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What was highest label on your first car speedometer?

  • 80 mph
  • 88 mph
  • 100 mph
  • 120 mph
  • 150 mph
  • it was in kph like civilized countries use you insensitive clod
  • Other (please specify in comments)

[ Results | Polls ]
Comments:71 | Votes:290

posted by janrinok on Sunday July 26 2015, @11:53PM   Printer-friendly
from the let-the-games-begin dept.

Videogame giants will soon be able to manufacture and sell consoles in China, after Beijing said it was lifting a ban first instituted in 2000.

Rules were relaxed in the country in 2014 to allow for the production and sale of "gaming entertainment" in the newly created Shanghai Free Trade Zone.

Now, according to the Wall Street Journal , the country's Ministry of Culture said that foreign and domestic console vendors would soon be able to make and sell their wares in the People's Republic.

It means that the likes of home-grown console manufacturer Eedoo, which is backed by Lenovo, will be competing with Microsoft, Sony and Nintendo.

China's gamers – having adapted to Beijing's attempt to protect its youth from supposedly unhealthy content – are big fans of massively multi-player online role-playing (MMORPG), which work better on PCs than consoles.

That said, the world's biggest videogame makers will no doubt be relishing the opportunity to return to such a potentially huge market.


Original Submission

posted by janrinok on Sunday July 26 2015, @10:07PM   Printer-friendly
from the me-and-my-mechanical-buddy dept.

Slate and University of Washington have recent articles discussing robotics and the issue of how hard they say it is to even begin to define the nature and scope of robotics, let alone something like liability resulting from harm. They say:

Robots display increasingly emergent behavior...in the sense of wondrous complexity created by simple rules and interactions—permitting the technology to accomplish both useful and unfortunate tasks in unexpected ways. And robots, more so than any technology in history, feel to us like social actors—a tendency so strong that soldiers sometimes jeopardize themselves [livescience.com] to preserve the "lives" of military robots in the field.

[Robotics] combines, arguably for the first time, the promiscuity of information with the capacity to do physical harm. Robotic systems accomplish tasks in ways that cannot be anticipated in advance, and robots increasingly blur the line between person and instrument. Today, software can touch you, which may force courts and regulators to strike a new balance.

This seems like calmly worded yet unnecessary hype that is severely premature. Why not simply hold manufactures and owners responsible like we do now? I suppose this ignores the possibility of eventual development of true AI, where such an entity might be 'a person' who could be sued or thrown in jail. If it's an AI iteration that is only as smart as a dog, then the dog's owner pays if it bites.


Original Submission

posted by janrinok on Sunday July 26 2015, @08:49PM   Printer-friendly
from the it's-going-to-rain-or-go-dark-before-tomorrow dept.

Here is a rather cool demonstration of receiving weather satellite images with a low cost USB dongle.

There are several American NOAA weather satellites in a polar orbit around Earth, each of which will pass the same point below every 12 hours or so. The satellites transmit pictures via FM radio at 137MHz. Using a DAB/FM/Freeview dongle, you can receive this signal on a computer running software-defined radio (SDR) software, and then decode it into a picture.

The receiver in this case is a Nooelec R820T USB Dongle, and several other neat SDR applications are also possible with this hardware.

Originally spotted on Lobsters


Original Submission

posted by janrinok on Sunday July 26 2015, @08:13PM   Printer-friendly
from the star-gazing dept.

[Ed: I realise that we have a good number amongst us who are particularly interested in space and the heavens. This 'story' is simply a long list of the best photographs seen this week, in the opinion of Wired, on matters related to the 'final frontier'. It will not be to everyone's taste - but I hope that at least some of us will find it interesting. If it is not for you, please hang on for the next story which will be along shortly.]

After a brief hiatus, WIRED is pleased to once again show you the very best the universe has to offer (and a GIF for good measure). We’ve heard your pleas: space photos are back.


Original Submission

And here we go!

Caption: A new false color image of Pluto released by New Horizons. The photo was enhanced to show differences in the dwarf planet’s texture and composition. NASA/JHUAPL/SwRI [Image]

Caption: Hubble Space Telescope captures the NGC 1140, a dwarf galaxy experiencing a starburst, an exceptionally high rate of star formation. The small galaxy is creating one star the size of our sun a year, the same rate as the much larger Milky Way. ESA/Hubble & NASA [Image]

Caption: A ‘mother daughter’ portrait of two of Saturn’s moons, Dione (top) and Tethys (bottom). Named after Greek mythology, the moons are believed to have formed out of the same disk when Saturn was young. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: This photo was taken by a NASA camera on the Deep Space Climate Observatory (DSCOVR), capturing the sunlit side of Earth from one million miles away. The color photos were made with the Earth Polychromatic Imaging Camera (EPIC), using three separate images to create this high res view. NASA [Image]

Caption: Two of Pluto’s smaller moons, Nix (left) and Hydra (right). Nix has enhanced color taken by Ralph while Hydra remains in black and white taken by LORRI. Scientists note Hyrda’s strange shape and have estimated the moon to be only 34 miles long and 25 miles wide. NASA/JHUAPL/SWRI [Image]

Caption: New Horizons final image of Pluto taken on July 15. The dwarf planet is silhouetted against the sun and highlighting Pluto’s atmosphere, which appears to be much larger than scientists first predicted. NASA/JHUAPL/SwRI [Image]

Caption: A photo of BDF 3299, a far away galaxy seen when the Universe was less than 800 million years old. Taken by the ALMA and the Very Large Telescope, the image shows a bright red spot which is a large cloud of material assembling a young galaxy. ESO/R. Maiolino [Image]

Caption: An image of Pluto (right) and Charon (left), one of the dwarf planet’s five moons. Data from New Horizons has determined Pluto to be 1,473 miles in diameter, a bit larger than many previous estimates. Charon is confirmed as 751 miles in diameter. NASA-JHUAPL-SWRI [Image]

Caption: A color image of Pluto taken on July 13, 2015. This photo is a combination of a black-and-white image snapped by LORRI and color captured by Ralph. New Horizons traveled nearly 3 billion miles and 10 years to reach the dwarf planet. NASA/APL/SwRI [Image]

Caption: An up close photo of Pluto shows icy mountains thought to be less than 100 million years old. “This is one of the youngest surfaces we’ve ever seen in the solar system,” says Jeff Moore, GGI team leader of NASA’s Ames Research Center. NASA-JHUAPL-SwRI [Image] [Image]

Caption: This photo is a detail of Pluto’s heart-shaped region nicknamed “Tombaugh Regio.” In the center are frozen plains that look a lot like mud cracks. The shapes are sporadic and surrounded by thin troughs. NASA/JHUAPL/SWRI [Image]

Caption: New details of Charon, Pluto’s largest moon. The surface has cliffs and troughs about 600 miles across, but very few craters. Preliminary research indicates the moon’s surface is fairly young, reshaped by geologic activity. NASA-JHUAPL-SwRI [Image]

Caption: This photo shows Pluto and Charon in false color to highlight the different features on each surface. The exaggeration shows Pluto’s “big heart,” a large feature that appears to have varying geologic, tectonic or morphologic origins. NASA/APL/SwRI [Image]

In case you missed it, NASA flew a probe by Pluto this week. And although we’re sure there are other space photos from the last seven days, nobody’s looking at them. So here are some highlights from a historic week of the little planet we never forgot. [Image]

Caption: This image is one of the first results from Kilo-Degree Survey (KiDS) project, using images from the VLT Survey Telescope and the massive camera OmegaCAM. The purple color is actually a combination of invisible dark matter and visible light. Kilo-Degree Survey Collaboration/A. Tudorica & C. Heymans/ESO [Image]

Caption: This photo is of Saturn’s moon Prometheus (top right corner), which sometimes orbits near Saturn’s F ring. When the moon goes into the ring, it often eaves a hole in the smaller ring particles. Previous entries can be see by the dark streaks near the bottom of the image. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: An example of a little-known spiral galaxy, often called LEDA 89996. The dark patches in the spirals are dust and gas which can be used as raw materials for new stars. The image was created by Hubble’s new camera which has captured some of the sharpest views of space to date. ESA/Hubble & NASA [Image]

Caption: A photo of Venus from the Hinode’s Solar Optical Telescope, beginning its rare orbit between Earth and the sun. Scientists have been studying images of the last event in 2012 to glean new information on the sun’s impact on Venus’ atmosphere during this period. JAXA/NASA/Hinode [Image]

Caption: The new Hubble Space Telescope took a photo of ESO 381-12, a galaxy which appears to have had a dramatic collision sometime in the recent past. It has an unusual shape, with delicate shells that bloom outward and still remain somewhat of a mystery to astronomers. NASA, ESA, P. Goudfrooij (STScI) [Image]

Caption: A Pluto flyby begins! NASA’s New Horizons spacecraft has finally made the nine-year, three-billion-mile trek to Pluto. Up-to-date coverage can be found on WIRED. NASA-JHUAPL-SWRI [Image]

Caption: This GIF is created from an images of “nested rings of X-ray light” around an erupting black hole. It was taken by NASA’s Swift satellite. The multiple rings are caused by multiple reflecting dust layers up to 7,000 light-years away. Andrew Beardmore (Univ. of Leicester) and NASA/Swift [Image]

Caption: An image of the planetary nebula NGC 6153, which is located about 4,000 light-years away in the southern constellation of Scorpius (The Scorpion). The blue haze is from a star like the sun that has depleted most of its fuel. ESA/Hubble & NASA, Acknowledgement: Matej Novak [Image]

Caption: A M7.9-class solar flare on June 25. Harmful radiation from a flare cannot pass through Earth's atmosphere, but the flares can disturb the atmosphere in the layer where GPS and communications signals travel. NASA/SDO [Image]

Caption: A photograph of the largest and brightest set of rings from X-ray light echoes ever observed. The rings were produced by a flare from a neutron star and gave astronomers a rare chance to precisely measure the distance to an object on the other side of the Milky Way galaxy. X-ray: NASA/CXC/Univ. of Wisconsin-Madison/S.Heinz et al; Optical: DSS [Image]

Caption: This image from the Cassini mission shows three of Saturn's many moons all caught together in a crescent shape. The three moons are Titan, Mimas, and Rhea. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: A photo of an aurora as seen from the International Space Station on June 23. The photo was captured by NASA Astronaut Scott Kelly. NASA [Image]

Caption: Astronomers recently discovered that the giant elliptical galaxy Messier 87 has swallowed an entire medium-sized galaxy over the last billion years. European Southern Observatory [Image]

Caption: Astronomers recently discovered the brightest galaxy ever found in the early Universe. There is strong evidence that examples of the first generation of stars might be found inside. Artist's Impression, David Sobral [Image]

Caption: A cluster called Liller 1 where the stars are so densely packed that it might be one of the few places in our galaxy where astronomers think stars can collide. Gemini Observatory/AURA [Image]

Caption: A photo of the barred spiral galaxy NGC 1097 that has a central supermassive black hole (SMBH) with a mass 140 million times the mass of the Sun. ESO/R. Gendler [Image]

Caption: An image of Saturn's moon Dione, taken during a close flyby at an altitude of 321 miles from Dione's surface. Saturn's geysering moon Enceladus can be seen in the upper right corner as well. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: NASA’s Solar Dynamics Observatory photo of the sun. The image shows what’s left of two arrow-shaped solar filaments, dark features hovering above the sun’s surface by its magnetic field. Scientists still don’t know how or why they form. NASA/SDO [Image]

Caption: This is the galaxy UGC 11411, an irregular blue compact dwarf galaxy. It’s ten times smaller than a regular galaxy and made up of large groups of giant stars that are so hot they sometimes have a blue hue. ESA/Hubble & NASA [Image]

Caption: A composite image of the barred spiral galaxy NGC 1097 with a supermassive black hole at the galactic center that has a mass 140 million times greater than our Sun. In comparison, the black hole at the center of the Milky Way has a mass that is only a few million times greater than our Sun. ALMA (NRAO/ESO/NAOJ), K. Onishi; NASA/ESA Hubble Space Telescope, E. Sturdivant; NRAO/AUI/NSF [Image]

Caption: NGC 6503 is a spiral galaxy at the edge of the “Local Void,” a seemingly empty section of space nearly 150 million light-years across. ESO/Digitized Sky Survey 2 [Image]

Caption: A first-time look at a giant red star, L2 Puppis, giving birth to a planetary nebula. ESO/P. Kervella [Image]

Caption: A photo of the Crab Nebula, a remnant of a supernova explosion. Remains of the exploded star are still expanding about 1500 kilometres per second. ESO / Manu Mejias [Image]

Caption: Saturn’s moon Thethys which is covered by multiple impact craters. The crater Odysseus (pictured on the right) covers about 18 percent of the moon’s surface. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: A southern constellation surrounding L2 Puppis in the Milky Way. ESO/Digitized Sky Survey 2 [Image]

Caption: A composite of NGC 5813, a group of galaxies with a supermassive black hole in its center. The black hole has had multiple eruptions over the last 50 million years. X-ray: NASA/CXC/SAO/S.Randall et al., Optical: SDSS [Image]

Caption: A dwarf irregular galaxy PGC 1843 which is part of the space surrounding our galaxy known as the Local Volume. ESA/Hubble & NASA [Image]

Caption: NASA’s Mars Reconnaissance Orbiter captures photo of a “fresh” crater near the Sirenum Fossae region of Mars. NASA/JPL/University of Arizona [Image]

Caption: A photo of Saturn’s strange moon, Hyperion, captured by NASA’s Cassini spacecraft when it flew by on May 31, 2015. NASA/JPL-Caltech/Space Science Institute

Caption: An up close shot of the "oddball" Hyperion, Saturn's moon. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: Hubble sees a fascinating core. ESA/Hubble & NASA [Image]

Caption: NASA instrument on Rosetta makes comet atmosphere discovery. ESA/Rosetta/NAVCAM [Image]

Caption: NASA spacecraft views aftermath of Texas floods. NASA/GSFC/METI/ERSDAC/JAROS, and U.S./Japan ASTER Science Team [Image]

Caption: Mysterious lunar swirls on the moon may be caused by crashing comets. NASA/Lunar Reconnaissance Orbiter [Image] [Image]

Caption: The star forming cloud RCW 34. In the brightest region of this glowing nebula called RCW 34, gas is heated dramatically by young stars and expands through the surrounding cooler gas. Once the heated hydrogen reaches the borders of the gas cloud, it bursts outwards into the vacuum like the contents of an uncorked champagne bottle — this process is referred to as champagne flow. But the young star-forming region RCW 34 has more to offer than a few bubbles; there seem to have been multiple episodes of star formation within the same cloud. ESO [Image]

Caption: Large Hubble survey confirms link between mergers and supermassive black holes with relativistic jets. In the most extensive survey of its kind ever conducted, a team of scientists have found an unambiguous link between the presence of supermassive black holes that power high-speed, radio-signal-emitting jets and the merger history of their host galaxies. Almost all of the galaxies hosting these jets were found to be merging with another galaxy, or to have done so recently. The results lend significant weight to the case for jets being the result of merging black holes and will be presented in the Astrophysical Journal. Artist's Illustration: ESA/Hubble, L. Calçada (ESO) [Image]

Caption: Rhea's Horizon. The surface of Rhea (949 miles or 1527 kilometers across) has been sculpted largely by impact cratering, each crater a reminder of a collision sometime in the moon's history. On more geologically active worlds like Earth, the craters would be erased by erosion, volcanoes or tectonics. But on quieter worlds like Rhea, the craters remain until they are disrupted or covered up by the ejecta of a subsequent impact. NASA/JPL-Caltech/Space Science Institute [Image]

Caption: This new NASA/ESA Hubble Space Telescope image presents the Arches Cluster, the densest known star cluster in the Milky Way. It is located about 25 000 light-years from Earth in the constellation of Sagittarius (The Archer), close to the heart of our galaxy, the Milky Way. It is, like its neighbour the Quintuplet Cluster, a fairly young astronomical object at between two and four million years old. The Arches cluster is so dense that in a region with a radius equal to the distance between the Sun and its nearest star there would be over 100 000 stars! NASA & ESA [Image]

Caption: A fish-eye view of the VLT. A ring of air glow encompasses the VLT in this fish-eye shot, while the band of the Milky Way bisects the night sky. ESO/G. Brammer [Image]

Caption: Herschel’s View of G49 Filament. New images of huge filamentary structures of gas and dust from the Herschel space observatory reveal how matter is distributed across our Milky Way galaxy. Long and flimsy threads emerge from a twisted mix of material, taking on complex shapes. This image shows a filament called G49, which contains 80,000 suns' worth of mass. This huge but slender structure of gas and dust extends about 280 light-years in length, while its diameter is only about 5 light-years across. In this image, longer-wavelength light has been assigned visible colors. Light with wavelengths of 70 microns is blue; 160-micron light is green; and 350-micron light is red. Cooler gas and dust are seen in red and yellow, with temperatures as low as minus 421 degrees Fahrenheit (minus 252 degrees Celsius). ESA/Herschel/PACS/SPIRE/Ke Wang et al. 2015 [Image]

Caption: Dawn Spirals Closer to Ceres, Returns a New View. A new view of Ceres, taken by NASA's Dawn spacecraft on May 23, shows finer detail is becoming visible on the dwarf planet. The spacecraft snapped the image at a distance of 3,200 miles (5,100 kilometers) with a resolution of 1,600 feet (480 meters) per pixel. The image is part of a sequence taken for navigational purposes. NASA/JPL-Caltech/UCLA/MPS/DLR/IDA [Image]

Caption: ESO’s Very Large Telescope images of the Medusa Nebula. ESO [Image]

Caption: Wide-field view of the sky around the Medusa Nebula. ESO/Digitized Sky Survey 2 [Image]

Caption: Coronal Loops Over a Sunspot Group. NASA, SDO [Image]

Caption: Hubble Revisits Tangled NGC 6240. NASA, ESA, the Hubble Heritage [Image]

Caption: Hubble Observes One-of-a-Kind Star Nicknamed 'Nasty'. NASA, ESA, and J. Mauerhan [Image]

Caption: Rover's Reward for Climbing: Exposed Geological Contact. NASA/JPL-Caltech [Image]

Caption: Galaxy’s snacking habits revealed. Angel Lopez-Sanchez (AAO/MQU) and Baerbel Koribalski (CSIRO) [Image]

Caption: SGR 1745-2900: Magnetar Near Supermassive Black Hole. NASA/CXC/INAF/F.Coti Zelati et al [Image]

Caption: Hubble 47 Tucanae - UV. NASA, ESA, and H. Richer and J. Heyl (University of British Columbia, Vancouver, Canada) [Image]

Caption: SpaceX's Dragon cargo capsule docking to the Earth-facing port of the Harmony module. NASA [Image]

Caption: The giant elliptical galaxy Centaurus A (NGC 5128) and its strange globular clusters. ESO,ESA/Hubble, NASA. Digitized Sky Survey. Acknowledgement: Davide de Martin [Image]

Caption: Iridescent Nightscape over La Silla. ESO/Y. Beletsky [Image]

Caption: Hubble Spots the Layers of NGC 3923. ESA/Hubble & NASA [Image]

Caption: Discovery of Rare Quasar Quartet. HENNAWI & ARRIGONI-BATTAIA, MPIA [Image]


Original Submission

posted by martyb on Sunday July 26 2015, @07:10PM   Printer-friendly
from the BASIC:-But-Any-String-Is-Complicated! dept.

Carlos Shahbazi has presented the first two articles of a series that introduce the layman to the basics of String Theory.
link: http://mappingignorance.org/2015/05/06/the-geometry-of-string-theory-compactifications-i-the-basics/

"The sphere is also a simple example of a compact manifold, which is a particular class of manifolds of utmost importance in String Theory compactifications, as we will see in a moment. The compactness condition can be intuitively understood using Euclidean space. A manifold embedded in Euclidean space, as the sphere in figure 3, is compact if and only if it is bounded, namely it is contained in a finite size region of E and it is closed, namely it contains all its limiting points."

[The second article is "The geometry of String Theory compactifications (II): finding the Calabi-Yau manifold" -Ed.]

If that's too easy for you; the same author also has "Black hole solutions of N=2, d=4 super-gravity with a quantum correction, in the H-FGK formalism"
link: http://www.mathpubs.com/author/Carlos+S.+Shahbazi


Original Submission

posted by takyon on Sunday July 26 2015, @05:13PM   Printer-friendly
from the deep-dive dept.

The deep oceans span more than half the globe and their frigid depths have long been known to contain vast, untapped deposits of prized minerals. These treasures of the abyss, however, have always been out of reach to miners.

But now, the era of deep seabed mining appears to be dawning fueled by technological advances in robotics and dwindling land-based deposits. Rising demand for copper, cobalt, gold and the rare-earth elements vital in manufacturing smartphones and other high-tech products is causing a prospecting rush to the dark seafloor thousands of meters (yards) beneath the waves.

[...] A group of international scientists, in a [paywalled for some] July 9 article in the journal Science, urged [UN agency] ISA to temporarily halt authorization of new mining contracts until networks of "marine protected areas" are established around areas targeted for mining.

"We owe it to future generations to ensure that we think before we act and gain a thorough understanding of the potential impacts of mining in the deep sea before any mining is permitted," said Matthew Gianni, co-founder of the Deep Sea Conservation Coalition, which sent observers to ISA's 21st session in Kingston.

But despite the warnings, in recent days ISA authorized its latest exploration contract, a 72,745 square kilometer (28,087 sq. mile) permit in the Pacific to China Minmetals Corp., sponsored by Beijing. China now has the most permits from the U.N. body with four.

[...] "The terrestrial industrial revolution happened before we had the tools to manage goals for development and goals for sustaining biodiversity. You can't really blame people in the 1700s for the damage they did to the environment..." he said. "But we certainly are to blame if we don't do seabed mining properly."


Original Submission

posted by takyon on Sunday July 26 2015, @03:30PM   Printer-friendly
from the hard-mode-os dept.

A relatively new fork of FreeBSD, HardenedBSD, has completed its Address Space Layout Randomization (ASLR) feature. Without ASLR, applications are loaded into memory in a deterministic manner. An attacker who knows where a vulnerability lies in memory can reliably exploit that vulnerability to manipulate the application into doing the attacker's bidding. ASLR removes the determinism, making it so that even if an attacker knows that a vulnerability exists, he doesn't know where that vulnerability lies in memory. HardenedBSD's particular implementation of ASLR is the strongest form ever implemented in any of the BSDs.

The next step is to update documentation and submit updates to the patches they have already submitted upstream to FreeBSD. ASLR is the first step in a long list of exploit mitigation technologies HardenedBSD plans to implement.


Original Submission

posted by takyon on Sunday July 26 2015, @01:45PM   Printer-friendly
from the suit-up dept.

R&D teams within HP Enterprise Services received memos this week reminding them about the company's rules regarding workplace fashion. "If you aren't dressed like the models in the posters that HP displays around its locations, then your appearance is sapping the productivity of the workers around you," was one summary of the memo by an anonymous source. Many employees have become comfortable wearing t-shirts and shorts on a regular basis, and it is believed that "scruffy-looking" engineers might alienate visiting customers.


Original Submission

posted by takyon on Sunday July 26 2015, @11:55AM   Printer-friendly
from the pity dept.

Stumbled upon this blog entry:

One paragraph from the OP instantly stuck out to me.

I don't want to [be] a typical "code monkey". I want to go deep into low level, even to clear math when we talk about computer science, but at same time, I want to have a job in shorter period of time than let's say 3 years. I was switching so many times between Python, C++, Java and I'm nowhere. I know it's bad practise, it's worst, but I don't know, I'm just confused.

...

Web development has an extremely low barrier to entry in comparison to, say, systems programming. Setting up a Wordpress blog takes significantly less knowledge and effort than building an operating system.
As a consequence, being a web developer does not carry the same prestige as being a software engineer (whatever that is). God have mercy on your soul if HN or /r/programming learns you implemented some common functionality in NodeJS for fun. (Expect the words "web scale" to show up in the comment thread somewhere).
...
As I became more involved in online communities, the narrative became increasingly clear that my confidence and sense of accomplishment were unwarranted. PHP was a terrible language, and PHP developers were terrible programmers. JavaScript was a terrible language, and JS developers couldn't perform asymptotic analysis to save their life. Web developers don't have degrees and it shows in their code. Drupal/Wordpress developers are an absolute joke. Web developers never took a compilers course, so they don't understand just how easy their "jobs" are. Web developers are overpaid for how little they know. Web developers have everything handed to them. Web developers have never had to manage memory or make hard decisions. Web developers have no knowledge of data structures or algorithms. Web developers are not real programmers.

Armed with impulsive spending habits and a sense of urgency, I went to Amazon and purchased just about every programming book not related to web development I could find. Cryptographic protocol implementations in C, Embedded Systems development, Linux Kernel Development, etc. I wanted to learn things that real programmers knew. I wanted to learn the hard things. I bought an Arduino, started hanging out in ##c on freenode, began reading through implementations of the C standard library.
I never fully read any of those books. Most of them I never even started. I didn't do anything substantial with the arduino. I never made it passed analyzing "assert.h" in the C standard library (which I was planning on progressing through alphabetically.)
...
When you hate what you do, you stop caring about it. When you stop caring about something, you aren't going to bother learning more about it.
For a period of nearly 3 years, I was stuck in a terribly unproductive mental state. I hated web development, but I didn't know how to do anything else. Web development was all I knew. Bills needed to be paid, so CRUD apps needed to be made.

And thus arose my main cognitive dilemma: I hated web development because it was easy, but it was never actually easy to me. Instead of concluding "maybe web development is actually hard and those people don't know what they're talking about", I concluded that I must be a terrible programmer.

Question to SN fellows: have you had moments like this (doesn't matter if in relation with Web development or not)? Have you crossed over them? If true, how?


Original Submission

posted by takyon on Sunday July 26 2015, @10:00AM   Printer-friendly
from the information-desert-that-is-mainstream-media dept.

AlterNet reports:

MSNBC announced on Thursday that "The Ed Schultz Show" would come to an end, to be replaced by a show hosted by political analyst Chuck Todd.

[...] The loss of Schultz is particularly troubling because he has managed a television program that has been more attentive to issues focused on economic inequality, labor unions, and the wider economy than perhaps any other cable television show.

In particular, he covered the Trans-Pacific Partnership more often than [all other cable programs combined], as Craig Harrington and Brian Powell, researchers with Media Matters documented:

[During an 18 month period] CNN and Fox News each mentioned the TPP during two broadcasts. MSNBC's The Ed Show discussed the trade agreement on 71 broadcasts, but the TPP was mentioned on the network's other evening programming only twice (once by host Ed Schultz during coverage of the president's State of the Union speech and a passing mention by All In host Chris Hayes).

On The Jimmy Dore Show (think: Mort Sahl or Jon Stewart) via my Pacifica Radio affiliate, Chuck Todd is mentioned often. My impression is more "political hack" than "political analyst".


Original Submission

posted by janrinok on Sunday July 26 2015, @08:02AM   Printer-friendly
from the RIP dept.

You might be surprised to find out that kuro5hin -- k5 -- is still around. Well, not for much longer. Absentee landlord Rusty Foster (temporarily?) blocked new user sign ups and in the process somehow managed to block existing users from logging in.

Dedicated users can edit the HTML to add back the login box (or use a query string). Though once popular, K5 never recovered from the last time Rusty blocked new users (eventually relenting and adding a $5 sign up fee). RIP. Truly a Web 1.0 icon.

[If you have further information regarding this story, or can confirm/disprove the claims, please let the Eds know by a simple submission or via IRC.]


Original Submission

posted by janrinok on Sunday July 26 2015, @06:01AM   Printer-friendly

Instead of thinking of Jupiter as totally inhospitable, let's take a page from this Venus playbook, and aim for exploration of the atmosphere instead, with a robot that floats in the clouds and harvests energy from the wind.

WindBots, or "persistent in-situ science explorers for gas giants," is a conceptual project that just got a US $100,000 grant from NASA's Innovative Advanced Concepts program to make itself slightly less conceptual. The general idea is to find a way to make atmospheric exploration possible for gas giants, where keeping a robot alive for any appreciable amount of time is a challenge.
...
The robot itself is still just as conceptual as the image above would suggest, but the notable feature ... are the rotors on the faces of the robot that can spin to create lift or change the robot's direction. Inside, besides a bunch of fancy science instruments, there'd likely be some mechanism to harvest energy from turbulent motion, kind of like what you can find in one of those self-winding wristwatches.

It's the only way to know if we can join the Space Tyrant.


Original Submission

posted by janrinok on Sunday July 26 2015, @03:52AM   Printer-friendly
from the as-different-as-hot-and-dark dept.

Electrochromic glass essentially uses electric charge to switch a window from allowing sunlight into blocking it out. Some have estimated that such "smart windows" could cut lighting needs by about 20 percent and the cooling load by 25 percent at peak times.

Now researchers at the University of Texas Austin have found a way to make them even better. They developed a novel nanostructure architectcure for electrochromic materials that enables a highly selective cool mode and warm mode—something thought to be impossible a few years back.

In research published in the journal Nano Letters, the University of Texas researchers along with scientists at Lawrence Berkeley National Laboratory were able to get nanostructured electrochromic materials to control 90 percent of the near-infrared (NIR) light and 80 percent of the visible light. What's more, it only requires a few minutes to switch between these two modes, whereas previously reported materials took hours to make this transition.

This would make a huge difference for energy efficiency everywhere, since windows are the Achilles' heel of a structure's insulation.


Original Submission

posted by janrinok on Sunday July 26 2015, @01:48AM   Printer-friendly
from the down-memory-lane dept.

.... on July 23, 1985 technology genuinely changed forever. At New York's Lincoln Center, as a full orchestra scored the evening and all its employees appeared in tuxedos, Commodore unveiled the work of its newly acquired Amiga subsidiary for the first time. The world finally saw a real Amiga 1000 and all its features. A baboon's face at 640x400 resolution felt life-changing, and icons like Blondie's Debbie Harry and Andy Warhol came onstage to demo state-of-the-art technology like a paint program.

Today, Amiga—specifically its initial Amiga 1000 computer—officially turns 30. The Computer History Museum (CHM) in Mountain View, CA will commemorate the event this weekend (July 25 and 26) with firsthand hardware exhibits, speakers, and a banquet where the Viva Amiga documentary will be shown. It's merely the most high-profile event among dozens of Amiga commemorative ceremonies across the world, from Australia to Germany to Cleveland.

What's the big deal? While things like the Apple II and TRS-80 Model 100 preceded it, the Amiga 1000 was the first true PC for creatives. As the CHM describes it, the Amiga 1000 was "a radical multimedia machine from a group of thinkers, tinkerers, and visionaries which delivered affordable graphics, animation, music, and multitasking interaction the personal computer world hadn't even dreamt of." It pioneered desktop video and introduced PCs to countless new users, rocketing Amiga and Commodore to the top for a brief moment in the sun.

Amiga fans, assemble!


Original Submission

posted by janrinok on Saturday July 25 2015, @11:54PM   Printer-friendly
from the the-times-they-are-a-changin' dept.

Richard Stallman, the founder of the Free Software Foundation and the GNU Project known by many in the open source worlds as rms, is not the sort of person you'd expect to endorse a product. But Stallman and the FSF have formed a partnership of sorts with Crowd Supply, a crowdfunding company that has been largely focused on open source hardware and software projects.

Crowd Supply is best known for launching the Librem laptop (a privacy-focused computer built by Purism) and the Novena (an open-hardware "laptop" designed by Andrew "bunnie" Huang and Sean "xobs" Cross). Based in Portland, Oregon, the company was founded by Joshua Lifton, a Ph D alumnus of MIT Media Lab and the former head of engineering at Puppet Labs. In addition to providing product designers with a crowdfunding platform, Crowd Supply also provides them with long-term sales, marketing, and fulfillment services.

The partnership with FSF was a natural fit, Lifton said in a statement on the arrangement. "The lines between hardware and software are blurring," Lifton explained. "It only makes sense to consider them jointly rather than separately."

Is this RMS's version of selling-out?