Showing posts with label factory. Show all posts
Showing posts with label factory. Show all posts

Thursday, 20 October 2011

Inside the Factory: How a Chef's Knife Is Made

PopSci goes to Germany to witness the cutting edge of manufacturing
Knives Await Grinding Paul Adams

Last week, I visited Solingen, Germany's "city of blades," where knives, swords, and the like have been made for centuries. In between sipping beers and munching wursts, I paid a visit to the factory of Zwilling J.A. Henckels, at their kind invitation, to peer at the semi-roboticized lines where they produce their knives.

The raw material comes into the factory on huge spools of sheet steel, each sheet the thickness of a knife. The steel is cut into individual blanks, destined to become individual knives. About three weeks elapse between when a blank comes off the spool and when it emerges, a finished knife, at the other end.

In my breathless tour of the factory, I watched as a giant press cut and stacked the blanks, which are made of the company's secret blend of stainless "special formula steel." The blank is transported to another building, where the first of the factory's 90-odd industrial robot arms takes it in hand.

In the classic design, the knife has a thickening where the blade meets the handle (aka the bolster). This is formed first, by heating the middle of the blank, and then pressing the metal's two ends together so the molten middle bulges and widens, in a process that my contact specifies is called upset forging. Next, a drop forge shapes the bolster, before the blank is quickly cropped into the rough shape of the knife it's going to be.

After that, it proceeds through a series of cooling, supercooling, and heat-tempering steps that give it its corrosion resistance and toughness. This is one of the benefits of the special steel, I'm told -- it heats and cools in very predictable ways, allowing the factory to use more precise temperatures rather than temperature ranges.

After the tempering, any distortions or warpings that the heat has created in the blade are hammered out by a highly skilled human, who picks up and eyes each knife, one at a time, and flattens any that need flattening with precise strokes of a little hammer.

The knife passes into the hands of another series of robots, which use grinding wheels to narrow down the thickish blank into the tapered contour of a blade. Only roughly, though -- the fine grinding and sharpening, as well as putting on the handles, is left to the factory's humans, who wear puffy gray overalls and exude the confidence that comes with being extremely good at your job, and quite possibly coming from a line of knifemakers generations old. Wooden handles are glued onto the tang of the knife and then riveted in place; plastic handles are simply melted on by heating the tang and inserting it in a ready handle. The edges of the handles are smoothed by robots.

Finally the knife is cleaned and passes onward to the scrutiny of the quality assurance women. If it has no flaws -- there's a big photo-book of possible flaws -- it gets packed up and winds up in someone's kitchen.

Check out the step-by-step gallery of pictures from the knifemaking process.


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Wednesday, 19 October 2011

Gallery: Inside a Knife Factory


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Astronomers reveal supernova factory

ScienceDaily (Oct. 2, 2011) — A team led by astronomers at Chalmers and Onsala Space Observatory has detected seven previously unknown supernovae in a galaxy 250 million light years away. Never before have so many supernovae been discovered at the same time in the same galaxy. The discovery proves what astronomers have long believed: that the galaxies which are the universe's most efficient star-factories are also supernova factories.

The astronomers used a worldwide network of radio telescopes in five countries, including Sweden, to be able to create extremely sharp images of the galaxy Arp 220. The scientists observed around 40 radio sources in the center of the galaxy Arp 220. These radio sources are hidden behind thick layers of dust and gas and invisible in ordinary telescopes. To discover the nature of these radio sources, they made measurements at different radio wavelengths and watched how they changed over several years.

"With all the data in place, we can now be certain that all seven of these sources are supernovae: stars that exploded in the last 60 years," says Fabien Batejat, main author of the article about the discovery.

So many supernovae have never before been detected in the same galaxy. The number is nevertheless consistent with how fast stars are forming in Arp 220.

"In Arp 220, we see far more supernovae than in our galaxy. We estimate that a star explodes in Arp 220 once every quarter. In the Milky Way, there is only one supernova per century," says Rodrigo Parra, astronomer at the European Southern Observatory in Chile and member of the team.

John Conway is professor of observational radio astronomy at Chalmers and deputy director of Onsala Space Observatory.

"Arp 220 is well-known as a place where star formation is very efficient. Now we have been able to show that star factories like this are also supernova factories," he says.

The radio measurements have also given researchers insight into how radio waves are generated in supernovae and their remnants.

"Our measurements show that a supernova's own magnetic field is what gives rise to its radio emission, not the magnetic fields in the galaxy around it," says Fabien Batejat.

The results will be published in the October 20 issue of the journal Astrophysical Journal.

The team is composed of Fabien Batejat, John Conway and Rossa Hurley from Onsala Space Observatory at Chalmers, Rodrigo Parra (European Southern Observatory, ESO, Santiago, Chile), Philip Diamond (CSIRO, Sydney, Australia), Colin J. Lonsdale (MIT Haystack Observatory, USA) and Carol J. Lonsdale (North American Alma Science Center, NRAO, Charlottesville, USA).

The observations were carried out using telescopes which belong to the European VLBI Network (EVN) together with the Very Long Baseline Array (VLBA). The VLBA is a set of ten radio telescopes located from Hawaii to St. Croix in the U.S. Virgin Islands and operated by the National Radio Astronomy Observatory.

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The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by Chalmers University of Technology.

Journal Reference:

Fabien Batejat, John E. Conway, Rossa Hurley, Rodrigo Parra, Philip J. Diamond, Colin J. Lonsdale, Carol J. Lonsdale. Resolution of the Compact Radio Continuum Sources in Arp220. Astrophysical Journal, 2011; (in press) [link]

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


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Tuesday, 11 October 2011

Astronomers reveal supernova factory

ScienceDaily (Oct. 2, 2011) — A team led by astronomers at Chalmers and Onsala Space Observatory has detected seven previously unknown supernovae in a galaxy 250 million light years away. Never before have so many supernovae been discovered at the same time in the same galaxy. The discovery proves what astronomers have long believed: that the galaxies which are the universe's most efficient star-factories are also supernova factories.

The astronomers used a worldwide network of radio telescopes in five countries, including Sweden, to be able to create extremely sharp images of the galaxy Arp 220. The scientists observed around 40 radio sources in the center of the galaxy Arp 220. These radio sources are hidden behind thick layers of dust and gas and invisible in ordinary telescopes. To discover the nature of these radio sources, they made measurements at different radio wavelengths and watched how they changed over several years.

"With all the data in place, we can now be certain that all seven of these sources are supernovae: stars that exploded in the last 60 years," says Fabien Batejat, main author of the article about the discovery.

So many supernovae have never before been detected in the same galaxy. The number is nevertheless consistent with how fast stars are forming in Arp 220.

"In Arp 220, we see far more supernovae than in our galaxy. We estimate that a star explodes in Arp 220 once every quarter. In the Milky Way, there is only one supernova per century," says Rodrigo Parra, astronomer at the European Southern Observatory in Chile and member of the team.

John Conway is professor of observational radio astronomy at Chalmers and deputy director of Onsala Space Observatory.

"Arp 220 is well-known as a place where star formation is very efficient. Now we have been able to show that star factories like this are also supernova factories," he says.

The radio measurements have also given researchers insight into how radio waves are generated in supernovae and their remnants.

"Our measurements show that a supernova's own magnetic field is what gives rise to its radio emission, not the magnetic fields in the galaxy around it," says Fabien Batejat.

The results will be published in the October 20 issue of the journal Astrophysical Journal.

The team is composed of Fabien Batejat, John Conway and Rossa Hurley from Onsala Space Observatory at Chalmers, Rodrigo Parra (European Southern Observatory, ESO, Santiago, Chile), Philip Diamond (CSIRO, Sydney, Australia), Colin J. Lonsdale (MIT Haystack Observatory, USA) and Carol J. Lonsdale (North American Alma Science Center, NRAO, Charlottesville, USA).

The observations were carried out using telescopes which belong to the European VLBI Network (EVN) together with the Very Long Baseline Array (VLBA). The VLBA is a set of ten radio telescopes located from Hawaii to St. Croix in the U.S. Virgin Islands and operated by the National Radio Astronomy Observatory.

Recommend this story on Facebook, Twitter,
and Google +1:

Other bookmarking and sharing tools:

Story Source:

The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by Chalmers University of Technology.

Journal Reference:

Fabien Batejat, John E. Conway, Rossa Hurley, Rodrigo Parra, Philip J. Diamond, Colin J. Lonsdale, Carol J. Lonsdale. Resolution of the Compact Radio Continuum Sources in Arp220. Astrophysical Journal, 2011; (in press) [link]

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


View the original article here