Friday, June 1, 2012

U.S. military trainers trickle back into Pakistan

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National Spelling Bee down to 9 finalists

Lena Greenberg, 14, of Philadelphia, waits to compete in the National Spelling Bee in Oxon Hill, Md., Wednesday, May 30, 2012. She spelled her word correctly. (AP Photo/Jacquelyn Martin)

Lena Greenberg, 14, of Philadelphia, waits to compete in the National Spelling Bee in Oxon Hill, Md., Wednesday, May 30, 2012. She spelled her word correctly. (AP Photo/Jacquelyn Martin)

Emma Steimle of Lawrence, Kansas spells her word during the third round of the National Spelling Bee, Wednesday, May 30, 2012, in Oxon Hill, Md. (AP Photo/Evan Vucci)

Lori Anne Madison, 6, of Woodbridge, Va., the youngest speller ever to compete in the National Spelling Bee, reacts after misspelling her word, ingluvies, in the third round of the bee in Oxon Hill, Md., on Wednesday, May 30, 2012. She will not be moving on to the semifinals. (AP Photo/Jacquelyn Martin)

(AP) ? Nine spellers are bringing their brains and competitive fire to the final round of the National Spelling Bee.

The field was cut from 50 in three brutally difficult semifinal rounds that elicited tears and squeals of delight. The final round starts at 8 p.m. Thursday.

Lena Greenberg, an excitable 14-year-old from Philadelphia, became the last speller to make the finals when she spelled "cholecystitis" ? an inflammation of the gallbladder. She says she didn't know the word but was able to piece it together.

The field also includes Gifton Wright of Spanish Town, Jamaica, who could become the second Jamaican winner in Scripps National Spelling Bee history.

Nicholas Rushlow of Pickerington, Ohio, who's been in the bee every year since 2008, made the finals for the first time. Last summer, he spelled every word in the dictionary.

Associated Press

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PowerA unveils MOGA Bluetooth controller for Android devices, we go hands-on

PowerA unveils Moga Bluetooth controller for Android devices, we go hands-on

PowerA's best known as a company that crafts controllers and accessories for console gaming systems, but at E3 this year the firm is announcing its first foray into the mobile space: a Bluetooth controller for Android. Called the MOGA, its got dual analog sticks and shoulder buttons, along with a fold-out, spring-loaded center portion that holds phones of all sizes in place while you get your game on -- not unlike Gametel's controller we saw at CES. The front of the device is glossy black plastic, while the rear is swathed in rubber, with ribbed portions on the grips to keep it firmly in hand.

A companion app, available for free through the Google Play store, is also a part of the Moga experience. Called the MOGA Pivot app, it scans your phone for games compatible with the controller, lists them, and lets you launch them direct from the app. Not only that, it'll periodically update the games list as new games are acquired and it'll download patch kits automatically for existing games as they become compatible with the controller. Additionally, it's got a store (powered by Google Play) that'll let users download new compatible games, and titles in the Play Store will have a badge to let folks know which games work with Moga. Currently, the company has 14 games on board -- including Duke Nukem 3D, Virtua Tennis Challenge and Sonic CD -- and are in talks with some other big publishers, so more titles will be supported in the coming weeks and months. We got a sneak peek at the MOGA ahead of E3 and talked with the folks from PowerA about their newest bit of kit, so join us after the break for our impressions.

Continue reading PowerA unveils MOGA Bluetooth controller for Android devices, we go hands-on

PowerA unveils MOGA Bluetooth controller for Android devices, we go hands-on originally appeared on Engadget on Thu, 31 May 2012 16:08:00 EDT. Please see our terms for use of feeds.

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Did Madonna Diss Lady Gaga During Concert? Likes or Yikes?

The queen of pop covered one of Lady Gaga’s songs in concert, but was it an homage or a jab? Plus, the second Hunger Games movie Catching Fire may be close to casting its new leading man, and Ariel Tweto from Discovery’s Flying Wild Alaska joins Pat Sandora as co-host. Get more celeb news and photos at iVillage.com/LikesorYikes

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Video: 'Game On' for Glu Mobile?

Niccolo de Masi, Glu Mobile CEO, tells CNBC's "Fast Money" the firm is well-positioned to keep growing as a standalone company.

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The Research of Computerized Accounting Teaching in Secondary ...

Abstract

Computerized Accounting is accounting and computer science and technology of combining an edge applications disciplines. According to the provisions in the <knowledge training and management approach of computerized accounting> promulgated by the Ministry of Finance, knowledge training of Computerized Accounting is divided into three levels: primary, intermediate and advanced. Secondary vocational schools teaching in the computerized accounting objectives should be targeted in the majority of students ?primary? level, Even students with the basic computer operation and maintenance capability, can use existing computer systems to master the use of related applications with accounting software skillfully, can do a good job of accounting data collection, storage, processing and transmission and so on. A minority of students reaches or approaches the ?intermediate? level. That is able to carry out general maintenance of the accounting software or set up parameters to provide operational support for the development of accounting software. Now, in our country, there are some common problems in the teaching of computerized accounting. They are mainly about the diversity of teaching objects, materials content of confusing, the mode of teaching simplified the process of mechanization and other phenomena in the actual process of teaching.This article?s purpose and significance are: 1. Discuss the mode of teaching computerized accounting on the multimedia environment (especially the network environment), to offer new ideas for the teaching of computerized accounting. 2. Research in the teaching content and teaching methods of computerized accounting in secondary vocational schools, to supply some references for the teaching in secondary vocational schools. 3. Research the teaching effectiveness after the reform of the computerized accounting education on the network environment, to improve students?ability of self-study, inquiry learning to provide reference value.This article?s research ideas are: to analysis from the development process and the current problems that exist in secondary vocational schools on computerized accounting teaching, research into teaching mode of computerized accounting, reform the content, design the system of teaching content and research specific teaching implementation and effect analysis about the course of computerized accounting.This article?s innovative research in the following areas:1. According to the objective of computerized accounting, to reform the teaching content, design the system of teaching content, designed and developed the software to use in the network course which suit for the computerized accounting in secondary vocational schools, as a platform for inquiry learning.2. Research into the teaching mode of computerized accounting in secondary vocational schools.3. To use of educational technology, research specific teaching implementation and effect analysis about the course of computerized accounting, to offer the reference for the development of computerized accounting teaching in secondary vocational schools.

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X-ray 'echoes' map a supermassive black hole's environs in distant galaxies

ScienceDaily (May 31, 2012) ? An international team of astronomers using data from the European Space Agency's (ESA) XMM-Newton satellite has identified a long-sought X-ray "echo" that promises a new way to probe supersized black holes in distant galaxies.

Most big galaxies host a big central black hole containing millions of times the sun's mass. When matter streams toward one of these supermassive black holes, the galaxy's center lights up, emitting billions of times more energy than the sun. For years, astronomers have been monitoring such "active galactic nuclei" (AGN) to better understand what happens on the brink of a monster black hole.

"Our analysis allows us to probe black holes through a different window. It confirms some long-held ideas about AGN and gives us a sense of what we can expect when a new generation of space-based X-ray telescopes eventually becomes available," said Abderahmen Zoghbi, a postdoctoral research associate at the University of Maryland at College Park (UMCP) and the study's lead author.

One of the most important tools for astronomers studying AGN is an X-ray feature known as the broad iron line, now regarded as the signature of a rotating black hole. Excited iron atoms produce characteristic X-rays with energies around 6,000 to 7,000 electron volts -- several thousand times the energy in visible light -- and this emission is known as the iron K line.

Matter falling toward a black hole collects into a rotating accretion disk, where it becomes compressed and heated before eventually spilling over the black hole's event horizon, the point beyond which nothing can escape and astronomers cannot observe. A mysterious and intense X-ray source near the black hole shines onto the disk's surface layers, causing iron atoms to radiate K-line emission. The inner part of the disk is orbiting the black hole so rapidly that the effects of Einstein's relativity come into play -- most notably, how time slows down close to the black hole. These relativistic effects skew or broaden the signal in a distinctive way.

Astronomers predicted that when the X-ray source near the black hole flared, the broad iron K line would brighten after a delay corresponding to how long the X-rays took to reach and illuminate the accretion disk. Astronomers call the process relativistic reverberation. With each flare from the X-ray source, a light echo sweeps across the disk and the iron line brightens accordingly.

Unfortunately, neither ESA's XMM-Newton satellite nor NASA's Chandra X-ray Observatory possess telescopes powerful enough to spot reverberations from individual flares.

he team reasoned that detecting the combined echoes from multiple flares might be possible if a sufficiently large amount of data from the right object could be analyzed. The object turned out to be the galaxy NGC 4151, which is located about 45 million light-years away in the constellation Canes Venatici. As one of the brightest AGN in X-rays, NGC 4151 has been observed extensively by XMM-Newton. Astronomers think that the galaxy's active nucleus is powered by a black hole weighing 50 million solar masses, which suggested the presence of a large accretion disk capable of producing especially long-lived and easily detectable echoes.

Since 2000, XMM-Newton has observed the galaxy with an accumulated exposure of about four days. By analyzing this data, the researchers uncovered numerous X-ray echoes, demonstrating for the first time the reality of relativistic reverberation. The findings appear in the May 8 issue of Monthly Notices of the Royal Astronomical Society.

The team found that echoes lagged behind the AGN flares by a little more than 30 minutes. Moving at the speed of light, the X-rays associated with the echo must have traveled an additional 400 million miles -- equivalent to about four times Earth's average distance from the sun -- than those that came to us directly from the flare.

"This tells us that the mysterious X-ray source in AGN hovers at some height above the accretion disk," said co-author Chris Reynolds, a professor of astronomy at UMCP and Zoghbi's adviser. Jets of accelerated particles often are associated with AGN, and this finding meshes with recent suggestions that the X-ray source may be located near the bases of these jets.

"The data show that the earliest echo comes from the most broadened iron line emission. This originates from closest to the black hole and fits well with expectations," said co-author Andy Fabian, an astrophysicist at the University of Cambridge in England.

Amazingly, the extreme environment at the heart of NGC 4151 is built on a scale comparable to our own solar system. If we replaced the sun with the black hole, the event horizon would extend less than halfway to Earth if the black hole spins rapidly; slower spin would result in a larger horizon. The X-ray source would hover above the black hole and its accretion disk at a distance similar to that between the sun and the middle of the asteroid belt.

"Teasing out the echo of X-ray light in NGC 4151 is a remarkable achievement. This work propels the science of AGN into a fundamental new area of mapping the neighborhoods of supermassive black holes," said Kimberly Weaver, an astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Md., who was not involved in the study. NASA Goddard hosts the XMM-Newton Guest Observer Facility, which supports U.S. astronomers who request observing time on the satellite.

The detection of X-ray echoes in AGN provides a new way of studying black holes and their accretion disks. Astronomers envision the next generation of X-ray telescopes with collecting areas large enough to detect the echo of a single AGN flare in many different objects, thereby providing astronomers with a new tool for testing relativity and probing the immediate surroundings of massive black holes.

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The above story is reprinted from materials provided by NASA/Goddard Space Flight Center.

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