Showing posts with label 3D images. Show all posts
Showing posts with label 3D images. Show all posts

Tuesday, January 22, 2013

Oppressive China Opens Public 3D Printing Booth

While 3D printing may be touted as bringing manufacturing back to the United States, that doesn't mean the rest of the world hasn't taken notice of the technology.

Earlier this week, a 3D Printing Experience Pavilion opened in Beijing's DRC Industrial Design and Cultural Industry Base, where visitors were able to see how 3D printers work firsthand.

With a few hours to spare, they could even have their own head scanned and printed as a bust, which follows the 3D printing booth that opened in a Japanese mall last year.

Among the printed objects on display were custom phone cases, miniatures (including Aldebaran Robotics' NAO, which featured prominently at the Shanghai World Expo), and jewelry.

Visitors who wanted to be scanned had to remain still for around 15 minutes for the process to be completed, whereupon their likeness was printed in single color ABS plastic – a process which takes between two to three hours. 3Ders reports that the 3D Printing Pavilion was spear-headed by Beijing company Suntop-Tech, which is the Chinese distributor of Stratasys' Fortus and Dimension 3D printers.

Friday, August 10, 2012

NASA Mars Rover Curiosity: NavCam's 3D Images

This picture is the first full-resolution 3D image from the navigational cameras on NASA's Curiosity Mars rover, taken shortly after the robot had lifted up its mast on sol 2 of its 98-week mission (a sol is a Martian solar day, which lasts for 24 hours, 39 minutes, and 35.244 seconds).

The view shows a pebble-strewn surface with the mountainous rim of Gale crater rising in the distance.

To create the eye-popping shot, NASA combined newly received data from the rover's twin navcams, which sit on the remote-sensing mast's WALL-E-like head.

These cameras act like left and right eyes for capturing stereo views of the Martian landscape (see images below).



The navcams can see out to 100 metres and will be used not only to plan the rover's path forward but also for deciding where to aim the MastCam and ChemCam.

MastCam can take colour pictures, video and stitched panoramas, while ChemCam will fire a laser from up to 7 metres away to vaporise rocks and analyse their composition via spectroscopy.

Once the team completes calibrating the cameras, they'll instruct the navcams to take a 360-degree panorama, helping rover drivers get a good hard look at the landing site before driving off toward their main science target, the intriguing mountain inside Gale named Mount Sharp.

Tuesday, April 24, 2012

Computing the best high-resolution 3-D tissue images

Real-time, 3-D microscopic tissue imaging could be a revolution for medical fields such as cancer diagnosis, minimally invasive surgery and ophthalmology.

University of Illinois researchers have developed a technique to computationally correct for aberrations in optical tomography, bringing the future of medical imaging into focus.

The computational technique could provide faster, less expensive and higher resolution tissue imaging to a broader population of users. The group describes its technique this week in the online early edition of the Proceedings of the National Academy of Sciences.

“Computational techniques allow you to go beyond what the optical system can do alone, to ultimately get the best quality images and three-dimensional datasets,” said Steven Adie, a postdoctoral researcher at the Beckman Institute for Advanced Science and Technology at Illinois. “This would be very useful for real-time imaging applications such as image-guided surgery.” 

Aberrations, such as astigmatism or distortion, plague high-resolution imaging. They make objects that should look like fine points appear to be blobs or streaks. The higher the resolution, the worse the problem becomes. It’s especially tricky in tissue imaging, when precision is vital to a correct diagnosis.

Adaptive optics can correct aberrations in imaging. It’s widely used in astronomy to correct for distortion as starlight filters through the atmosphere. A complex system of mirrors smooth out the scattered light before it enters the lens. Medical scientists have begun applying adaptive optics hardware to microscopes, hoping to improve cell and tissue imaging.

“It’s the same challenge, but instead of imaging through the atmosphere, we’re imaging through tissue, and instead of imaging a star, we’re imaging a cell,” said Stephen Boppart, a professor of electrical and computer engineering, of bioengineering and of internal medicine at the U. of I. “But a lot of the optical problems are the same.”

Unfortunately, hardware-based adaptive optics are complicated, tedious to align and extremely expensive. They can only focus on one focal plane at a time, so for tomography – 3-D models constructed from sectional images as in a CT scan, for example – the mirrors have to be adjusted and a new image scanned for each focal plane. In addition, complex corrective systems are impractical for handheld or portable devices, such as surgical probes or retinal scanners.

Therefore, instead of using hardware to correct a light profile before it enters the lens, the Illinois team uses computer software to find and correct aberrations after the image is taken.

Boppart's group teamed up with with Scott Carney, a professor of electrical and computer engineering and the head of the Optical Science Group at the Beckman Institute, to develop the technique, called computational adaptive optics.

They demonstrated the technique in gel-based phantoms laced with microparticles as well as in rat lung tissue. They scan a tissue sample with an interferometric microscope, which is an optical imaging device using two beams of light.

The computer collects all of the data and then corrects the images at all depths within the volume. Blurry streaks become sharp points, features emerge from noise, and users can change parameters with the click of a mouse.

“Being able to correct aberrations of the entire volume helps us to get a high-resolution image anywhere in that volume,” said Adie. “Now you can see tissue structures that previously were not very clear at all.”

Computed adaptive optics can be applied to any type of interferometric imaging, such as optical coherence tomography, and the computations can be performed on an ordinary desktop computer, making it accessible for many hospitals and clinics.

Next, the researchers are working to refine the algorithms and explore applications. They are combining their computational adaptive optics with graphics processors, looking forward to real-time in-vivo applications for surgery, minimally invasive biopsy and more.  

Wednesday, March 14, 2012

NASA Chandra: Astronomers map dark matter distribution in 3D in Abell 383 galaxy cluster

The dark matter in Abell 383 is stretched out like a gigantic football with the point of the football is aligned close to the line of sight.

The X-ray data (purple) from Chandra in the composite image show the hot gas, which is by far the dominant type of normal matter in the cluster.

Galaxies are shown with the optical data from the Hubble, the ESO's Very Large Telescope (VLT), and the Sloan Digital Sky Survey, coloured in blue and white.

Credit: X-ray: NASA/CXC/Caltech/A.Newman et al/Tel Aviv/A.Morandi & M.Limousin; Optical: NASA/STScI, ESO/VLT, SDSS

Two teams of astronomers have used data from NASA's Chandra X-ray Observatory and other telescopes to map the distribution of dark matter in a galaxy cluster known as Abell 383, which is located about 2.3 billion light years from Earth.

Not only were the researchers able to find where the dark matter lies in the two dimensions across the sky, they were also able to determine how the dark matter is distributed along the line of sight.

Dark matter is invisible material that does not emit or absorb any type of light, but is detectable through its gravitational effects.

Several lines of evidence indicate that there is about six times as much dark matter as "normal", or baryonic, matter in the Universe.

Understanding the nature of this mysterious matter is one of the outstanding problems in astrophysics.

Galaxy clusters are the largest gravitationally-bound structures in the universe, and play an important role in research on dark matter and cosmology, the study of the structure and evolution of the universe.

The use of clusters as dark matter and cosmological probes hinges on scientists' ability to use objects such as Abell 383 to accurately determine the three-dimensional structures and masses of clusters.

The recent work on Abell 383 provides one of the most detailed 3-D pictures yet taken of dark matter in a galaxy cluster.


Both teams combined the X-ray observations of the "normal matter" in the cluster with gravitational lensing information determined from optical data.

Gravitational lensing, an effect predicted by Albert Einstein, causes the material in the galaxy cluster, both normal and dark matter, to bend and distort the optical light from background galaxies.

The distortion is severe in some parts of the image, producing an arc-like appearance for some of the galaxies.

In other parts of the image the distortion is subtle and statistical analysis is used to study the distortion effects and probe the dark matter.

Friday, January 6, 2012

The New Gamers Immersive Dome Display Unit - The TOOB! - Video



WHAT IS THE PLAN?
TOOB plans to manufacture and sell the world’s first affordable dome displays. TOOB has spent the last 2 years developing its 2nd generation product TOOB Earth.

WHAT IS TOOB Earth?
TOOB Earth is a 1.2 Metre (4ft) diameter half dome which when used with a standard projector fitted with a standard lens can project an image onto the inside curved surface giving the viewer the sense of being fully immersed in the content.Think IMAX/ OMNI MAX but in the home.


One of the key differentiator's is that the projector and screen are all contained within the same footprint meaning you no longer need to compromise on space.

TOOB Earth is the first in a range of dome products planned and will be the foundation for the world’s first consumer focused Gaming/ Simulation/ Film curved screen company.

Its uniquely patented design allows you to place your dome on any hard surface or on our GRAVITY-E adjustable stand.
Using the GRAVITY-E stand adds a further layer of flexibility as it then allows you to either use TOOBs brand new TSR/ TFX & M-spec simulation rigs
or use many existing racing or flight rigs which can be comfortably slide underneath. Or simply use the GRAVITY-E as a furniture piece in your room for watching stereo 3D movies.

CORPORATE
TOOB is well suited for the corporate environment and this is a great opportunity to get a TOOB and be one of the first to showcase TOOB Dome technology with your business.

TOOB's 007 reward shows how you can take a TOOB product and customise it with a unique brand or design.

In April 2011 TOOB attended the Gadget Show Live in Birmingham (UK) visted by over 40,000 tech hungry guests.

TOOB was so popular it increased footfall on our partners stand by thousands. The increased footfall generated more sales.

TOOB gave 1400 demos during the event. That guarenteed 1400 more potential customers + the 1000s of people that stoped to look at the technology.
(T.O.O.B. LTD acknowledges all rights, copyrights and trademarks of 3rd parties, the above image is an artists illustration only)


Monday, September 19, 2011

DLR Vesta: an asteroid full of surprises

South pole centred colour coded digital terrain model of the 'basin'
The latest 3D images, which show the whole asteroid, make something very clear – Vesta holds quite a number of challenges for the scientists on the Dawn team.

"For example, we can see a very large impact crater in the south polar region, the likes of which we have never seen before," emphasises Jaumann.

The shape and structure of the crater differ from every other impact crater in the Solar System.

"We are unable to find similar craters on other bodies, and cannot yet explain exactly what has caused it."

Another critical question faced by the planetary scientists is whether or not there has been volcanism on Vesta.

The numerous impact craters are not making this easy for scientists. "Any evidence of volcanic activity has been covered by impact ejecta and our current challenge is to find traces of volcanic deposits," explains Jaumann.

Dark material associated with craters that appears in some of the 3D images might provide the scientists with information on potential volcanic activity. But it could also be the remnants of the impacting body, in which case, the search for signs of volcanism must continue.

More information on Vesta at DLR Portal - Vesta - an asteroid full of surprises

Monday, July 5, 2010

ESA PLANCK FSM Image

PLANCK_FSM_03 Image

http://www.esa.int/images/PLANCK_FSM_03_Black.jpg

The microwave sky as seen by ESA's Plancksatellite

This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz.

The mottled structure of the CMBR, with its tiny temperature fluctuations reflecting the primordial density variations from which today’s cosmic structure originated, is clearly visible in the high-latitude regions of the map.

The central band is the plane of our Galaxy. A large portion of the image is dominated by the diffuse emission from its gas and dust. The image was derived from data collected by Planck during its first all-sky survey and comes from observations taken between August 2009 and June 2010. This image is a low- resolution version of the full data set.

To the right of the main image, below the plane of the Galaxy, is a large cloud of gas in our Galaxy. The obvious arc of light surrounding it is Barnard’s Loop – the expanding bubble of an exploded star. Planck has seen whole other galaxies.

The great spiral galaxy in Andromeda, 2.2 million light-years from Earth, appears as a sliver of microwave light, released by the coldest dust in its giant body. Other, more distant, galaxies with supermassive black holes appear as single points of microwaves dotting the image.

Planck was built for ESA by the Prime Contractor Thales Alenia Space (Cannes, France) with contributions from space industry drawn from ESA’s 18 Member States. Because of differing accounting procedures in the many bodies contributing, precise costings are impossible to give.

However, the overall cost to ESA and its Member State institutions as well as cooperating agencies world- wide (including NASA and Canadian Space Agency) in round figures is 600M€

Credits: ESA/ LFI & HFI Consortia

Saturday, June 26, 2010

German TanDEM-X satellite returns first 3D images

BBC News - German TanDEM-X satellite returns first images

Germany's new radar satellite, TanDEM-X, has returned its first images.

The spacecraft was launched from Kazakhstan on Monday on a mission to make the most precise 3D map of the Earth's surface.

The pictures demonstrate the platform is in excellent health and ready to team up with the TerraSAR-X satellite launched in 2007.

Together, the pair will trace the variation in height across the globe to a precision of better than two metres.

This digital elevation model (DEM) will support a multitude of applications, such as the programming of navigation computers in military jets to enable them to fly ultra low. The data will also be given to relief workers to show them where an earthquake has wrought most damage in a city.

Infoterra GmbH, the company with exclusive rights to commercialize the TanDEM information, says the market for radar products is steadily growing.

The new images depict a landscape in Ukraine, the north of Madagascar, and Moscow.

The pictures illustrate neatly the particular specialism of using radar to sense the planet's surface.

In the Madagascan data, for example, the choppiness of the waves in the open stretches of the Indian Ocean can be contrasted with the smooth reflection of the radar signal from the enclosed, clam waters of the Baie de Diego.

And in the image of Moscow-Sheremetyevo airport, the flat concrete surfaces of the runways appear as black lines because the radar beam has been very efficiently reflected away from the satellite.