Invention of the 4th Circuit element

Filed under: , by: Jubin

1 May 2008--Anyone familiar with electronics knows the trinity of fundamental components: the resistor, the capacitor, and the inductor. In 1971, a University of California, Berkeley, engineer predicted that there should be a fourth element: a memory resistor, or memristor. But no one knew how to build one. Now, 37 years later, electronics have finally gotten small enough to reveal the secrets of that fourth element. The memristor, Hewlett-Packard researchers revealed today in the journal Nature , had been hiding in plain sight all along--within the electrical characteristics of certain nanoscale devices. They think the new element could pave the way for applications both near- and far-term, from nonvolatile RAM to realistic neural networks. The memristor's story starts nearly four decades ago with a flash of insight by IEEE Fellow and nonlinear-circuit-theory pioneer Leon Chua. Examining the relationships between charge and flux in resistors, capacitors, and inductors in a 1971 paper, Chua postulated the existence of a fourth element called the memory resistor. Such a device, he figured, would provide a similar relationship between magnetic flux and charge that a resistor gives between voltage and current. In practice, that would mean it acted like a resistor whose value could vary according to the current passing through it and which would remember that value even after the current disappeared. But the hypothetical device was mostly written off as a mathematical dalliance. Thirty years later, HP senior fellow Stanley Williams and his group were working on molecular electronics when they started to notice strange behavior in their devices. ”They were doing really funky things, and we couldn't figure out what [was going on],” Williams says. Then his HP collaborator Greg Snider rediscovered Chua's work from 1971. ”He said, ’Hey guys, I don't know what we've got, but this is what we want ,' ” Williams remembers. Williams spent several years reading and rereading Chua's papers. ”It was several years of scratching my head and thinking about it.” Then Williams realized their molecular devices were really memristors. ”It just hit me between the eyes.” The reason that the memristor is radically different from the other fundamental circuit elements is that, unlike them, it carries a memory of its past. When you turn off the voltage to the circuit, the memristor still remembers how much was applied before and for how long. That's an effect that can't be duplicated by any circuit combination of resistors, capacitors, and inductors, which is why the memristor qualifies as a fundamental circuit element. The classic analogy for a resistor is a pipe through which water (electricity) runs. The width of the pipe is analogous to the resistance of the flow of current--the narrower the pipe, the greater the resistance. Normal resistors have an unchanging pipe size. A memristor, on the other hand, changes with the amount of water that gets pushed through. If you push water through the pipe in one direction, the pipe gets larger (less resistive). If you push the water in the other direction, the pipe gets smaller (more resistive). And the memristor remembers. When the water flow is turned off, the pipe size does not change. Such a mechanism could technically be replicated using transistors and capacitors, but, Williams says, ”it takes a lot of transistors and capacitors to do the job of a single memristor.” The memristor's memory has consequences: the reason computers have to be rebooted every time they are turned on is that their logic circuits are incapable of holding their bits after the power is shut off. But because a memristor can remember voltages, a memristor-driven computer would arguably never need a reboot. ”You could leave all your Word files and spreadsheets open, turn off your computer, and go get a cup of coffee or go on vacation for two weeks,” says Williams. ”When you come back, you turn on your computer and everything is instantly on the screen exactly the way you left it.” Chua deduced the existence of memristors from the mathematical relationships between the circuit elements. The four circuit quantities (charge, current, voltage, and magnetic flux) can be related to each other in six ways. Two quantities are covered by basic physical laws, and three are covered by known circuit elements (resistor, capacitor, and inductor), says Columbia University electrical engineering professor David Vallancourt. That leaves one possible relation unaccounted for. Based on this realization, Chua proposed the memristor purely for the mathematical aesthetics of it, as a class of circuit element based on a relationship between charge and flux.


Chua calls the HP work a paradigm shift; he likens the addition of the memristor to the circuit design arsenal to adding a new element to the periodic table: for one thing, ”now all the EE textbooks need to be changed,” he says.
So why hadn't anyone seen memristance? Chua actually produced a memristor in the 1970s with an impractical combination of resistors, capacitors, inductors, and amplifiers as a proof of concept. But memristance as a property of a material was, until recently, too subtle to make use of. It is swamped by other effects, until you look at materials and devices that are mere nanometers in size.
No one was looking particularly hard for memristance, either. In the absence of an application, there was no need. No engineers were saying, ”If we only had a memristor, we could do X,” says Vallancourt. In fact, Vallancourt, who has been teaching circuit design for years, had never heard of memristance before this week.
"now all the EE textbooks need to be changed"
-IEEE Kirchoff Award winner Leon Chua on the discovery of the memresistor.
But the smaller the scales of the devices scientists and engineers were working with got, the more the devices started behaving with the postulated ”memristor” effect, says Chua, who is now a senior professor at Berkeley.
There had been clues to the memristor's existence all along. ”People have been reporting funny current voltage characteristics in the literature for 50 years,” Williams says. ”I went to these old papers and looked at the figures and said, ’Yup, they've got memristance, and they didn't know how to interpret it.' ”
”Without Chua's circuit equations, you can't make use of this device,” says Williams. ”It's such a funky thing. People were using all the wrong circuit equations. It's like taking a washing machine motor and putting it into a gasoline-powered car and wondering why it won't run.”
Williams found an ideal memristor in titanium dioxide--the stuff of white paint and sunscreen. Like silicon, titanium dioxide (TiO 2 ) is a semiconductor, and in its pure state it is highly resistive. However, it can be doped with other elements to make it very conductive. In TiO 2 , the dopants don't stay stationary in a high electric field; they tend to drift in the direction of the current. Such mobility is poison to a transistor, but it turns out that's exactly what makes a memristor work. Putting a bias voltage across a thin film of TiO 2 semiconductor that has dopants only on one side causes them to move into the pure TiO 2 on the other side and thus lowers the resistance. Running current in the other direction will then push the dopants back into place, increasing the TiO 2 's resistance.
HP Labs is now working out how to manufacture memristors from TiO 2 and other materials and figuring out the physics behind them. They also have a circuit group working out how to integrate memristors and silicon circuits on the same chip. The HP group has a hybrid silicon CMOS memristor chip ”sitting on a chip tester in our lab right now,” says Williams.
The implications for circuit design may be niche at the moment. ”This will require a fair amount of work to exploit,” says Columbia's Vallancourt. Applications will have to be identified in which the memristor's unique characteristics offer possibilities not covered by today's components.
Williams is in talks with several neuroscience/engineering labs that are pursuing the goal of building devices that emulate neural systems. Chua says that synapses, the connections between neurons, have some memristive behavior. Therefore, a memristor would be the ideal electronic device to emulate a synapse.
By redesigning certain types of circuits to include memristors, Williams expects to obtain the same function with fewer components, making the circuit itself less expensive and significantly decreasing its power consumption. In fact, he hopes to combine memristors with traditional circuit-design elements to produce a device that does computation in a non-Boolean fashion. ”We won't claim that we're going to build a brain, but we want something that will compute like a brain,” Williams says. They think they can abstract ”the whole synapse idea” to do essentially
analog computation in an efficient manner. ”Some things that would take a digital computer forever to do, an analog computer would just breeze through,” he says.
The HP group is also looking at developing a memristor-based nonvolatile memory. ”A memory based on memristors could be 1000 times faster than magnetic disks and use much less power,” Williams says, sounding like a kid in a candy store.
Chua agrees that nonvolatile memory is the most near-term application. ”I'm very happy that this is a breakthrough,” he says. ”The reality is that at the nanoscale, this effect becomes dominant, and you'll find it whether you like it or not. I'm glad I can point people in the right direction.”

Cool Cosmos Photos Part 5

Filed under: by: Necrobutcher


Several hundred never before seen galaxies are visible in this "deepest-ever" view of the universe, called the Hubble Deep Field (HDF), made with NASA's Hubble Space Telescope. Besides the classical spiral and elliptical shaped galaxies, there is a bewildering variety of other galaxy shapes and colors that are important clues to understanding the evolution of the universe. Some of the galaxies may have formed less that one billion years after the Big Bang.

Representing a narrow "keyhole" view all the way to the visible horizon of the universe, the HDF image covers a speck of sky 1/30th the diameter of the full Moon (about 25% of the entire HDF is shown here). This is so narrow, just a few foreground stars in our Milky Way galaxy are visible and are vastly outnumbered by the menagerie of far more distant galaxies, some nearly as faint as 30th magnitude, or nearly four billion times fainter than the limits of human vision. (The relatively bright object with diffraction spikes just left of center may be a 20th magnitude star.) Though the field is a very small sample of sky area it is considered representative of the typical distribution of galaxies in space because the universe, statistically, looks the same in all directions.

The image was assembled from many separate exposures (342 frames total were taken, 276 have been fully processed to date and used for this picture) with the Wide Field and Planetary Camera 2 (WFPC2), for ten consecutive days between December 18 to 28, 1995. This picture is from one of three wide-field CCD (Charged Coupled Device) detectors on the WFPC2.

This "true-color" view was assembled from separate images were taken in blue, red, and infrared light. By combining these separate images into a single color picture, astronomers will be able to infer — at least statistically — the distance, age, and composition of galaxies in the field. Bluer objects contain young stars and/or are relatively close, while redder objects contain older stellar populations and/or farther away.


(with inputs from HubbleSite News Center)

It's been a long time since I last contributed to this series. Sorry for the delay and hope you enjoy.

Google talk:useful tricks

Filed under: by: arnab7889

TRICK 1:
create a desktop shortcut for your friend->To create a desktop shortcut to quickly chat with your GTalk friend, just right

click on your desktop and go to New > Shortcut and type gtalk:chat?jid=username@gmail.com. To initiate a quick call, use the shortcut gtalk:call?jid=username@gmail.com where username should be replaced by your buddy’s GTalk ID. This method doesn’t work on Windows Vista, but only on XP.

TRICK 2:
KEYBOARD SHORTCUTS->
Google Talk provides plenty of keyboard shortcuts that you can use to perform a variety of actions. Their documentation doesn’t seem to be listing the shortcuts though, so here’s a list of many user discovered shortcuts. Learn them once, and you’ll find them indispensable forever.


1. CTRL + Mousewheel up/down: It will change the font size in a conversation window.
2. CTRL + E: Center text
3. CTRL + R: Right justify text
4. CTRL + L: Left justify text
5. F11: Start a call
6. F12: Stop the call
7. ESC: Close the current window
8. ALT + ESC: Minimize the current window.
9. CTRL + SHIFT + L: Switch between points, numbers, letters, capital letters, roman numbers and capital roman numbers.
10. TAB: Switch between multiple chat windows.
11. CTRL + I: Same as TAB.
12. SHIFT + TAB: Same as TAB but in reverse order.
13. CTRL + TAB: Same as SHIFT + TAB.

TRICK 3:
CHANGE THE FORMAT->
Did you know that you can format text on Google Talk even though there are no visible buttons present for that purpose. You can do basic formatting in Google Talk like making the text bold, italic and underline. To make the text bold, just enclose it within *asterisks* and to make it italic, just enclose it within _underscores_


TRICK 4:
THE BEST OF THE TRICK.RUN MULTIPLE GTALK WINDOWS AT A TIME.HERE IS A PICTURE TO MAKE IT CLEAR.

Google Talk, by default, doesn’t provide a way to log in to multiple accounts at once. However, you can achieve that by a workaround.

Just edit your existing desktop shortcut to Google Talk by right clicking on the desktop icon, going to properties and then appending the parameter /nomutex to the target, like this: C:Program FilesGoogleGoogle Talk.exe /nomutex. You can use this shortcut to launch multiple instances of Google Talk, thereby allowing you to login to multiple Google Talk accounts simultaneously.

Hope this tricks proves helpful to you.Anyways I always feel Yahoo messenger is better than google talk, there you don't need to do all these.

Cool Cosmos Photos Part 4

Filed under: by: Necrobutcher


In the direction of the constellation Canis Major, two spiral galaxies pass by each other like majestic ships in the night. The near-collision has been caught in images taken by NASA's Hubble Space Telescope and its Wide Field Planetary Camera 2.

The larger and more massive galaxy is cataloged as NGC 2207 (on the left in the Hubble Heritage image), and the smaller one on the right is IC 2163. Strong tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging out stars and gas into long streamers stretching out a hundred thousand light-years toward the right-hand edge of the image.


(with inputs from HubbleSite NewsCenter)

Enjoy

Cool Cosmos Photos - Part 3

Filed under: by: Necrobutcher


Undersea corral? Enchanted castles? Space serpents? These eerie, dark pillar-like structures are actually columns of cool interstellar hydrogen gas and dust that are also incubators for new stars. The pillars protrude from the interior wall of a dark molecular cloud like stalagmites from the floor of a cavern. They are part of the "Eagle Nebula" (also called M16 — the 16th object in Charles Messier's 18th century catalog of "fuzzy" objects that aren't comets), a nearby star-forming region 6,500 light-years away in the constellation Serpens.

The pillars are in some ways akin to buttes in the desert, where basalt and other dense rock have protected a region from erosion, while the surrounding landscape has been worn away over millennia. In this celestial case, it is especially dense clouds of molecular hydrogen gas (two atoms of hydrogen in each molecule) and dust that have survived longer than their surroundings in the face of a flood of ultraviolet light from hot, massive newborn stars (off the top edge of the picture). This process is called "photoevaporation. "This ultraviolet light is also responsible for illuminating the convoluted surfaces of the columns and the ghostly streamers of gas boiling away from their surfaces, producing the dramatic visual effects that highlight the three-dimensional nature of the clouds. The tallest pillar (left) is about about 4 light-years long from base to tip.

As the pillars themselves are slowly eroded away by the ultraviolet light, small globules of even denser gas buried within the pillars are uncovered. These globules have been dubbed "EGGs." EGGs is an acronym for "Evaporating Gaseous Globules," but it is also a word that describes what these objects are. Forming inside at least some of the EGGs are embryonic stars — stars that abruptly stop growing when the EGGs are uncovered and they are separated from the larger reservoir of gas from which they were drawing mass. Eventually, the stars themselves emerge from the EGGs as the EGGs themselves succumb to photoevaporation.

The picture was taken on April 1, 1995 with the Hubble Space Telescope Wide Field and Planetary Camera 2. The color image is constructed from three separate images taken in the light of emission from different types of atoms. Red shows emission from singly-ionized sulfur atoms. Green shows emission from hydrogen. Blue shows light emitted by doubly- ionized oxygen atoms.


(with inputs from HubbleSite NewsCenter)


This is one of Hubble's most famous images, known as The Pillars Of Creation. Enjoy.

Duckworth-Lewis - my understanding

Filed under: by: arnab7889



The Duckworth/Lewis system was invented by two statisticians, Frank Duckworth and Tony Lewis in an attempt to solve the perennial problem of creating a fair target for the side batting second in a limited-overs match shortened by the weather(rain,bad light,sand storm even snow storm) or problems due to artificial lights.

At its simplest, the problem is this. If the side batting first in a 50-over match makes 250 runs, the target for the side batting second is 250 to tie, 251 to win. Their average run-rate must therefore exceed 5 per over if they are to win in a full 50 overs. But if rain or bad light stops further play after only 20 overs, during which the second side score 101 runs, then comparing average run-rates would make the second side the winner. But if they had lost nine wickets in gaining those 101 runs, then few would give much for their chances in an uninterrupted 50 overs. So the old average-run rate system gave an unfair advantage to the side batting second if the number of overs was reduced. They could blaze away without worrying too much about losing wickets. Other variants were tried, such as basing the target on the best overs of the side batting first, but this was unfair to the side batting second.

Enter Messrs Duckworth and Lewis, who studied the performances in a great number of limited overs matches, and concluded that the factor to take into account was what they called the "resources" available to each side. The resources depend on the number of wickets lost and the number of balls remaining to be bowled.

But the calculations are very cumbersome,so I am giving the link to duckworth-lewis calculator.So whenever you have interrupted cricket you know where to log in.
duckworth-lewis calculator

Having said all this how often we have seen team getting duckworth-lewis wrong(for eg south africa in 2003 WC), or how often we have seen teams getting undue advantage.It's the only way to avoid bad weather is to cover the stadiums provided the floodlights are working properly,else you will require duckworth-lewis again.

Information:duckworth-lewis.com

Cool Cosmos Photos - Part 2

Filed under: by: Necrobutcher


Over the past 19 years Hubble has taken dozens of exotic pictures of galaxies going "bump in the night" as they collide with each other and have a variety of close encounters of the galactic kind. Just when you thought these interactions couldn't look any stranger, this image of a trio of galaxies, called Arp 194, looks like one of the galaxies has sprung a leak. The bright blue streamer is really a stretched spiral arm full of newborn blue stars. This typically happens when two galaxies interact and gravitationally tug at each other.

Resembling a pair of owl eyes, the two nuclei of the colliding galaxies can be seen in the process of merging at the upper left. The blue bridge looks like it connects to a third galaxy. In reality the galaxy is in the background and not connected at all. Hubble's sharp view allows astronomers to try and visually sort out what are foreground and background objects when galaxies, superficially, appear to overlap. This picture was issued to celebrate the 19th anniversary of the launch of the Hubble Space Telescope aboard the space shuttle Discovery in 1990. During the past 19 years Hubble has made more than 880,000 observations and snapped over 570,000 images of 29,000 celestial objects.


(with inputs from HubbleSite SpaceCenter)


Enjoy.

Cool Cosmos Photos - 1

Filed under: by: Necrobutcher


This composite image shows the jet from a black hole at the center of a galaxy striking the edge of another galaxy,

the first time such an interaction has been found. In the image, data from several wavelengths have been combined. X-rays from Chandra (colored purple), optical and ultraviolet (UV) data from Hubble (red and orange), and radio emission from the Very Large Array (VLA) and MERLIN (blue) show how the jet from the main galaxy on the lower left is striking its companion galaxy to the upper right. The jet impacts the companion galaxy at its edge and is then disrupted and deflected, much like how a stream of water from a hose will splay out after hitting a wall at an angle.

Each wavelength shows a different aspect of this system, known as 3C321. The Chandra X-ray image provides evidence that each galaxy contains a rapidly growing supermassive black hole at its center. Hubble's optical light images (orange) show the glow from the stars in each galaxy. A bright spot in the VLA and MERLIN radio image shows where the jet has struck the side of the galaxy - about 20,000 light-years from the main galaxy - dissipating some of its energy. An even larger "hotspot" of radio emission detected by VLA (seen in an image with a much larger field-of-view) reveals that the jet terminates much farther away from the galaxy, at a distance of about 850,000 light-years away. The Hubble UV image shows large quantities of warm and hot gas in the vicinity of the galaxies, indicating the supermassive black holes in both galaxies have had a violent past. Faint emission from Chandra, Hubble and Spitzer, not shown in this image, indicate that the galaxies are orbiting in a clockwise direction, implying that the companion galaxy is swinging into the path of the jet.

Since the Chandra data shows that particle acceleration is still occurring in this hotspot, the jet must have struck the companion galaxy relatively recently, less than about a million years ago (i.e. less than the light travel time to the hotspot). This relatively short cosmic time frame makes this event a very rare phenomenon. This "death star galaxy" will produce large amounts of high-energy radiation, which may cause severe damage to the atmospheres of any planets in the companion galaxy that lie in the path of the jet. From the Earth we look down the barrel of jets from supermassive black holes, however these so-called "blazars" are at much safer distances of millions or billions of light-years.

(with inputs from HubblesSite Space Center)

This is the first in a series( I hope!). I wil be publishing the rest soon. Let me know what you think of it. 

KERS-curse or boon

Filed under: by: arnab7889


This a new technology that has been introduced in F1 this year ,which has made it even more interesting.
KERS-kinetic energy recovery system.

The most important thing about KERS is that it is not a compulsory regulation change. The technology has been suggested as an improvement to Formula 1 as it saves on energy and therefore helps to improve the green image of the sport. The basic premise of KERS is that energy that is usually lost during braking is stored and/or converted into more power.

There are two types of system: the battery and flywheel. The first is an obvious concept where the excess power is stored in a battery until being released when required. The flywheel option means the energy is used constantly but connecting to the flywheel only occurs when the power boost is needed. At the moment, the regulations look as if they are heading towards a boost button, which a driver can use when he is lining up behind another car and ready to overtake, or is about to be overtaken.

We’ve already seen problems in testing the new technology. Red Bull have seen a component fail at their factory causing an evacuation due to the smoke released. A BMW mechanic had a well publicised electric shock, and drivers have expressed concerns.

There are other problems as well, though. Whether a team is implementing a battery or a flywheel, the new components need to be housed in the car, and will have to be as light as possible. If a car has stored electricity and comes to a stop, either in the pit lane, or out on track, the power needs to be discharged before anyone can approach the vehicle safely. This means mechanics and marshals taking extra precautions before dealing with a car.

It doesn’t appear that there is a vast improvement in terms of speed and performance yet, however the technology is in its very early stages. The FIA have mandated the stages at which development should take place, if a team choose to implement KERS, but it will take a few years before we see any major influence on track action. Most teams and drivers are open to the new technology, but perhaps skeptical about its benefits and concerned about safety.

But the best thing that has happened for F1 is that the title race is very open now,for the last few years we have seen that it was battle between ferrari,mclaren,renault for the top position.Now the compettion has opened up for all.Ferrari the last years constructer's champion has failed to score a single point in the 1st 3 races,Mclaren isn't doing well either,whereas teams like red bull,brawn gp(formerly honda infact honda sold their team)williams,toyota are doing reamarkably well.So we are in for a pleasant surprise.




LOOK OUT.........EYES OVER THE SKY

Filed under: by: AMITSAHA27


Is this a treat to the terrorists ?.......YES now we are looking to every activity of the terrorists.

HOW ???
....................RISAT-2

Yes I am talking about the spy satellite RISAT-2.

India launched an Israeli made spy satellite RITSAT-2 on Monday that will help it keep a close eye on its borders stretching from Pakistan in the west to China in the north and east.The PSLVC12 rocket manufactured by Indian Space and Research Organisation lifted the surveillance satellite at 6.45 am from the spaecport in Srikarikota in Orissa state and placed its first Radar Imaging Satellite (RISAT2) and micro-educational satellite ANUSAT into orbit about 19 minutes later in a textbook launch, it was officially said.

Thus the INDIAN ARMY is strengthed by this spy satellite. It gives India an eye (through clouds and other weather vagaries) on its restive borders with pakistan, China and Bangladesh.

The satellite is supposed to be an all-seeing all-weather platform that at a height of 550 kms lets you see things like a motorbike on the street.This means terrorist movement on the LoC will now have a greater chance of being picked up by Indian forces.

India is much more safer now.....but not the jihadis.......