Thursday, 1 November 2012

GIS NEWS : Locating Earthquake Victims, New GIS Tools, now in the Cloud


Locating Earthquake Victims, New GIS Tools, now in the Cloud
New tools to locate victims of earthquakes, and global information systems, to be featured at Global Humanitarian conference in Seattle. The world's first reliable earthquake victims locator, new global information systems (GIS) platforms, latest cloud based tools to be featured at IEEE Global Humanitarian Technology Conference October 21 -24, 2012 in Seattle, Washington.
If there is a major earthquake over five points on the Richter scale this app automatically and instantaneously sends an email out to say you've been in an earthquake, says Australian business leader Adam Wells, developer of Earthquake Buddy to be featured at the conference. And if you're not heard from within, say thirty minutes, that they can come and find you.
Earthquake Buddy is an app downloaded from the iPhone App Store and has no monthly fees. Its the worlds first, nothing else like it, says Wells. During an earthquake anywhere in the world people preselected will receive a notice from the cloud. From international seismic feeds there will be a tagged map of where you were when the earthquake happened, says Wells.
Also featured at the conference and using new cloud enabled technology is a GIS platform that enables relief agencies and non-government organizations (NGOs) to see the real world around them in fine geographic detail. We've found ways to abstract nearly everything that could be seen in the real world, says David Gadsden, who is leading the nonprofit organization program for the Environmental Systems Research Institute (Esri). This is really a paradigm shift for Esri technology, and GIS technology globally. Prior to the roll out of the cloud it really took some investment in infrastructure to implement GIS across an organization.
Both Wells and Gadsden made their comments on the Science News Radio Network program, the Promise of Tomorrow with Colonel Mason which is covering the conference. The program originates in Dallas, Texas, and is now archived and Webcast for its world audience. Wells spoke by phone from a site on the bay in Sidney, Australia, and Gadsden from his office in Olympia, WA.
Solutions to cure the worlds greatest human problems will get a thorough study at the conference, produced by the Institute of Electrical and Electronics Engineers (IEEE). More information on conference technical sessions, website registration, hotel reservations and exhibiting is available at the website www.ieeeghtc.org

Testing Mars and Moon soil for sheltering astronauts from radiation


Testing Mars and Moon soil for sheltering astronauts from radiation
Humans venturing beyond Earth orbit deeper into space face increased exposure to cosmic radiation, so ESA have teamed with Germany’s GSI particle accelerator to test potential shielding for astronauts, including Moon and Mars soil.
ESA’s two-year project is assessing the most promising materials for shielding future astronauts going to the Moon, the asteroids or Mars.“We are working with the only facility in Europe capable of simulating the high-energy heavy atomic nuclei found in galactic cosmic radiation – the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt, Germany,” explained Alessandra Menicucci, overseeing the project.
“We assessed materials including aluminium, water, polyethylene plastic, multilayer structures and simulated Moon and Mars material – the latter on the basis these will be accessible to planetary expeditions.
Lunar soil simulant
“We have also confirmed a new type of hydrogen storage material holds particular promise.”Space is awash with charged particles, meaning that astronauts are officially classed as radiation workers. The International Space Station orbits within Earth’s magnetic field, safeguarding its occupants from the bulk of space radiation. To venture further out, dedicated shielding will be required.
Space radiation comes from the Sun – in the form of intense but short-lived ‘solar particle events’ – as well as galactic cosmic radiation originating beyond our Solar System: atomic nuclei produced by dying stars, their passage sped by magnetic fields as they cross the galaxy.
GSI
“Solar particle events are made up of protons that can be shielded quite simply,” added Alessandra.“The real challenge for deep-space missions is galactic cosmic radiation, which cannot be shielded completely because of its very high energy, although the exposure level decreases with increased solar activity.
Most are small protons or helium nuclei, but about 1% are larger, the size of an iron atom or more – known as ‘high-ionising high energy particles’ or HZE for short. Radiation shielding can be counter-intuitive because denser and thicker does not always mean better.
Astronauts
HZEs striking metal shields can produce showers of secondary particles that might be even more harmful. And as shield thickness increases, overall the energy loss of ionising radiation rises to a peak then declines rapidly.“In general, the lighter a material’s atomic nuclei the better the protection,” notes Alessandra.
Water and polyethylene performed better than aluminium for instance, and new hydrogen-rich materials developed by UK Company Cella Energy tested better still. Cella Energy originally developed its patent-pending materials for storing hydrogen fuel but is currently investigating their radiation resistance.

On Internet rules, India now more willing to say ICANN


On Internet rules, India now more willing to say ICANN
The Hindu India has reinvented its position on Internet governance, hoping to become a new voice of reason in what has so far been a deeply polarised global debate. Distances itself from any model propagating governments taking “charge” or “balkanising” the web
India has reinvented its position on Internet governance, hoping to become a new voice of reason in what has so far been a deeply polarised global debate. The change, effected after detailed inter-ministerial as well as multi-stakeholder consultation, is intended to distance India from any model propagating governments taking “charge” or “balkanising” the Internet. It was unveiled at the recent Budapest Cyber Space Conference.
According to Minister of State for Telecom Sachin Pilot, who led the Indian delegation to Budapest, instead of opposing the U.S.-based Internet Corporation for Assigned Names and Numbers (ICANN) and its operations through an earlier proposal called the U.N. Committee on Internet-Related Policies (UN-CIRP), India will pursue enhanced cooperation through wider dialogue.
“In our meetings with Fadi Chehade, the new CEO of ICANN, I have sought far stronger representation of the developing world on the four ICANN Advisory committees”, Mr. Pilot told The Hindu.ICANN’s committees include the “At Large Advisory Committee (ALAC), Governmental Advisory Committee (GAC), Root Server System Advisory Committee (RSSAC) and the Security and Stability Advisory Committee (SSAC).
Countries such as Russia, China, Uzbekistan and Tajikistan have been advocating governance models that seek to place the Internet under U.N. control while the U.S. and western states have been reluctant to move away from the status quo position of ICANN-led Internet governance. India had positioned its UN-CIRP proposal as something that would lie in between these two extremes. But while the international debate continues, it is keen to step up its engagement with ICANN which remains, for the moment, the only game in town.
“The extreme views being floated by some countries on Internet governance could lead to the balkanisation of Internet and we are against any such move, including control of Internet by government or inter-governmental bodies. We seek enhanced dialogue and continuation of a working group to find ways to resolve the sharp differences that currently exist,” Mr. Pilot said.
Mr. Pilot’s position is consistent with that of Telecom Minister Kapil Sibal, who maintained at two recent meetings on Internet governance in India in September 2012, that India was firmly against government control of the Internet while seeking consensus among multi-stakeholders to develop an appropriate model for the effective management of the Internet.
India had attracted criticism from the U.S. and from corporate stakeholders who want no dilution of the current ICANN-run system after it presented its UN-CIRP model for Internet governance last October at the 66th General Assembly of the United Nations in New York.
While the UN-CIRP essentially sought a shift from the existing ICANN-run model that is perceived to be too close to the U.S. government, many domestic stakeholders were critical of the lack of consultation in the run-up to the October 2011 statement. Signs of a rethink in the government were evident when senior officials in the ministries concerned refused to entertain questions on the genesis of the UN-CIRP proposal put to them by The Hindu over the past few months.
In the run-up to the Budapest meet, a UPA task-force held closed-door consultations involving the Ministry of External Affairs, Ministry of Telecom and IT, industry bodies and others. Latha Reddy, the Deputy National Security Adviser, coordinated this effort. On the issue of India’s earlier UN-CIRP model, Mr. Pilot also confirmed, “We are moving ahead with new proposals. While the existing system certainly needs to be changed, India’s position will include multi-stakeholder involvement and not inter-governmental bodies that may have been proposed in the past.”
The Indian government’s changed stance on Internet governance, though subtle, is expected to generate further attention at the upcoming Internet Governance Forum in Baku, Azerbaijan next month, where thousands of delegates representing governments, business, civil society, academia and media from across the world will collect to discuss the issue.

X-raying stellar winds in a high-speed collision


X-raying stellar winds in a high-speed collision
Two massive stars racing in orbit around each other have had their colliding stellar winds X-rayed for the first time, thanks to the combined efforts of ESA’s XMM-Newton and NASA’s Swift space telescopes. Stellar winds, pushed away from a massive star’s surface by its intense light, can have a profound influence on their environment.
In some locations, they may trigger the collapse of surrounding clouds of gas and dust to form new stars. In others, they may blast the clouds away before they have the chance to get started. Now, XMM-Newton and Swift have found a ‘Rosetta stone’ for such winds in a binary system known as Cyg OB2 #9, located in the Cygnus star-forming region, where the winds from two massive stars orbiting around each other collide at high speeds.
Colliding winds at Cyg OB2 #9
Cyg OB2 #9 remained a puzzle for many years. Its peculiar radio emission could only be explained if the object was not a single star but two, a hypothesis that was confirmed in 2008.At the time of the discovery, however, there was no direct evidence for the winds from the two stars colliding, even though the X-ray signature of such a phenomenon was expected.
This signature could only be found by tracking the stars as they neared the closest point on their 2.4-year orbit around each other, an opportunity that presented itself between June and July 2011.As the space telescopes looked on, the fierce stellar winds slammed together at speeds of several million kilometres per hour, generating hot plasma at a million degrees which then shone brightly in X-rays.
Colliding winds at WR 22
The telescopes recorded a four-fold increase in energy compared with the normal X-ray emission seen when the stars were further apart on their elliptical orbit.“This is the first time that we have found clear evidence for colliding winds in this system,” says Yael Nazé of the Université de Liège, Belgium, and lead author of the paper describing the results reported in Astronomy & Astrophysics.
“We only have a few other examples of winds in binary systems crashing together, but this one example can really be considered an archetype for this phenomenon.”Unlike the handful of other colliding wind systems, the style of the collision in Cyg OB2 #9 remains the same throughout the stars’ orbit, despite the increase in intensity as the two winds meet.
“In other examples the collision is turbulent; the winds of one star might crash onto the other when they are at their closest, causing a sudden drop in X-ray emission,” says Dr Nazé.“But in the Cyg OB2 #9 systems there is no such observation, so we can consider it the first ‘simple’ example that has been discovered – that really is the key to developing better models to help understand the characteristics of these powerful stellar winds. ”
“This particular binary system represents an important stepping stone in our understanding of stellar wind collisions and their associated emissions, and could only be achieved by tracking the two stars orbiting around each other with X-ray telescopes,” adds ESA’s XMM-Newton project scientist Norbert Schartel.

Lost asteroid rediscovered with a little help from ESA


Lost asteroid rediscovered with a little help from ESA
A potentially hazardous asteroid once found but then lost has been rediscovered and its orbit confirmed by a determined amateur astronomer working with ESA’s space hazards programme. The half-kilometre object will not threaten Earth anytime soon.
Amateur astronomer Erwin Schwab, from Germany, conducted his asteroid hunt in September during a regular observation slot at ESA’s Optical Ground Station in Tenerife, Spain, sponsored by the Agency’s Space Situational Awareness programme.
He was determined to rediscover the object, known by its catalogue name as 2008SE85.Potentially Hazardous Asteroid 2008SE85 was discovered in September 2008 by the Catalina Sky Survey, and observed by a few observatories to October 2008.
Asteroid considered lost
Since then, however, nobody had observed the object and predictions for its current position had become so inaccurate that the object was considered to be ‘lost’.
Orbit of 2008SE85
Erwin planned his observing sequence to look for the object within the area of uncertainty of its predicted position. After only a few hours, he found it about 2° – four times the apparent size of the Moon – away from its predicted position.“I found the object on the evening of Saturday, 15 September, while checking the images on my computer,” says Erwin.
“I then saw it again at 01:30 on Sunday morning – and that was my birthday! It was one of the nicest birthday presents.” These new observations of the roughly 500 m-diameter asteroid will allow a much more accurate determination of its orbit and help confirm that it will not be a threat to Earth anytime soon.
Potentially Hazardous Asteroids approach Earth closer than about 7 million km; about 1300 is known. When a new asteroid is discovered, follow-up observations must be done within a few hours and then days to ensure it is not subsequently lost.
USA-based Minor Planet Center acknowledges the find Asteroid position measurements are collected from observers worldwide by the US-based Minor Planet Center, which acknowledged the rediscovery of 2008SE85 by releasing a Minor Planet Electronic Circular announcing the new observations.
1m telescope at ESA's Optical Ground Station
“These observations were part of the strong collaboration that we have with a number of experienced backyard observers,” says Detlef Koschny, Head of the Near-Earth Object segment of ESA’s Space Situational Awareness programme.
"It’s not the first time our collaboration with amateurs has scored such a success. Members of the Teide Observatory Tenerife Asteroid Survey started by Matthias Busch from Heppenheim, Germany, discovered two new near-Earth objects during the last year while working with our observing programme."

Wednesday, 31 October 2012

New data stealing Trojan rocks Android


New data stealing Trojan rocks Android
The new threat to Android devices makes its way to Google Play store, disguised as a credible application. Android’s application store, Google Play's security has once again been rattled with the discovery of a new malware application which is said to be stealing sensitive information from the users' Android smartphones.
Identified as 'Trojan!FakeLookout.A' by TrustGo Security Labs, this malicious app steals user SMS/MMS messages and video files, as well as all the files on the user's SD card and transmits them to a remote FTP server of the malware maker. The virus has the potential to cause significant privacy breaches and exposes all the sensitive personal and business data on users' devices to its creators in no time.
TrustGo, one of the popular global security software solutions providers have identified this new threat in an application on the Google Play Android marketplace. The malicious Application was hidden within an app named, "Updates" by developer Good Byte Labs on the Google Play store and has been expected to have infected a large number Android smartphones world over.
Although till now no user has reported of being affected by the malware but it is quite possible that the users who have been infected are not aware of it as of now.
Normally, if this Trojan package is executed, users would experience heavier data usage as the malicious application keeps uploading data to servers.
For the removal of this malware, users can use antivirus applications such as Lookout by TrustGo labs to remove this Trojan form their devices, if the antivirus program fails to remove then a hard reset of the device is advised for the removal of the Trojan, but remember to take a backup of the data before resetting the device to avoid losing important data.
For further information visit: http://www.themobileindian.com/news/8945&p=1

Tuesday, 30 October 2012

Astronomers Uncover a Surprising Trend In Galaxy Evolution

Astronomers Uncover a Surprising Trend In Galaxy Evolution
  WASHINGTON -- A comprehensive study of hundreds of galaxies observed by the Keck telescopes in Hawaii and NASA's Hubble Space Telescope has revealed an unexpected pattern of change that extends back 8 billion years, or more than half the age of the universe.
"Astronomers thought disk galaxies in the nearby universe had settled into their present form by about 8 billion years ago, with little additional development since," said Susan Kassin, an astronomer at NASA's Goddard Space Flight Center in Greenbelt, Md., and the study's lead researcher. "The trend we've observed instead shows the opposite, that galaxies were steadily changing over this time period."
Today, star-forming galaxies take the form of orderly disk-shaped systems, such as the Andromeda Galaxy or the Milky Way, where rotation dominates over other internal motions. The most distant blue galaxies in the study tend to be very different, exhibiting disorganized motions in multiple directions. There is a steady shift toward greater organization to the present time as the disorganized motions dissipate and rotation speeds increase. These galaxies are gradually settling into well-behaved disks.
Blue galaxies -- their color indicates stars are forming within them -- show less disorganized motions and ever-faster rotation speeds the closer they are observed to the present. This trend holds true for galaxies of all masses, but the most massive systems always show the highest level of organization.
Researchers say the distant blue galaxies they studied are gradually transforming into rotating disk galaxies like our own Milky Way. "Previous studies removed galaxies that did not look like the well-ordered rotating disks now common in the universe today," said co-author Benjamin Weiner, an astronomer at the University of Arizona in Tucson. "By neglecting them, these studies examined only those rare galaxies in the distant universe that are well-behaved and concluded that galaxies didn't change."
Rather than limit their sample to certain galaxy types, the researchers instead looked at all galaxies with emission lines bright enough to be used for determining internal motions. Emission lines are the discrete wavelengths of radiation characteristically emitted by the gas within a galaxy. They are revealed when a galaxy's light is separated into its component colors. These emission lines also carry information about the galaxy's internal motions and distance.
The team studied a sample of 544 blue galaxies from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) Redshift Survey, a project that employs Hubble and the twin 10-meter telescopes at the W. M. Keck Observatory in Hawaii. Located between 2 billion and 8 billion light-years away, the galaxies have stellar masses ranging from about 0.3 percent to 100 percent of the mass of our home galaxy.
A paper describing these findings will be published Oct. 20 in The Astrophysical Journal. The Milky Way galaxy must have gone through the same rough-and-tumble evolution as the galaxies in the DEEP2 sample, and gradually settled into its present state as the sun and solar system were being formed.
In the past 8 billion years, the number of mergers between galaxies large and small has decreased sharply. So has the overall rate of star formation and disruptions of supernova explosions associated with star formation. Scientists speculate these factors may play a role in creating the evolutionary trend they observe. Now that astronomers see this pattern, they can adjust computer simulations of galaxy evolution until these models are able to replicate the observed trend. This will guide scientists to the physical processes most responsible for it.
The DEEP2 survey is led by Lick Observatory at the University of California at Santa Cruz in collaboration with the University of California at Berkeley, the University of Hawaii at Manoa, Johns Hopkins University in Baltimore, Md., the University of Chicago and the California Institute of Technology in Pasadena. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Md., conducts Hubble science operations. STScI is operated by the Association of Universities for Research in Astronomy, Inc. in Washington.
Article No.2
NASA must reinvest in nanotechnology research, according to new Rice University paper
The United States may lose its leadership role in space to other countries unless it makes research and development funding and processes - especially in nanotechnology - a renewed and urgent priority, according to a new paper from Rice University's Baker Institute for Public Policy.
The paper, "NASA's Relationship with Nanotechnology: Past, Present and Future Challenges," investigates how NASA has both guided and defunded cutting-edge nanotechnology development since 1996 at its own research facilities and in its collaborations with university scientists and laboratories.
The research was conducted by a team at Rice that included Baker Institute science and technology policy fellow Kirstin Matthews, current Rice graduate student Kenneth Evans and former graduate students Padraig Moloney and Brent Carey. The paper sheds light on a broad field that holds tremendous potential for improving space flight by reducing the weight of spacecraft and developing smaller and more accurate sensors.
This area of research, however, saw a dramatic cutback from 2004 to 2007, when NASA reduced annual nanotechnology R and D expenditures from $47 million to $20 million. NASA is the only U.S. federal agency to scale back investment in this area, the authors found, and it's part of an overall funding trend at NASA.From 2003 to 2010, while the total federal science research budget remained steady between $60 billion and $65 billion (in constant 2012 dollars), NASA's research appropriations decreased more than 75 percent, from $6.62 billion to $1.55 billion.
The authors argue that the agency should restructure, refocus and strengthen its R and D programs."The United States currently lacks a national space policy that ensures the continuity of research and programs that build on existing capabilities to explore space, and that has defined steps for human and robotic exploration of low-Earth orbit, the moon and Mars," Matthews said.
"With Congress and the president wrestling over the budget each year, it is vital that NASA present a clear plan for science and technology R and D that is linked to all aspects of the agency. This includes connecting R and D, with nanotechnology as a lead area, to applications related to the agency's missions."
The authors said that to effectively engage in new technology R and D, NASA should strengthen its research capacity and expertise by encouraging high-risk, high-reward projects to help support and shape the future of U.S. space exploration
"Failure to make these changes, especially in a political climate of flat or reduced funding, poses substantial risk that the United States will lose its leadership role in space to other countries - most notably China, Germany, France, Japan and Israel - that make more effective use of their R and D investments," Matthews said.
Article No.3
ISS Orbit to be adjusted for Next Spacecraft
Specialists of the Moscow Region-based Mission Control Center will on Wednesday carry out a maneuver to readjust the orbit of the International Space Station, a spokesman for the center said.
The readjustment will be carried out with the use of thrusters of the Russian Zvezda service module."The operation is expected to begin at 19:24 Moscow time [15:24 GMT]. The engines of the Zvezda module will operate for 19 seconds," the spokesman said adding that the station's average orbit altitude will be raised by one kilometer to 436 km (270.9 miles).
The reboost is intended to ensure the best conditions for the docking of the Soyuz TMA-06M manned spacecraft with the orbital outpost, slated for October 25.
The Soyuz TMA-06M will bring to the station a new crew, which comprises Russian cosmonauts Oleg Novitsky and Yevgeny Tarelkin, and NASA astronaut Kevin Ford.
Adjustments to the station's orbit are carried out regularly to compensate for the Earth's gravity and to facilitate the successful docking and undocking of spacecraft.