Saturday, June 14, 2014

NASA Turns World Cup into Lesson in Aerodynamics

NASA Turns World Cup into Lesson in Aerodynamics
June 12, 2014

Dr. Rabi Mehta uses smoke and lasers to inspect the flow pattern around an Adidas Brazuca football.
Image Credit: NASA's Ames Research Center
Excitement is building for fans across the globe with today’s first match of the Fédération Internationale de Football Association (FIFA) 2014 World Cup tournament. These fans include NASA engineers, who used the lead-up to the tournament to test the aerodynamics of this year’s new ball design, developed by Adidas and dubbed the Brazuca ball.
Although NASA is not in the business of designing or testing balls, the tournament provides an opportunity to explain the concepts of aerodynamics to students and individuals less familiar with the fundamentals of aerodynamics.

World Cup ball being tested at NASA Ames Research Center (no narration)
Image Credit: NASA's Ames Research Center
“Sports provide a great opportunity to introduce the next generation of researchers to our field of aerodynamics by showing them something they can relate to,” said Rabi Mehta, chief of the Experimental Aero-Physics Branch at NASA's Ames Research Center in Moffett Field, California.
Aerodynamics is the study of how air and liquids, referred to collectively as "fluids" in aerodynamics research, flow around objects. Engineers at Ames, a world leader in fundamental aerodynamics research, possess an in-depth understanding of how fluids flow around simple three-dimensional shapes such as cylinders and spheres. With this knowledge, engineers can predict how even the minor alterations in these basic shapes change flow patterns.
The previous World Cup ball, the Jabulani, was described as sometimes demonstrating "supernatural" movements. It was beloved by strikers but hated by goalkeepers because, when kicked with little or no spin, the ball "knuckled," giving strikers a greater chance of scoring. Knuckling occurs when, at zero or near-zero spin, the seams of the ball channel airflow in an unusual and erratic manner making its trajectory unpredictable.

Dr. Rabi Mehta and Christina Ngo view a test of a of a traditional 32-panel football scale-model in the 17-inch water channel. Flow patterns are visualized using florescent dye and black lights.
Image Credit: NASA's Ames Research Center
Taking full advantage of a ball’s flight characteristics to gain an advantage is nothing new in sports. In baseball, the only difference between a curveball, a fastball, a slider or a knuckle ball is how a pitcher manipulates the spin of the baseball with respect to its stiches. On a football, there are no external stiches piecing the outer covering of the ball together but it does have seams, many of them.
To address the unpredictability of the Jabulani ball, Adidas worked with hundreds of players to develop the Brazuca football. A traditional football has 32 panels, the Jabulani has eight panels and the Brazuca has only six.

A scale model of the 32-panel ball in Ames' water channel. The green dye shows the water flow around the object. The pink dye is injected separately just behind the ball to show the position of the low-pressure zone behind the ball.
Image Credit: NASA's Ames Research Center
Despite having fewer panels, the finger-like panels on the Brazuca increase the seam length, compared to previous World Cup balls. The seams are also deeper than those of the Jabulani and the panels are covered with tiny bumps; all of these factors influence the ball’s aerodynamics.

A close up of the Brazuca ball in Ames' Fluid Mechanics Laboratory's two-foot by two-foot wind tunnel. Smoke highlighted by lasers visualizes air flow around the ball.
Image Credit: NASA's Ames Research Center
What seems like common sense about air moving around a simple sphere does not, in fact, bear true. The airflow around a sphere is not smooth; a great amount of drag is created behind the object. An example of this can be seen on a golf course, where a smooth golf ball travels much shorter distances than a regular, dimpled golf ball. The dimples on the ball’s surface agitate the air creating a smaller low-pressure wake behind the ball and decreasing drag, therefore increasing its distance.
“There is a thin layer of air that forms near the ball’s surface called the boundary layer and it is the state and behavior of that layer that is critical to the performance of the ball,” said Mehta. “The materials used, the ball’s surface roughness and its distribution determines its aerodynamics.”
The overall increased roughness of the Brazuca football will help to decrease the ball’s knuckling tendencies at kicking speeds typically encountered in the World Cup.
In the 2-by 2-foot wind tunnel in the Fluid Mechanics Laboratory at Ames, Mehta demonstrates the airflow around the Brazuca football releasing controlled smoke flow over the surface of the ball highlighted with laser light to increase flow visibility. At different speeds, there are noticeable differences in airflow around the ball.
“What we are looking for in the smoke patterns is at what speed the smoke patterns suddenly change,” remarked Mehta. This is when the knuckling effect is greatest.”
Tests in the wind tunnel and a 17-inch water channel, which uses florescent dye dispensed into the fluid flow under black lights, shows that the speed of greatest knuckling for a traditional ball is around 30 miles per hour (mph). This is well below the typical kicking speed of a World Cup-caliber player, which is about 50 to 55 mph. Interestingly, the Jabulani, a much smoother ball, produced its greatest knuckling effect in that same speed range (about 50 mph), which is why the players in the 2010 World Cup noticed  the effect more frequently.
The smoother a ball is, the higher the speed at which the knuckling effect occurs. However, with the increased roughness of the Brazuca, this critical speed for maximum knuckling is reduced to about 30 mph. So it is expected that the 2014 World Cup ball will have a more predictable flight path at typical striking speeds.
“The players should be happier with the new ball,” predicted Mehta. “It is more stable in flight and will handle more like a traditional 32-panel ball.”
Will this make the game less exciting? The answer is -- no. With a new understanding of the aerodynamics of the Brazuca football, the audience, especially kids, can better appreciate the feats of skill on the field. Elite athletes will continue to manipulate the ball in amazing ways. They don’t have the terms like “Bend it like Beckham” for nothing.
GOOOOOOAAAAAAL!

Thursday, March 20, 2014

NASA Launches Its Third Global 'Codeathon' with New Coastal Flooding Challenge



March 19, 2014
RELEASE 14-075
NASA Launches Its Third Global 'Codeathon' with New Coastal Flooding Challenge
NASA Chief Scientist Ellen Stofan
NASA Chief Scientist Ellen Stofan spoke Wednesday at the White House Climate Data Initiative launch, during which she announced the third International Space Apps Challenge.
Image Credit: 
NASA/Aubrey Gemignani
NASA along with space agencies around the world are preparing for the third annual International Space Apps Challenge, which will be held April 12-13. Participants will develop mobile applications, software, hardware, data visualization and platform solutions that could contribute to space exploration missions and help improve life on Earth.
At the Climate Data Initiative launch at the White House Wednesday, NASA Chief Scientist Ellen Stofan announced the inclusion of a new challenge focused on coastal flooding, developed by NASA and NOAA, and based on federal cross-agency data. The Coastal Inundation in Your Community challenge is one of four climate-related challenges using data provided by NASA, the National Oceanic and Atmospheric Administration (NOAA) and the Environmental Protection Agency (EPA).
The challenge encourages entrepreneurs, technologists, and developers to create and deploy data-driven visualizations and simulations that will help people understand their exposure to coastal-inundation hazards and other vulnerabilities.
“Solutions developed through this challenge could have many potential impacts,” said Stofan. "This includes helping coastal businesses determine whether they are currently at risk from coastal inundation, and whether they will be impacted in the future by sea level rise and coastal erosion."
The two-day International Space Apps Challenge will be a “codeathon”-style event locally hosted at almost 100 locations spanning six continents. More than 200 data sources, including data sets, data services, and tools will be made available. This event will bring tech-savvy citizens, scientists, entrepreneurs, educators, and students together to help solve challenges relevant to both space exploration and social needs.
"The International Space Apps Challenge is one of the U.S. commitments to the Open Government Partnership to explore new ways that open space data can help the planet and further space exploration," said Deborah Diaz, deputy chief information officer at NASA Headquarters in Washington.
This year, more than 40 new challenges will represent NASA mission priorities and be organized in five themes: Earth Watch, Technology in Space Human Spaceflight, Robotics, and Asteroids. About half of the challenges are in the Earth Watch theme, which supports NASA's focus on Earth science in 2014.
For the first time in more than a decade, five NASA Earth science missions are being launched into space in the same year, opening new and improved remote eyes to monitor our changing planet. 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.

Climate Data Initiative Launches; Challenge Announced At the Climate Data Initiative launch at the White House Wednesday, NASA Chief Scientist Ellen Stofan announced a new challenge -- Coastal Inundation in Your Community -- focused on coastal flooding, developed by NASA and NOAA, and based on federal cross-agency data.


Climate Data Initiative Launches; Challenge Announced

At the Climate Data Initiative launch at the White House Wednesday, NASA Chief Scientist Ellen Stofan announced a new challenge -- Coastal Inundation in Your Community -- focused on coastal flooding, developed by NASA and NOAA, and based on federal cross-agency data.

Tuesday, March 18, 2014

NASA's STEREO Studies Extreme Space Weather


NASA's STEREO Studies Extreme Space Weather
March 18, 2014
Scientists studied this unusually fast coronal mass ejection – shown here in a movie from NASA's STEREO-A from July 22, 2012, at 10:00 p.m. EDT until 2 a.m. on July 23 – to improve models of extreme space weather. Because the CME headed toward STEREO-A, it appears like a giant halo around the sun.
Image Credit: 
NASA/STEREO/Helioviewer
On July 22, 2012, a massive cloud of solar material erupted off the sun's right side, zooming out into space and passing one of NASA's twin Solar Terrestrial Relations Observatory, or STEREO, spacecraft along the way. Scientists clocked this giant cloud, known as a coronal mass ejection, or CME, as traveling over 1,800 miles per second as it left the sun.
Conversations began to buzz and the emails to fly: this was the fastest CME ever observed by STEREO, which since its launch in 2006 has helped make CME speed measurements much more precise. Measuring a CME at this speed, traveling in a direction safely away from Earth, represented a fantastic opportunity for researchers studying the sun's effects. Now, a paper in Nature Communications, published on March 18, 2014, describes how a combination of events worked together to create these incredible speeds.
"The authors believe this extreme event was due to the interaction of two CMEs separated by only 10 to 15 minutes," said Joe Gurman, project scientist for STEREO at NASA's Goddard Space Flight Center in Greenbelt, Md. "Plus the CMEs traveled through a region of space that had been cleared out by another CME four days earlier."
STEREO A sees 1,800 mps cme.
This image captured on July 23, 2012, at 12:24 a.m. EDT, shows a coronal mass ejection that left the sun at the unusually fast speeds of over 1,800 miles per second.
Image Credit: 
NASA/STEREO
The researchers describe the July 2012 event as a perfect storm, referring to the phrase originally coined for the October 1991 Atlantic Ocean storm to describe an event where a rare combination of circumstances can drastically aggravate a situation.
Such work helps scientists understand how extreme solar events form and what their effects might be if aimed toward Earth. At Earth, the harshest space weather can have strong effects on the magnetic system surrounding the planet, which in turn can affect satellites and interrupt GPS and radio communications. At its worst, rapidly changing magnetic field lines around Earth can induce electric surges in the power utility grids on the ground. One of the best ways to protect against such problems, and perhaps learn to predict the onset of one of these storms, is to make computer models matching the observations of past events.
In the case of the July 2012 event, three spacecraft offered data on the CMEs: the two STEREO spacecraft and the joint European Space Agency/NASA Solar and Heliospheric Observatory, or SOHO. SOHO lies between Earth and the sun, while the two STEREO spacecraft have orbits that for most of their journey give views of the sun that cannot be had from Earth. Each spacecraft observed the CMEs from a different angle, and together they could help map out a three-dimensional image of what happened.
The authors suggest it was the successive, one-two punch of the CMEs that was the key to the high speeds of the event – speeds that would lead to circling Earth five times in one minute.  A CME from four days earlier had an impact too. First, it swept aside particles in the way, making it all the easier for the next CMEs to travel.  Second, it altered the normal spiral of the magnetic fields around the sun to a straighter pattern above the region that was the source for these CMEs, thus allowing for freer movement.
"A key finding is that it’s not just the initial conditions on the sun that can produce an extreme space weather storm," said Gurman. "The interactions between successive coronal mass ejections farther out in interplanetary space need to be considered as well."
The researchers found that state-of-the-art models that didn't take the effects of successive CMEs into consideration failed to correctly simulate the July 2012 event.  Such information will be incorporated into the models being tested by space weather forecasters. This should lead to better predictions of the worst storms and better protection of Earth and our technology in space.
Related Links

STEREO Spacecraft Studies Extreme Space Weather

STEREO Spacecraft Studies Extreme Space Weather

On July 22, 2012, a massive cloud of solar material erupted off the sun's right side, zooming out into space and passing one of NASA's twin Solar Terrestrial Relations Observatory, or STEREO, spacecraft along the way. Scientists clocked this giant cloud, known as a coronal mass ejection, or CME, as traveling over 1,800 miles per second as it left the sun. This was the fastest CME ever observed by STEREO, which since its launch in 2006 has helped make CME speed measurements much more precise.

NASA Releases First Interactive Mosaic of Lunar North Pole


NASA Releases First Interactive Mosaic of Lunar North Pole
Interactive mosaic from NASA's Lunar Reconnaissance Orbiter
A new interactive mosaic from NASA's Lunar Reconnaissance Orbiter covers the north pole of the moon from 60 to 90 degrees north latitude at a resolution of 6-1/2 feet (2 meters) per pixel. Close-ups of Thales crater (right side) zoom in to reveal increasing levels of detail.
Image Credit: 
NASA/GSFC/Arizona State University
Scientists, using cameras aboard NASA's Lunar Reconnaissance Orbiter (LRO), have created the largest high resolution mosaic of our moon’s north polar region. The six-and-a-half feet (two-meters)-per-pixel images cover an area equal to more than one-quarter of the United States.
Web viewers can zoom in and out, and pan around an area. Constructed from 10,581 pictures, the mosaic provides enough detail to see textures and subtle shading of the lunar terrain. Consistent lighting throughout the images makes it easy to compare different regions.
"This unique image is a tremendous resource for scientists and the public alike," said John Keller, LRO project scientist at NASA's Goddard Space Flight Center, Greenbelt, Md. "It's the latest example of the exciting insights and data products LRO has been providing for nearly five years."
The images making up the mosaic were taken by the two LRO Narrow Angle Cameras, which are part of the instrument suite known as the Lunar Reconnaissance Orbiter Camera (LROC). The cameras can record a tremendous dynamic range of lit and shadowed areas.
"Creation of this giant mosaic took four years and a huge team effort across the LRO project," said Mark Robinson, principal investigator for the LROC at Arizona State University in Tempe. "We now have a nearly uniform map to unravel key science questions and find the best landing spots for future exploration."
The entire image measures 931,070 pixels square – nearly 867 billion pixels total. A complete printout at 300 dots per inch – considered crisp resolution for printed publications – would require a square sheet of paper wider than a professional U.S. football field and almost as long. If the complete mosaic were processed as a single file, it would require approximately 3.3 terabytes of storage space. Instead, the processed mosaic was divided into millions of small, compressed files, making it manageable for users to view and navigate around the image using a web browser.
LRO entered lunar orbit in June 2009 equipped with seven instrument suites to map the surface, probe the radiation environment, investigate water and key mineral resources, and gather geological clues about the moon's evolution.
Researchers used additional information about the moon's topography from LRO's Lunar Orbiter Laser Altimeter, as well as gravity information from NASA's Gravity Recovery and Interior Laboratory (GRAIL) mission, to assemble the mosaic. Launched in September 2011, the GRAIL mission, employing twin spacecraft named Ebb and Flow, generated a gravity field map of the moon -- the highest resolution gravity field map of any celestial body.
LRO is managed by Goddard for the Science Mission Directorate (SMD) at NASA Headquarters in Washington. LROC was designed and built by Malin Space Science Systems and is operated by the University of Arizona. NASA's Jet Propulsion Laboratory in Pasadena, Calif., managed the GRAIL mission for SMD.
For more information about LRO, visit:
To access the complete collection of LROC images, visit:
To view the image with zoom and pan capability, visit: