domingo, 19 de octubre de 2014

NASA : NASA Begins Sixth Year of Airborne Antarctic Ice Change Study

Hola amigos: AL VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa sobre sus estudios en la Antártica sobre que  comienza Sexto Año de Airborne Antártida Estudio Cambio de Hielo. Ellos dicen..."NASA está llevando a cabo su sexto año consecutivo de vuelos de investigación Operación IceBridge sobre la Antártida para estudiar los cambios en la capa de hielo del continente, glaciares y hielo marino. Campaña aérea de este año, que comenzó su primer vuelo la mañana del jueves, volverá a examinar una sección de la capa de hielo de la Antártida que hace poco se encontró que en un declive irreversible.........
Para las próximas semanas, los investigadores volarán a bordo de aviones de investigación de la NASA DC-8 de Punta Arenas, Chile. Este año también marca el regreso de la Antártida occidental tras la campaña de 2013 con base en la estación McMurdo de la Fundación Nacional de Ciencia.....
NASA’s DC-8 research aircraft will be flying scientists and instruments over Antarctica to study changes in the continent’s ice sheet, glaciers and sea ice.
NASA’s DC-8 research aircraft will be flying scientists and instruments over Antarctica to study changes in the continent’s ice sheet, glaciers and sea ice.
Image Credit: 
NASA
 
NASA is carrying out its sixth consecutive year of Operation IceBridge research flights over Antarctica to study changes in the continent’s ice sheet, glaciers and sea ice. This year’s airborne campaign, which began its first flight Thursday morning, will revisit a section of the Antarctic ice sheet that recently was found to be in irreversible decline.
For the next several weeks, researchers will fly aboard NASA’s DC-8 research aircraft out of Punta Arenas, Chile. This year also marks the return to western Antarctica following 2013’s campaign based at the National Science Foundation’s McMurdo Station.
“We are curious to see how much these glaciers have changed in two years,” said Eric Rignot, IceBridge science team co-lead and glaciologist at the University of California, Irvine and NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California.
IceBridge will use a suite of instruments that includes a laser altimeter, radar instruments, cameras, and a gravimeter, which is an instrument that detects small changes in gravity. These small changes reveal how much mass these glaciers have lost. Repeated annual measurements of key glaciers maintains a long-term record of change in the Antarctic that goes back to NASA’s Ice, Cloud and Land Elevation Satellite (ICESat) which stopped collecting data in 2009.
IceBridge researchers plan to measure previously unsurveyed regions of Antarctica. One example is a plan to look at the upper portions of Smith Glacier in West Antarctica, which is thinning faster than any other glaciers in the region. The mission also plans to collect data in portions of the Antarctic Peninsula, such as the Larsen C, George VI and Wilkins ice shelves and the glaciers that drain into them. The Antarctic Peninsula has been warming faster than the rest of the continent.
“The Antarctic Peninsula is changing fairly rapidly and we need to be there to capture that change,” said Michael Studinger, IceBridge project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
The mission also will collect data on Antarctic sea ice, which recently reached a record high coverage. This contrasts with declining sea ice in the Arctic and is due do a variety of factors such as changing wind patterns. Antarctic sea ice coverage is slightly above average and the growth varies from one part of Antarctica to another. For example, ice cover in the Bellingshausen Sea has been decreasing while ice in the nearby Ross Sea is growing.
“There are very strong regional variations on how sea ice is changing,” said Nathan Kurtz, a sea ice scientist at Goddard. These regional trends together yield a small increase, so studying each region will help scientists get a better grasp on the processes affecting sea ice there.
In addition to extending ICESat’s data record over land and sea ice, IceBridge will also help set the stage for ICESat-2 by measuring ice the satellite will fly over. One of IceBridge’s highest priority surveys is a circular flight the DC-8 will fly around the South Pole at 88 degrees south latitude. This latitude line is where all of ICESat-2’s orbits will converge in the Southern Hemisphere. Measuring ice elevation at these locations will help researchers build a time series of data that spans more than a decade and provide a way to help verify ICESat-2’s data.
IceBridge’s Antarctic field campaign will run through late November. The IceBridge project science office is based at Goddard. The DC-8 research aircraft is based at NASA’s Armstrong Flight Research Center’s facility in Palmdale, California.
For more about Operation IceBridge, visit:
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 NASA's recent Earth science activities, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

nsf.gov - National Science Foundation - Halting the spread of Ebola: Case of Nigeria a model for quick action, scientists find

Hola amigos: A VUELO DE UN QUINDE EL BLOG., la Fundación Nacional de Ciencia de Los Estados Unidos, nos informa sobre las investigaciones  que se están contra el Virus del Ébola en Nigeria...."Ebola. La palabra trae temor a un enemigo invisible y potencialmente letal. Pero hay formas de detener su propagación, dicen los científicos en enfermedades infecciosas.
Se requiere una intervención rápida, de acuerdo con los investigadores, quienes recientemente publicaron sus hallazgos en la revista Eurosurveillance.
Analizar casos de Ébola en Nigeria, un país con éxito en la contención de la enfermedad, los científicos estima que la tasa de mortalidad, la progresión de la transmisión, la proporción de trabajadores de la salud infectados, y el efecto de las intervenciones de control del tamaño de la epidemia......................
Rapid control measures critical to stopping the virus in its tracks
health workers in biohazard gear
Stopping Ebola in its tracks calls for rapid control measures in Africa and elsewhere.
Credit and Larger Version
October 16, 2014
The following is part ten in a series on the NSF-NIH-USDA Ecology and Evolution of Infectious Diseases (EEID) Program. See parts: one, two, three, four, five, six, seven, eight and nine.
Ebola. The word brings fear of an unseen and potentially lethal enemy. But there are ways to stop its spread, say infectious disease scientists.
Quick intervention is needed, according to the researchers, who recently published their findings in the journal Eurosurveillance.
Analyzing Ebola cases in Nigeria, a country with success in containing the disease, the scientists estimated the rate of fatality, transmission progression, proportion of health care workers infected, and the effect of control interventions on the size of the epidemic.
 
Rapid response needed
 
"Rapid control is necessary, as is demonstrated by the Nigerian success story," says Arizona State University (ASU) scientist Gerardo Chowell, senior author of the paper.
"This is critically important for countries in the West Africa region that are not yet affected by the Ebola epidemic, as well as for countries in other regions of the world that risk importation of the disease."
The research is funded by the U.S. National Science Foundation (NSF)-National Institutes of Health (NIH)-Department of Agriculture (USDA) Ecology and Evolution of Infectious Diseases (EEID) Program.
"Controlling a deadly disease like Ebola requires understanding how it's likely to spread, and knowing the ways of managing that spread that are most likely to be effective," says Sam Scheiner, NSF EEID program director.
"Being able to respond quickly needs a foundation of knowledge acquired over many years. The work of these scientists is testimony to long-term funding by the EEID program."
 
Control measures in Nigeria
 
The largest Ebola outbreak to date is ongoing in West Africa, with more than 8,000 reported cases and 4,000 deaths. However, just 20 Ebola cases have been reported in Nigeria, with no new cases since early September.
All the cases in Nigeria stem from a single traveler returning from Liberia in July.
The study used epidemic modeling and computer simulations to project the size of the outbreak in Nigeria if control interventions had been implemented during various time periods after the initial case, and estimated how many cases had been prevented by the actual early interventions.
"This timely work demonstrates how computational simulations, informed by data from health care officials and the complex social web of contacts and activities, can be used to develop both preparedness plans and response scenarios," says Sylvia Spengler, program director in NSF's Directorate for Computer and Information Science and Engineering, which also supported the research.
Control measures implemented in Nigeria included holding all people showing Ebola symptoms in an isolation ward if they had had contact with the initial case. If Ebola was confirmed through testing, people diagnosed with the disease were moved to a treatment center.
Asymptomatic individuals were separated from those showing symptoms; those who tested negative without symptoms were discharged.
Those who tested negative but showed symptoms--fever, vomiting, sore throat and diarrhea--were observed and discharged after 21 days if they were then free of symptoms, while being kept apart from people who had tested positive.
 
Brief window of opportunity
 
Ebola transmission is dramatically influenced by how rapidly control measures are put into place.
"Actions taken by health authorities to contain the spread of disease sometimes can, perversely, spread it," says NSF-funded scientist Charles Perrings, also of ASU.
"In the Nigeria case, people who tested negative but had some of the symptoms were not put alongside others who tested positive," says Perrings. "So they had no incentive to flee, and their isolation did nothing to increase infection rates. Elsewhere in the region isolation policies have had a different effect."
The researchers found that the projected effect of control interventions in Nigeria ranged from 15-106 cases when interventions are put in place on day 3; 20-178 cases when implemented on day 10; 23-282 cases on day 20; 60-666 cases on day 30; 39-1,599 cases on day 40; and 93-2,771 on day 50.
The person who was initially infected generated 12 secondary cases in the first generation of the disease; five secondary cases were generated from those 12 in the second generation; and two secondary cases in the third generation.
That leads to a rough estimate of the reproduction number according to disease generation declining from 12 during the first generation, to approximately 0.4 during the second and third disease generations.
A reproductive number above 1.0 indicates that the disease has the potential to spread.
Recent estimates of the reproduction number for the ongoing Ebola epidemic in Sierra Leone and Liberia range between 1.5 and 2 (two new cases for each single case), indicating that the outbreak has yet to be brought under control.
The effectiveness of the Nigerian response, scientists say, is illustrated by a dramatic decrease in the number of secondary cases over time.
The success story for Nigeria, they maintain, sets a hopeful example for other countries, including the United States.
Co-authors of the Eurosurveillance paper are Gerardo Chowell, Arizona State University; Folorunso Oludayo Fasina, University of Pretoria, South Africa; Aminu Shittu, Usmanu Danfodiyo University, Nigeria; David Lazarus, National Veterinary Research Institute, Plateau State, Nigeria; Oyewale Tomori, Nigerian Academy of Science, University of Lagos, Lagos, Nigeria; Lone Simonsen, George Washington University, Washington, D. C.; and Cecile Viboud, National Institutes of Health, Bethesda, Md.
-- Cheryl Dybas, NSF (703) 292-7734 cdybas@nsf.gov
-- Julie Newberg, ASU (480) 727-3116 julie.newberg@asu.edu
Related Programs Ecology and Evolution of Infectious Disease
Related WebsitesNSF Special Report: Ecology and Evolution of Infectious Diseases: http://www.nsf.gov/news/special_reports/ecoinf/
NSF Grant: US-UK Collab: Risks of Animal and Plant Infectious Diseases through Trade (RAPID Trade):
 http://www.nsf.gov/awardsearch/showAward?AWD_ID=1414374&HistoricalAwards=false
NSF Grant: III: Small: Data Management for Real-Time Data Driven Epidemic Spread Simulations: http://www.nsf.gov/awardsearch/showAward?AWD_ID=1318788&HistoricalAwards=false
NSF News: Outbreak: Ecology and Evolution of Infectious Disease grants support research on disease transmission:
 http://www.nsf.gov/news/news_summ.jsp?cntn_id=129280

Particles of the Ebola virus have found their way to several African countries--and beyond.
Credit and Larger Version
poster showing steps in global health security to stope ebola outbreak
Global health security depends on how fast an infection is recognized and brought under control.
Credit and Larger Version
Ebola virus, as seen under a transmission electron microscope.
Ebola, as seen under a transmission electron microscope.
Credit and Larger Version
Outbreak distribution map of Ebola in Africa, since its first known incidence.
Outbreak distribution map of Ebola in Africa, since its first known incidence.
Credit and Larger Version
graphic showing the ebola virus ecology
How does Ebola begin? To find answers, look to the ecology of infectious diseases.
Credit and Larger Versión
The National Science Foundation (NSF)
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

NASA : NASA TV to Air Russian Spacewalk from International Space Station

Hola amigos: AL VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, que nos dice: ...."NASA Television transmitirá la cobertura en vivo de una caminata espacial de seis horas por dos miembros de la tripulación rusa a bordo de la Estación Espacial Internacional a partir de las 9 am EDT Miércoles, 22 de octubre...........
Expedition 41 Commander Max Suraev and Flight Engineer Alexander Samokutyaev of the Russian Federal Space Agency will don Orlan spacesuits and step outside the International Space Station Wednesday, Oct. 22, to perform work on the exterior of the station's Russian modules.
Expedition 41 Commander Max Suraev and Flight Engineer Alexander Samokutyaev of the Russian Federal Space Agency will don Orlan spacesuits and step outside the International Space Station Wednesday, Oct. 22, to perform work on the exterior of the station's Russian modules.
Image Credit: 
NASA
NASA Television will broadcast live coverage of a six-hour spacewalk by two Russian crew members aboard the International Space Station beginning at 9 a.m. EDT Wednesday, Oct. 22.
Expedition 41 Commander Max Suraev and Flight Engineer Alexander Samokutyaev of the Russian Federal Space Agency will don Orlan spacesuits and exit the station’s Pirs airlock at 9:24 a.m. They will remove and jettison several pieces of hardware no longer needed on the Russian segment of the station and conduct a detailed photographic survey of the exterior surface of the Russian modules.
The spacewalk will be the 184th in support of space station assembly and maintenance, the third in as many weeks for Expedition 41 crew members, and the second career spacewalks for both Suraev and Samokutyaev.
Suraev will be designated as extravehicular (EV) crew member 1 and will wear an Orlan suit bearing red stripes. Samokutyaev will be designated as EV-2 and will wear a suit with blue stripes.
For NASA TV streaming video, schedule and downlink information, visit:
For more information about the International Space Station and its research and crews, visit:
 
NASA
Guillermo Gonzalo Sánchez Achutegui

NASA : NASA Spacecraft Provides New Information About Sun’s Atmosphere

Hola amigos: AL VUELO DE UN QUINDE EL BLOG., la Agencia Espacial NASA, nos informa que: NASA's Interface Region Imaging Spectrograph (IRIS); ha proporcionado a los científicos con cinco nuevos hallazgos sobre cómo la atmósfera del Sol, o corona, se calienta mucho más caliente que su superficie, lo que causa constante flujo de salida del sol de partículas llamado viento solar, y qué mecanismos aceleran partículas que alimentan las erupciones solares....
 
La nueva información ayudará a los investigadores a entender mejor cómo nuestra energía transferencias estrella más cercana a través de su atmósfera y realizar un seguimiento de la actividad solar dinámico que puede afectar a la infraestructura tecnológica en el espacio y en la Tierra. Los detalles de los hallazgos aparecen en la edición actual de la Ciencia.

  "Estos resultados revelan una región del Sol más complicado de lo que se pensaba anteriormente", dijo Jeff Newmark, director interino de la División de Heliofísica de la NASA en Washington. "La combinación de datos de IRIS con las observaciones de otras misiones Heliofísica está permitiendo grandes avances en nuestra comprensión del Sol y sus interacciones con el sistema solar."..........
NASA’s Solar Dynamics Observatory provided the outer image of a coronal mass ejection on May 9, 2014.
NASA’s Solar Dynamics Observatory provided the outer image of a coronal mass ejection on May 9, 2014. The IRIS spacecraft. The IRIS mission views the interface region that lies between the sun’s photosphere and corona in unprecedented detail for researchers to study.
Image Credit: 
NASA, Lockheed Martin Solar & Astrophysics Laboratory
 

NASA's Interface Region Imaging Spectrograph (IRIS) has provided scientists with five new findings into how the sun’s atmosphere, or corona, is heated far hotter than its surface, what causes the sun’s constant outflow of particles called the solar wind, and what mechanisms accelerate particles that power solar flares.
The new information will help researchers better understand how our nearest star transfers energy through its atmosphere and track the dynamic solar activity that can impact technological infrastructure in space and on Earth. Details of the findings appear in the current edition of Science.
 "These findings reveal a region of the sun more complicated than previously thought," said Jeff Newmark, interim director for the Heliophysics Division at NASA Headquarters in Washington. "Combining IRIS data with observations from other Heliophysics missions is enabling breakthroughs in our understanding of the sun and its interactions with the solar system."
The first result identified heat pockets of 200,000 degrees Fahrenheit, lower in the solar atmosphere than ever observed by previous spacecraft. Scientists refer to the pockets as solar heat bombs because of the amount of energy they release in such a short time. Identifying such sources of unexpected heat can offer deeper understanding of the heating mechanisms throughout the solar atmosphere.
For its second finding, IRIS observed numerous, small, low lying loops of solar material in the interface region for the first time. The unprecedented resolution provided by IRIS will enable scientists to better understand how the solar atmosphere is energized.
A surprise to researchers was the third finding of IRIS observations showing structures resembling mini-tornadoes occurring in solar active regions for the first time. These tornadoes move at speeds as fast as 12 miles per second and are scattered throughout the chromosphere, or the layer of the sun in the interface region just above the surface.  These tornados provide a mechanism for transferring energy to power the million-degree temperatures in the corona.
Another finding uncovers evidence of high-speed jets at the root of the solar wind.  The jets are fountains of plasma that shoot out of coronal holes, areas of less dense material in the solar atmosphere and are typically thought to be a source of the solar wind.
The final result highlights the effects of nanoflares throughout the corona. Large solar flares are initiated by a mechanism called magnetic reconnection, whereby magnetic field lines cross and explosively realign. These often send particles out into space at nearly the speed of light. Nanoflares are smaller versions that have long been thought to drive coronal heating. IRIS observations show high energy particles generated by individual nanoflare events impacting the chromosphere for the first time.     
"This research really delivers on the promise of IRIS, which has been looking at a region of the sun with a level of detail that has never been done before," said De Pontieu, IRIS science lead at Lockheed Martin in Palo Alto, California. "The results focus on a lot of things that have been puzzling for a long time and they also offer some complete surprises."
IRIS is a Small Explorer mission managed by NASA’s Goddard Space Flight Center, in Greenbelt, Maryland for the agency’s Science Mission Directorate at NASA Headquarters. NASA's Ames Research Center in Moffett Field, California, provides mission operations and ground data systems. The Norwegian Space Centre is providing regular downlinks of science data. Lockheed Martin designed the IRIS observatory and manages the mission for NASA. The Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, built the telescope. Montana State University in Bozeman designed the spectrograph. Other contributors for this mission include the University of Oslo and Stanford University in Stanford, California.
For more information about IRIS, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

domingo, 7 de septiembre de 2014

NASA : NASA Awards Ozone Mapping and Profiling Suite Modification for the Joint Polar Satellite

Small Asteroid to Safely Pass Close to Earth Sunday

This graphic depicts the passage of asteroid 2014 RC past Earth on September 7, 2014
This graphic depicts the passage of asteroid 2014 RC past Earth on September 7, 2014. At time of closest approach, the space rock will be about one-tenth the distance from Earth to the moon. Times indicated on the graphic are Universal Time.
Image Credit: 
NASA/JPL-Caltech
Orbit of Asteroid 2014 RC
This graphic depicts the orbit of asteroid 2014 RC around the sun. A house-sized asteroid will safely fly past Earth Sunday afternoon, September 7, at a distance equivalent to about one-tenth of the distance between Earth and the moon.
Image Credit: 
NASA/JPL-Caltech
 
A small asteroid, designated 2014 RC, will safely pass very close to Earth on Sunday, Sept. 7, 2014.  At the time of closest approach, based on current calculations to be about 2:18 p.m. EDT (11:18 a.m. PDT / 18:18 UTC), the asteroid will be roughly over New Zealand.  From its reflected brightness, astronomers estimate that the asteroid is about 60 feet (20 meters) in size.
Asteroid 2014 RC was initially discovered on the night of August 31 by the Catalina Sky Survey near Tucson, Arizona, and independently detected the next night by the Pan-STARRS 1 telescope, located on the summit of Haleakalā on Maui, Hawaii.  Both reported their observations to the Minor Planet Center in Cambridge, Massachusetts.  Additional follow-up observations by the Catalina Sky Survey and the University of Hawaii 88-inch (2.2-meter) telescope on Mauna Kea confirmed the orbit of 2014 RC. 
At the time of closest approach, 2014 RC will be approximately one-tenth the distance from the center of Earth to the moon, or about 25,000 miles (40,000 kilometers). The asteroid's apparent magnitude at that time will be about 11.5, rendering it unobservable to the unaided eye.  However, amateur astronomers with small telescopes might glimpse the fast-moving appearance of this near-Earth asteroid.
The asteroid will pass below Earth and the geosynchronous ring of communications and weather satellites orbiting about 22,000 miles (36,000 kilometers) above our planet’s surface.  While this celestial object does not appear to pose any threat to Earth or satellites, its close approach creates a unique opportunity for researchers to observe and learn more about asteroids.
While 2014 RC will not impact Earth, its orbit will bring it back to our planet's neighborhood in the future.  The asteroid's future motion will be closely monitored, but no future threatening Earth encounters have been identified.
For a heliocentric view of the orbit of asteroid 2014 RC with respect to Earth and other planets, visit:
NASA
 
 
NASA Awards Ozone Mapping and Profiling Suite Modification for the Joint Polar Satellite System-2 Mission
NASA has awarded a sole source contract modification to Ball Aerospace and Technology Corp. of Boulder, Colorado, for the Ozone Mapping and Profiling Suite (OMPS) for flight on the Joint Polar Satellite System-2 (JPSS-2) mission.
The JPSS-2 mission is funded by the National Oceanic and Atmospheric Administration (NOAA) to provide global environmental data in low Earth polar orbit in support of NOAA's mission. NASA is the acquisition agent for the flight systems and components of the ground system.
This is a cost-plus-award-fee modification in the amount of $113 million. This action extends the period of performance of the contract from November 2013 through May 2021.
Under this contract, Ball Aerospace and Technology will manufacture, test and deliver the OMPS instrument, support instrument integration on the JPSS-2 spacecraft and provide launch and post-launch support. The OMPS instrument will be similar to the OMPS currently flying on the joint NASA-NOAA Suomi NPP mission and planned for the JPSS-1 mission. JPSS-1 is being planned for launch in 2016 and JPSS-2 is planned for launch in 2021.
OMPS will monitor ozone from space, collect total column and vertical profile ozone data, and continue the current daily global data provided by the Solar Backscatter Ultraviolet radiometer-2 and Total Ozone Mapping Spectrometer. The collection of this data contributes to fulfilling the U.S. treaty obligation to monitor the ozone depletion for the Montreal Protocol to ensure no gaps on ozone coverage.
For information about NASA and agency programs, visit:
Guillermo Gonzalo Sánchez Achutegui

NASA : Commander of Underwater NASA Mission Available for Interviews



Akihiko Hoshide was born in 1968 in Tokyo. He received a bachelor's degree in Mechanical Engineering from Keio University in 1992 and a master of science in Aerospace Engineering from the University of Houston, Cullen College of Engineering in 1997

NASA will venture to the depths of the Atlantic Ocean this month to investigate technologies and procedures for use in near- and long-term space missions. The commander of the seven-day mission, NASA astronaut Randy Bresnik, will be available for media interviews via phone or Skype between 2:15 and 2:45 p.m. EDT Friday, Sept. 12.
To participate in the interviews, contact William Jeffs at william.p.jeffs@nasa.gov by 5 p.m. Wednesday, Sept. 10.
The 19th NASA Extreme Environment Mission Operations (NEEMO) mission begins Monday, Sept. 8. Bresnik will be joined by Canadian Space Agency astronaut Jeremy Hansen, European Space Agency (ESA) astronaut Andreas Mogensen, and Herve Stevenin, ESA’s Head of Extravehicular Activity Training at the European Astronaut Center in Cologne, Germany.
The crew members of NEEMO 19 will test technologies and training techniques for use aboard the International Space Station and future deep space exploration missions. Mission objectives include evaluating technologies to improve crew performance when executing standard space station procedures; testing tools and techniques to conduct spacewalk tasks in varying levels of gravity; and, investigating the capability of just-in-time training to decrease crew training time while increasing crew efficiency for space station and future exploration missions.
The NEEMO crew, along with two professional habitat technicians, will conduct this mission in Florida International University’s undersea research habitat Aquarius Reef Base, located about six miles off the coast of Key Largo, Florida, and 62 feet below the surface of the Atlantic Ocean.
Embry Riddle Aeronautical University will conduct robotics and engineering investigations focused on technologies to support future space exploration missions and underwater operations.
The crew members will share their experiences during NEEMO 19 on Twitter at:
For more information about NEEMO, the crew members, and links to follow the mission on Facebook and Twitter, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

NASA : Space Station Crew Members Tour NASA Facility, Talk Earth Science


NASA astronaut Rick Mastracchio and Japan Aerospace Exploration Agency astronaut Koichi Wakata
NASA astronaut Rick Mastracchio and Japan Aerospace Exploration Agency astronaut Koichi Wakata, Expedition 38 flight engineers, are pictured during Cygnus cargo spacecraft preparation in the Harmony node of the International Space Station.
Image Credit: 
NASA
Astronauts Rick Mastracchio of NASA and Koicha Wakata of the Japan Aerospace Exploration Agency will tour NASA’s Goddard Space Flight Center in Greenbelt, Maryland, at 10 a.m. EDT Wednesday, Sept. 17. Reporters are invited to join the tour.
While at Goddard, Mastracchio and Wakata will view the new Global Precipitation Measurement (GPM) control room and other satellite control centers. The GPM Core Observatory was launched into orbit in February while the two astronauts were aboard the International Space Station. The GPM team will brief Mastracchio, Wakata and the media on the observatory’s collection of data on rain, snowfall and other types of precipitation, data that is now available to the general public.
There also will be a brief question and answer opportunity with the astronauts. The tour and interview opportunity is expected to conclude no later than 11:30 a.m.
The visit is part of several days Mastracchio and Wakata will spend in the Washington area for events and activities to highlight their 188 days in orbit as members of the space station's Expedition 38/39 crews.
To participate in the event at Goddard, U.S. reporters and foreign media with green cards must contact Ed Campion at edward.s.campion@nasa.gov or 301-286-0697 by 5 p.m. Tuesday, Sept. 16. Non-green card holding foreign media must provide passport or visa information no later than 4 p.m. Monday, Sept. 8, to allow time for processing and approval for access to Goddard.
Mastracchio’s official biography is available at:
Wakata's official biography is available at:
For more information on NASA’s GPM Core Observatory, visit:
For more on NASA Earth science launches, research and applications, visit:
For more information about the International Space Station, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

NASA: NASA Administrator Marks Completion of World’s Largest Spacecraft Welding Tool for Space

Sparks Fly as NASA Pushes the Limits of 3-D Printing Technology
Testing Continues With More Complex 3-D Printed Rocket Components
Engineers just completed hot-fire testing with two 3-D printed rocket injectors. Certain features of the rocket components were designed to increase rocket engine performance. The injector mixed liquid oxygen and gaseous hydrogen together, which combusted at temperatures over 6,000 degrees Fahrenheit, producing more than 20,000 pounds of thrust.
Image Credit: 
NASA photo/David Olive
 
NASA has successfully tested the most complex rocket engine parts ever designed by the agency and printed with additive manufacturing, or 3-D printing, on a test stand at NASA's Marshall Space Flight Center in Huntsville, Alabama.
NASA engineers pushed the limits of technology by designing a rocket engine injector --a highly complex part that sends propellant into the engine -- with design features that took advantage of 3-D printing. To make the parts, the design was entered into the 3-D printer's computer. The printer then built each part by layering metal powder and fusing it together with a laser, a process known as selective laser melting.
The additive manufacturing process allowed rocket designers to create an injector with 40 individual spray elements, all printed as a single component rather than manufactured individually. The part was similar in size to injectors that power small rocket engines and similar in design to injectors for large engines, such as the RS-25 engine that will power NASA's Space Launch System (SLS) rocket, the heavy-lift, exploration class rocket under development to take humans beyond Earth orbit and to Mars.
Youtube Override: 
3-D Printed Rocket Injector Roars to Life: The most complex 3-D printed rocket injector ever built by NASA roars to life on the test stand at NASA’s Marshall Space Flight Center in Huntsville, Alabama.
"We wanted to go a step beyond just testing an injector and demonstrate how 3-D printing could revolutionize rocket designs for increased system performance," said Chris Singer, director of Marshall's Engineering Directorate. "The parts performed exceptionally well during the tests."
Using traditional manufacturing methods, 163 individual parts would be made and then assembled. But with 3-D printing technology, only two parts were required, saving time and money and allowing engineers to build parts that enhance rocket engine performance and are less prone to failure.
Two rocket injectors were tested for five seconds each, producing 20,000 pounds of thrust. Designers created complex geometric flow patterns that allowed oxygen and hydrogen to swirl together before combusting at 1,400 pounds per square inch and temperatures up to 6,000 degrees Fahrenheit. NASA engineers used this opportunity to work with two separate companies -- Solid Concepts in Valencia, California, and Directed Manufacturing in Austin, Texas. Each company printed one injector.
"One of our goals is to collaborate with a variety of companies and establish standards for this new manufacturing process," explained Marshall propulsion engineer Jason Turpin. "We are working with industry to learn how to take advantage of additive manufacturing in every stage of space hardware construction from design to operations in space. We are applying everything we learn about making rocket engine components to the Space Launch System and other space hardware."
Additive manufacturing not only helped engineers build and test a rocket injector with a unique design, but it also enabled them to test faster and smarter. Using Marshall's in-house capability to design and produce small 3-D printed parts quickly, the propulsion and materials laboratories can work together to apply quick modifications to the test stand or the rocket component.
"Having an in-house additive manufacturing capability allows us to look at test data, modify parts or the test stand based on the data, implement changes quickly and get back to testing," said Nicholas Case, a propulsion engineer leading the testing. "This speeds up the whole design, development and testing process and allows us to try innovative designs with less risk and cost to projects."
Marshall engineers have tested increasingly complex injectors, rocket nozzles and other components with the goal of reducing the manufacturing complexity and the time and cost of building and assembling future engines. Additive manufacturing is a key technology for enhancing rocket designs and enabling missions into deep space.
For more information about SLS, visit:
 
NASA Administrator Marks Completion of World’s Largest Spacecraft Welding Tool for Space Launch System
NASA’s new Vertical Assembly Center (VAC), a 170-foot-high marvel of machinery that will be used to assemble elements of the agency's Space Launch System (SLS), now is complete and ready to weld parts for the rocket that will send humans to an asteroid and Mars.
Media are invited to join NASA Administrator Charles Bolden at the ribbon cutting for the enormous new tool at 11 a.m. EDT Friday, Sept. 12, at the agency's Michoud Assembly Facility in New Orleans where the core stage is being built. The event will air live on NASA Television and the agency's website.
Bolden and other officials from NASA and Boeing, the prime contractor for the SLS core stage and avionics, will be available for a brief media opportunity following the ceremony.
The Vertical Assembly Center will be used to join domes, rings and barrels segments to complete the SLS fuel tanks. The tool also will be used to perform evaluations of the completed welds. Towering more than 200 feet tall, with a diameter of 27.6 feet, the core stage will store cryogenic liquid hydrogen and liquid oxygen to feed the vehicle’s RS-25 engines.
Bolden also will visit NASA's Stennis Space Center near Bay St. Louis, Mississippi, following the Michoud events, and will be available to talk to media at 2:15 p.m. CDT at the base of the historic B-2 Test Stand, along with other NASA representatives. The B-2 Test Stand was used to test the S-1C stage on the Saturn V moon rocket and the Main Propulsion Test Article, the configuration of three main engines flown on space shuttle missions. The stand will next be used to test the core stage of SLS and its configuration of four RS-25 engines.
Media who wish to attend both the Michoud and Stennis events must contact Chip Howat at carl.j.howat@nasa.gov or 504-214-6745 no later than 4 p.m. CDT Thursday, Sept. 11. Media must arrive at 13800 Old Gentilly Road, Bldg. 101 visitor's lobby, by 9:15 a.m. Friday, Sept. 12, for access to the facility. Official media credentials with photo identification are required for access.
Those interested only in attending the Stennis event must contact Paul Foerman at paul.foerman-1@nasa.gov or 228-688-1880 no later than 4 p.m. CDT Thursday, Sept. 11.
For more information about SLS, visit:
For NASA TV streaming video, schedules and downlink information, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

NASA: NASA Television to Broadcast Sept. 10 Return of Space Station Crew


Exp. 40 crew returns
NASA astronaut Steve Swanson, Expedition 40 commander, along with cosmonauts Alexander Skvortsov and Oleg Artemyev, both flight engineers with the Russian Federal Space Agency, return to Earth Sept. 10 after six month aboard the International Space Station.
 
Three crew members aboard the International Space Station are scheduled to end almost six months on the orbiting laboratory on Sept. 10 and NASA Television will provide complete coverage.
Expedition 40 Commander Steve Swanson of NASA and Flight Engineers Alexander Skvortsov and Oleg Artemyev of the Russian Federal Space Agency (Roscosmos) will undock their Soyuz spacecraft from the station at 7:02 p.m. EDT Sept. 10, for a landing in Kazakhstan at 10:25 p.m. (8:25 a.m. Sept. 11, Kazakh time). Their return will end 169 days in space since launching from Kazakhstan March 26 for a mission that covered almost 72 million miles in orbit.
At the time of undocking, Expedition 41 formally will begin aboard the station under the command of Max Suraev of Roscosmos. Suraev and his crewmates, Reid Wiseman of NASA and Alexander Gerst of the European Space Agency, will operate the station as a three-person crew for two weeks until the arrival of three new crew members. NASA astronaut Barry Wilmore and Russian cosmonauts Alexander Samokutyaev and Elena Serova are scheduled to launch from Baikonur, Kazakhstan, Sept. 25, (U.S. time), on a six-hour flight to the space station.
NASA TV coverage will begin Tuesday, Sept. 9, with a change of command ceremony when Swanson will turn over control of station operations to Suraev, and will continue Sept. 10 and 11 with Expedition 40 landing and post-landing activities.
NASA coverage, all in EDT, includes:
Tuesday, Sept. 9:
-- 5:15 p.m. - Expedition 40/41 change of command ceremony
Wednesday, Sept. 10:
-- 3:15 p.m. - Farewells and hatch closure coverage (hatch closure at 3:35 p.m.)
-- 6:45 p.m. - Undocking (undocking at 7:02 p.m.)
-- 9:15 p.m. - Deorbit burn and landing coverage (deorbit burn at 9:31 p.m. and landing at 10:25 p.m.)
Thursday, Sept. 11:
-- 12 a.m. - Video File of hatch closure, undocking and landing activities
-- 12 p.m. - Video File of landing and post-landing activities and interview with Steve Swanson in Kazakhstan
For the NASA TV schedule and coordinate information, visit:
For b-roll and other media resources, visit:
For more information about the International Space Station, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

NASA : NASA Launches Satellite to Study How Sun's Atmosphere Is Energized




NASA Launches Satellite to Study How Sun's Atmosphere Is Energized

WASHINGTON -- NASA's Interface Region Imaging Spectrograph (IRIS) spacecraft launched Thursday at 7:27 p.m. PDT (10:27 p.m. EDT) from Vandenberg Air Force Base, Calif. The mission to study the solar atmosphere was placed in orbit by an Orbital Sciences Corporation Pegasus XL rocket.
"We are thrilled to add IRIS to the suite of NASA missions studying the sun," said John Grunsfeld, NASA's associate administrator for science in Washington. "IRIS will help scientists understand the mysterious and energetic interface between the surface and corona of the sun."
IRIS is a NASA Explorer Mission to observe how solar material moves, gathers energy and heats up as it travels through a little-understood region in the sun's lower atmosphere. This interface region between the sun's photosphere and corona powers its dynamic million-degree atmosphere and drives the solar wind. The interface region also is where most of the sun's ultraviolet emission is generated. These emissions impact the near-Earth space environment and Earth's climate.
The Pegasus XL carrying IRIS was deployed from an Orbital L-1011 carrier aircraft over the Pacific Ocean at an altitude of 39,000 feet, off the central coast of California about 100 miles northwest of Vandenberg. The rocket placed IRIS into a sun-synchronous polar orbit that will allow it to make almost continuous solar observations during its two-year mission.
The L-1011 took off from Vandenberg at 6:30 p.m. PDT and flew to the drop point over the Pacific Ocean, where the aircraft released the Pegasus XL from beneath its belly. The first stage ignited five seconds later to carry IRIS into space. IRIS successfully separated from the third stage of the Pegasus rocket at 7:40 p.m. At 8:05 p.m., the IRIS team confirmed the spacecraft had successfully deployed its solar arrays, has power and has acquired the sun, indications that all systems are operating as expected.
"Congratulations to the entire team on the successful development and deployment of the IRIS mission," said IRIS project manager Gary Kushner of the Lockheed Martin Solar and Atmospheric Laboratory in Palo Alto, Calif. "Now that IRIS is in orbit, we can begin our 30-day engineering checkout followed by a 30-day science checkout and calibration period."
IRIS is expected to start science observations upon completion of its 60-day commissioning phase. During this phase the team will check image quality and perform calibrations and other tests to ensure a successful mission.
NASA's Explorer Program at Goddard Space Flight Center in Greenbelt, Md., provides overall management of the IRIS mission. The principal investigator institution is Lockheed Martin Space Systems Advanced Technology Center. NASA's Ames Research Center will perform ground commanding and flight operations and receive science data and spacecraft telemetry.
The Smithsonian Astrophysical Observatory designed the IRIS telescope. The Norwegian Space Centre and NASA's Near Earth Network provide the ground stations using antennas at Svalbard, Norway; Fairbanks, Alaska; McMurdo, Antarctica; and Wallops Island, Va. NASA's Launch Services Program at the agency's Kennedy Space Center in Florida is responsible for the launch service procurement, including managing the launch and countdown. Orbital Sciences Corporation provided the L-1011 aircraft and Pegasus XL launch system.
For more information about the IRIS mission, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui

NASA : NASA to Investigate Climate Impacts of Arctic Sea Ice Loss


Youtube Override: 
Image Credit: 
NASA's Goddard Space Flight Center/J. Beck
 
A new NASA field campaign will begin flights over the Arctic this summer to study the effect of sea ice retreat on Arctic climate. The Arctic Radiation IceBridge Sea and Ice Experiment (ARISE) will conduct research flights Aug. 28 through Oct. 1, covering the peak of summer sea ice melt.
ARISE is NASA's first Arctic airborne campaign designed to take simultaneous measurements of ice, clouds and the levels of incoming and outgoing radiation, the balance of which determines the degree of climate warming. The campaign team will fly aboard NASA’s C-130 aircraft from Thule Air Base in northern Greenland the first week and from Eielson Air Force Base near Fairbanks, Alaska, through the remainder of the campaign.
In recent years the Arctic has experienced increased summer sea ice loss. Scientists expect the exposure of more open water to sunlight could enhance warming in the region and cause the release of more moisture to the atmosphere. Additional moisture could affect cloud formation and the exchange of heat from Earth’s surface to space. Researchers are grappling with how these changes in the Arctic affect global climate.
NASA’s C-130
NASA’s C-130 aircraft will carry scientists over the Arctic starting this month from northern Greenland and Fairbanks, Alaska.
Image Credit: 
NASA
 
"A wild card in what's happening in the Arctic is clouds and how changes in clouds, due to changing sea-ice conditions, enhance or offset warming," said Bill Smith, ARISE principal investigator at NASA's Langley Research Center in Hampton, Virginia.
ARISE was planned over the last year to take advantage of NASA’s existing capabilities for gathering data about ongoing changes in the Arctic. Satellites provided some information about clouds and the energy balance in the Arctic, but the multiple instruments flown during ARISE should provide further insight.
"The clouds and surface conditions over the Arctic as we observe them from satellites are very complex," Smith said. "We need more information to understand how to better interpret the satellite measurements, and an aircraft can help with that."
The array of instruments on ARISE should help scientists better observe how sea ice loss is affecting Arctic cloud formation and therefore the balance of incoming and outgoing radiation. Low-level clouds typically reflect more sunlight and offset warming, while higher clouds are typically less reflective and act to trap more heat in the atmosphere.
“It’s a complex business, but it depends on a lot of things we can, in fact, measure,” said Hal Maring, program manager for radiation sciences in the Earth Science Division at NASA Headquarters in Washington.
ARISE researchers will fly survey missions that target different cloud types and surface conditions, such as open water, land ice and sea ice. The missions will be timed to fly under the orbit paths of key satellite instruments, such as the Clouds and the Earth’s Radiant Energy Systems (CERES) instruments on multiple NASA satellites. Each morning, mission planners will look at satellite timings and weather forecasts to design flight plans that meet the most objectives of the campaign.
The NASA C-130, based at the Wallops Flight Facility in Virginia, will carry instruments that measure solar (incoming) and infrared (outgoing) radiation, ice surface elevation and cloud properties such as cloud particle size. This will be the first time that many of these instruments, including the mission's laser altimeter, have flown together.
The ARISE campaign is a joint effort of the Radiation Sciences, Cryospheric Sciences and Airborne Sciences programs of the Earth Science Division in NASA's Science Mission Directorate in Washington.
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.
To learn more about NASA's Earth science activities in 2014, visit:
NASA
Guillermo Gonzalo Sánchez Achutegui