being considered as part of the research plans for the one-year mission set for 2015, and some are already being performed with crews living aboard the space station for six-month durations. These will allow the agency to build upon existing knowledge about long duration spaceflight.
Although the investigations conducted on the Kelly brothers are not expected to provide definitive data about the effects of spaceflight on individuals — because there are only two subjects for data collection — they do serve as a demonstration project for future research initiatives. These investigations may identify changes to pursue in research of larger astronaut populations.
“This is a unique opportunity for the agency,” says Kundrot. “The investigations are a pathfinder for the agency with regard to the study of astronaut physiology.”
“This pilot project will, for the first time in space, integrate physiology with 21st century -omics techniques currently performed at leading medical schools and hospitals,” says Graham Scott, NSBRI chief scientist.
Who knew the next big thing in space life science would be so subtle?

NASA Selects 10 Proposals for Unprecedented Twin Astronaut Study

Only one set of twins has ever been into space, and now those twins are providing an unprecedented opportunity for scientists to understand better the effects of microgravity on the human body.
NASA's Human Research Program (HRP) will fund 10 short-term, first-of-its-kind investigations into the molecular, physiological and psychological effects of spaceflight in a continuous effort to reduce the health impacts of human space exploration. The National Space Biomedical Research Institute is partnering with HRP to provide genetic counseling and assisting in the management of the research.
This unique opportunity is made possible by NASA's decision to fly veteran astronaut Scott Kelly aboard the International Space Station for one year, beginning March 2015, while his identical twin brother, retired astronaut Mark Kelly, remains on Earth.
This study will focus in part on the comparison of blood samples collected from Scott and Mark at regular intervals before, during and after the one-year mission. Physiological and psychological testing also will be conducted on the brothers before, during and after the mission.
Scientific and technical experts from academia and government reviewed 40 proposals submitted in response to the research announcement "Human Exploration Research Opportunities - Differential Effects on Homozygous Twin Astronauts Associated with Differences in Exposure to Spaceflight Factors." The 10 selected proposals, which are from 10 institutions in seven states, will receive a combined $1.5 million during a three-year period.
HRP regularly assesses crew health and performance during spaceflight to evaluate associated risks. From these assessments, HRP develops strategies to monitor and mitigate these risks. These studies often have the considerable added benefit of advancing health care for people on Earth.
For a complete list of the selected proposals, principal investigators and organizations, visit:
For information about NASA's Human Research Program, visit:
For information on the National Space Biomedical Research Institute, visit:
For information about the International Space Station, its crews and research, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com  

NASA : NASA's WISE Survey Finds Thousands of New Stars, But No 'Planet X'


A nearby star stands out in red in this image from the Second Generation Digitized Sky Survey
A nearby star stands out in red in this image from the Second Generation Digitized Sky Survey.
Image Credit:
DSS/NASA/JPL-Caltech
Data from NASA's Wide-field Infrared Survey Explorer, or WISE
Data from NASA's Wide-field Infrared Survey Explorer, or WISE, has found no evidence for a hypothesized body sometimes referred to as "Planet X."
Image Credit:
Penn State University
WISE J104915.57-531906
The third closest star system to the sun, called WISE J104915.57-531906, is at the center of the larger image, which was taken by NASA's Wide-field Infrared Survey Explorer (WISE).
Image Credit:
NASA/JPL/Gemini Observatory/AURA/NSF
Screen capture from the animation
Animation of a fast-moving, nearby star.
 
After searching hundreds of millions of objects across our sky, NASA's Wide-Field Infrared Survey Explorer (WISE) has turned up no evidence of the hypothesized celestial body in our solar system commonly dubbed "Planet X."
Researchers previously had theorized about the existence of this large, but unseen celestial body, suspected to lie somewhere beyond the orbit of Pluto. In addition to "Planet X," the body had garnered other nicknames, including "Nemesis" and "Tyche."
This recent study, which involved an examination of WISE data covering the entire sky in infrared light, found no object the size of Saturn or larger exists out to a distance of 10,000 astronomical units (au), and no object larger than Jupiter exists out to 26,000 au. One astronomical unit equals 93 million miles. Earth is 1 au, and Pluto about 40 au, from the sun.
"The outer solar system probably does not contain a large gas giant planet, or a small, companion star," said Kevin Luhman of the Center for Exoplanets and Habitable Worlds at Penn State University, University Park, Pa., author of a paper in the Astrophysical Journal describing the results.
But searches of the WISE catalog are not coming up empty. A second study reveals several thousand new residents in our sun's "backyard," consisting of stars and cool bodies called brown dwarfs.
"Neighboring star systems that have been hiding in plain sight just jump out in the WISE data," said Ned Wright of the University of California, Los Angeles, the principal investigator of the mission.
The second WISE study, which concentrated on objects beyond our solar system, found 3,525 stars and brown dwarfs within 500 light-years of our sun.
"We're finding objects that were totally overlooked before," said Davy Kirkpatrick of NASA's Infrared and Processing Analysis Center at the California Institute of Technology, Pasadena, Calif. Kirkpatrick is lead author of the second paper, also in the Astrophysical Journal. Some of these 3,525 objects also were found in the Luhman study, which catalogued 762 objects.
The WISE mission operated from 2010 through early 2011, during which time it performed two full scans of the sky -- with essentially a six-month gap between scans. The survey captured images of nearly 750 million asteroids, stars and galaxies. In November 2013, NASA released data from the AllWISE program, which now enables astronomers to compare the two full-sky surveys to look for moving objects.
In general, the more an object in the WISE images appears to move over time, the closer it is. This visual clue is the same effect at work when one observes a plane flying low to the ground versus the same plane flying at higher altitude. Though traveling at the same speed, the plane at higher altitude will appear to be moving more slowly.
Searches of the WISE data catalog for these moving objects are uncovering some of the closest stars. The discoveries include a star located about 20 light-years away in the constellation Norma, and as reported last March, a pair of brown dwarfs only 6.5 light-years away -- making it the closest star system to be discovered in nearly a century.
Despite the large number of new solar neighbors found by WISE, "Planet X" did not show up. Previous speculations about this hypothesized body stemmed in part from geological studies that suggested a regular timing associated with mass extinctions on Earth. The idea was that a large planet or small star hidden in the farthest reaches of our solar system might periodically sweep through bands of outer comets, sending them flying toward our planet. The Planet X-based mass extinction theories were largely ruled out even prior to the new WISE study.
Other theories based on irregular comet orbits had also postulated a Planet X-type body. The new WISE study now argues against these theories as well.
Both of the WISE searches were able to find objects the other missed, suggesting many other celestial bodies likely await discovery in the WISE data.
"We think there are even more stars out there left to find with WISE. We don't know our own sun's backyard as well as you might think," said Wright.
WISE was put into hibernation upon completing its primary mission in 2011. In September 2013, it was reactivated, renamed NEOWISE and assigned a new mission to assist NASA's efforts to identify the population of potentially hazardous near-Earth objects. NEOWISE will also characterize previously known asteroids and comets to better understand their sizes and compositions.
JPL managed and operated WISE for NASA's Science Mission Directorate. The mission was selected competitively under NASA's Explorers Program managed by the agency's Goddard Space Flight Center in Greenbelt, Md. The science instrument was built by the Space Dynamics Laboratory in Logan, Utah. The spacecraft was built by Ball Aerospace & Technologies Corp. in Boulder, Colo. Science operations and data processing take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA. More information is online
NASA
Guillermo Gonzalo Sánchez Achutegui

NASA: NASA Radar Demonstrates Ability to Foresee Sinkholes


Aerial photo of a 25-acre sinkhole that formed unexpectedly near Bayou Corne, La., in Aug. 2012.
Aerial photo of a 25-acre sinkhole that formed unexpectedly near Bayou Corne, La., in Aug. 2012.
Image Credit:
On Wings of Care, New Orleans, La.
Analyses by NASA's UAVSAR after the Bayou Corne, La., sinkhole formed show it detected precursory ground movement of up to 10.2 inches (260 millimeters) more than a month before the sinkhole collapsed. Colors represent surface displacement (one full color wrap equals 4.7 inches (120 millimeters).
Image Credit: NASA/JPL-Caltech
Sinkhole map
Sinkholes are common hazards worldwide and are found in all regions of the United States. This map shows parts of the United States where certain rock types are susceptible to dissolving in water, leading to the formation of underground cavities that can result in sinkholes.
Image Credit:
U.S. Geological Survey
New analyses of NASA airborne radar data collected in 2012 reveal the radar detected indications of a huge sinkhole before it collapsed and forced evacuations near Bayou Corne, La. that year.

The findings suggest such radar data, if collected routinely from airborne systems or satellites, could at least in some cases foresee sinkholes before they happen, decreasing danger to people and property.
Sinkholes are depressions in the ground formed when Earth surface layers collapse into caverns below. They usually form without warning. The data were collected as part of an ongoing NASA campaign to monitor sinking of the ground along the Louisiana Gulf Coast.
Researchers Cathleen Jones and Ron Blom of NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif., analyzed interferometric synthetic aperture radar (InSAR) imagery of the area acquired during flights of the agency's Uninhabited Airborne Vehicle Synthetic Aperture Radar (UAVSAR), which uses a C-20A jet, in June 2011 and July 2012. InSAR detects and measures very subtle deformations in Earth's surface.
Their analyses showed the ground surface layer deformed significantly at least a month before the collapse, moving mostly horizontally up to 10.2 inches (260 millimeters) toward where the sinkhole would later form. These precursory surface movements covered a much larger area -- about 1,640 by 1,640 feet, (500 by 500 meters) -- than that of the initial sinkhole, which measured about 2 acres (1 hectare).
Results of the study are published in the February issue of the journal Geology.
"While horizontal surface deformations had not previously been considered a signature of sinkholes, the new study shows they can precede sinkhole formation well in advance," said Jones. "This kind of movement may be more common than previously thought, particularly in areas with loose soil near the surface."
The Bayou Corne sinkhole formed unexpectedly Aug. 3, 2012, after weeks of minor earthquakes and bubbling natural gas that provoked community concern. It was caused by the collapse of a sidewall of an underground storage cavity connected to a nearby well operated by Texas Brine Company and owned by Occidental Petroleum. On-site investigation revealed the storage cavity, located more than 3,000 feet (914 meters) underground, had been mined closer to the edge of the subterranean Napoleonville salt dome than thought. The sinkhole, which filled with slurry --a fluid mixture of water and pulverized solids-- has gradually expanded and now measures about 25 acres (10.1 hectares) and is at least 750 feet (229 meters) deep. It is still growing.
"Our work shows radar remote sensing could offer a monitoring technique for identifying at least some sinkholes before their surface collapse, and could be of particular use to the petroleum industry for monitoring operations in salt domes," said Blom. "Salt domes are dome-shaped structures in sedimentary rocks that form where large masses of salt are forced upward. By measuring strain on Earth's surface, this capability can reduce risks and provide quantitative information that can be used to predict a sinkhole's size and growth rate."
Typically, sinkholes have no natural external surface drainage, and they form through natural processes and human activities. They occur in regions of "karst" terrain where the rock below the surface can be dissolved by groundwater, most commonly in areas with limestone or other carbonate rocks, gypsum, or salt beds. When the rocks dissolve, they form spaces and caverns underground. Sinkholes vary in size from a few feet across to hundreds of acres, and some can be very deep. They are common hazards worldwide and are found in all regions of the United States, with Florida, Missouri, Texas, Alabama, Kentucky, Tennessee and Pennsylvania reporting the most sinkhole damage. While sinkhole deaths are rare, in February 2013 a man in Tampa, Fla., was killed when his house was swallowed by a sinkhole.
The human-produced Bayou Corne sinkhole occurred in an area not prone to sinkholes. The Gulf Coast of Louisiana and eastern Texas sits on an ancient ocean floor with salt layers that form domes as the lower-density salt rises. The Napoleonville salt dome underneath Bayou Corne extends to within 690 feet (210 meters) of the surface. Various companies mine caverns in the dome by dissolving the salt to obtain brine and subsequently store fuels and salt water in the caverns.
Jones and Blom say continued UAVSAR monitoring of the area as recently as October 2013 has shown a widening area of deformation, with the potential to affect other nearby storage cavities located near the salt dome's outer wall. Because the Bayou Corne sinkhole is now filled with water, it is harder to measure deformation of the area using InSAR. However, if the deformation extends far past the sinkhole boundaries, InSAR could continue to track surface movement caused by changes below the surface.
Continued growth of the sinkhole threatens the community and Highway 70, so there is a pressing need for reliable estimates of how fast it may expand and how big it may eventually get.
"This kind of data could be of great value in determining the direction in which the sinkhole is likely to expand," said Jones. "At Bayou Corne, it appears that material is continuing to flow into the huge cavern that is undergoing collapse."
Blom says there are no immediate plans to fly UAVSAR over sinkhole-prone areas.
"You could spend a lot of time flying and processing data without capturing a sinkhole," he said. "Our discovery at Bayou Corne was really serendipitous. But it does demonstrate one of the expected benefits of an InSAR satellite that would image wide areas frequently.
"Every year, unexpected ground motions from sinkholes, landslides and levee failures cost millions of dollars and many lives," said Jones. "When there is small movement prior to a catastrophic collapse, such subtle precursory clues can be detected by InSAR."
NASA monitors Earth's vital signs from land, air and space with a fleet of satellites and ambitious airborne and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.
For more information about UAVSAR, visit:
For more information about NASA's Earth science activities in 2014, visit:
For information on the latest NASA Earth science findings, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

martes, 4 de marzo de 2014

nsf.gov - National Science Foundation - New bilateral pilot opportunity will fund collaborations between US and UK bioscience researchers

Proposals on systems biology, computational biology, bioinformatics and synthetic biology are eligible for consideration for joint US/UK funding
flags of the United States and the United Kingdom
U.S./U.K. research teams may now seek joint U.S./U.K. funding through a simplified mechanism.
Credit and Larger Version
March 4, 2014
A new, two-year pilot opportunity--known as The U.S. NSF/BIO-UK BBSRC Lead Agency Pilot Opportunity--is being formally launched today.
This Pilot opportunity is designed to make it easier for research teams comprised of scientists from the United States and the United Kingdom to manage funding logistics and to simultaneously obtain funding from both countries. It is funded by the U.S. National Science Foundation's (NSF) Directorate for Biological Sciences and the U.K.'s Biotechnology and Biological Sciences Research Council (BBSRC).
This Pilot opportunity will use a simplified, flexible review process that will allow U.S./U.K. research teams to submit a single proposal that will undergo a single review process by only one of the partner agencies. Successful proposals will be funded by both NSF and the BBSRC.
Cora B. Marrett, acting director of NSF, said, "Although NSF has always funded U.S. scientists involved in international collaborations, such collaborations have become increasingly important, partly because of the rapid globalization of research. The many benefits of this Pilot opportunity will include better coordination of funding for U.S./U.K. research teams and increased bilateral awareness of scientific strengths and advancements between the U.S. and U.K. funding agencies."
Jackie Hunter, BBSRC chief executive, said, "Partnerships are vital to U.K. bioscience, offering the opportunity to combine resources and expertise to tackle global challenges. As funders, we are working to reduce some of the barriers encountered by researchers when working with international partners. This pilot is an important step that will help to streamline the collaborative funding process between NSF and BBSRC, making applications easier for those in our community working with the U.S."
The Pilot opportunity was created under a Memorandum of Understanding between NSF and the U.K.'s research councils, which support research partnerships between the two countries. The Pilot opportunity is designed to reduce obstacles that have traditionally been faced by researchers wishing to form international teams. These obstacles include identifying appropriate funding agencies; risking "double jeopardy," where one country's funding agency decides to fund an international team's research proposal, but the partner country does not; and dealing with the different timetables of different funding agencies.
The first step in applying for funding under The Pilot opportunity will be for each research team to select a lead agency based on whether its proposed research would fall more within the scope of NSF'S Directorate for Biological Sciences or that of the BBSRC. Then, each team will submit to its proposed lead agency an Intention to Submit (ITS) that summarizes its proposed research, funding request and other associated information. These documents will be reviewed in August 2014 and August 2015.
Based on each team's ITS, the team's lead agency will determine whether the team will be invited to submit a full proposal. Full proposals will be reviewed in fall 2014 and fall 2015; these reviews will be conducted according to the review criteria of each team's lead agency. Proposals that cover systems biology, computational biology, bioinformatics and synthetic biology (the latter, only for fall 2015 submissions) will be eligible for consideration.
Although the review criteria of NSF and BBSRC are not identical, both agencies' criteria include evaluations by invited reviewers on proposals' scientific or intellectual merit as well as on their broader societal impacts. The decision made by the lead agency on each proposal will be discussed with the partner agency. If a research team receives an award, its U.S. researchers will be funded by NSF, and its U.K. researchers will be funded by the BBSRC.
More information about The U.S. NSF/BIO-UK BBSRC Lead Agency Pilot Opportunity, including submission deadlines, is provided in NSF's Dear Colleague Letter and on the BBSRC's website, which features its Management Plan for the pilot opportunity.
-NSF-
Media Contacts Lily Whiteman, National Science Foundation, (703) 292-8310,
lwhitema@nsf.gov
Robert Dawson, Biotechnology and Biological Sciences Research Council of U.K., 01793413204, robert.dawson@bbsrc.ac.uk
Program Contacts James Deshler, National Science Foundation, (703) 292-7871,
The National Science Foundation (NSF) is an independent federal agency that supports fundamental research and education across all fields of science and engineering. In fiscal year (FY) 2014, its budget is $7.2 billion. NSF funds reach all 50 states through grants to nearly 2,000 colleges, universities and other institutions. Each year, NSF receives about 50,000 competitive requests for funding, and makes about 11,500 new funding awards. NSF also awards about $593 million in professional and service contracts yearly.
Useful NSF Web Sites:
NSF Home Page: http://www.nsf.gov
NSF News: http://www.nsf.gov/news/
For the News Media: http://www.nsf.gov/news/newsroom.jsp
Science and Engineering Statistics: http://www.nsf.gov/statistics/
Awards Searches: http://www.nsf.gov/awardsearch/
The National Science Foundation (NSF)
Guillermo Gonzalo Sánchez Achutegui