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The Ars Electronica Futurelab made a high-profile guest appearance in Los Angeles. As part of the Walt Disney Concert Hall’s IN/SIGHT series, Esa Pekka Salonen conducted the L.A. Philharmonic Orchestra in a performance of Ravel’s “Mother Goose” that featured impressive visualizations designed by the Linz-based media art lab.
Credit: Ars Electronica Futurelab
This is a visualization of a blog community. It's one of the end results of our project. In the visualization, thicker lines suggest a stronger connection between the two blogs. If you want to know more, or play with it, hop over to www.blogslikethis.com/
Hydrogen accounts for about 74 percent of the normal matter in the Universe. This visualization shows the electron clouds of hydrogen through the probability density function when the principal quantum number, N, is 1 and 2. The probability density illustrates where the electron is most likely to be found if measured, red indicates high probability, blue indicates low probability.
Update: 2020/06/22: A 16k version is now available.
Update: 2020/07/06: A visualization showing all electron orbitals for N=1 to 6 is also available on Youtube: youtu.be/HyRHT4yOvms
An interactive web visualization I have been working on in processing. Part of the script is modified from an older project which builds an interactive map of Wikipedia , that project is at wikiweb.anthonymattox.com/ and is great fun.
My goal now is to create a better version of that and make it more flexible to do a few things, mapping out any individual website and building an interactive map include the whole web.
I'm also using the my new improved particle system which you can see some examples of in my blog at www.anthonymattox.com/blog, although the link class need a little work.
This visualization shows the wave functions of hydrogen when the principal quantum number, N, is between 1 and 2. The wave function is the solution of the Schrödinger equation and describes the electron in its wave form. Yellow and red colors show positive, while blue and purple denote negative values. Its complex square is the probability density, which actually shows where the electron might be found in the atom when measured.
That visualization can be found here: www.flickr.com/photos/188522613@N05/49924325132/in/datepo...
Update: 2020/06/22: A 16k version is now available.
Created by Martin Wattenberg with Marek Walczak (who licenses it under this CC license), Thinking Machine 4 explores the invisible, elusive nature of thought. Play chess against a transparent intelligence, its evolving thought process visible on the board before you.
The artwork is an artificial intelligence program, ready to play chess with the viewer. If the viewer confronts the program, the computer's thought process is sketched on screen as it plays. A map is created from the traces of literally thousands of possible futures as the program tries to decide its best move. Those traces become a key to the invisible lines of force in the game as well as a window into the spirit of a thinking machine.
The average San Francisco prices go beyond the $700k limit. But even so, housing is way cheaper in Baltimore.
Sources:
sent to my group www.flickr.com/groups/abc-visualized for the letter A:
1. Port Lockroy and the Europa., 2. A, 3. Looking Back..., 4. Landing
Money plays a central role to life in EVE. What does 200B ISK in damage actually look like? When I lose a Battleship, how much is that setting me back? How many Logistics ships could you buy instead of one Dreadnaught?
More details on how I collected the data, and why, in my post on this visualization.
You'll need to zoom in on this to see the details.
This image is part my new blog about EVE Online that tries to explain and document the world, with a focus on making it accessible for non-players and new players.
Ascent Penthouse
Client: Mr Dung - IAM Architecture
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@ Long Nguyen & Thu Nguyen
Architecture - Interior Design & 3D Visualization
0979 962 864, Ho Chi Minh City
advlongnguyen@gmail.com
Edited Chandra Space Telescope visualization of the center of the Milky Way Galaxy. Round variant.
Original caption: Want to take a trip to the center of the Milky Way? Check out a new immersive, ultra-high-definition visualization. This 360-movie offers an unparalleled opportunity to look around the center of the galaxy, from the vantage point of the central supermassive black hole, in any direction the user chooses.
By combining NASA Ames supercomputer simulations with data from NASA's Chandra X-ray Observatory, this visualization provides a new perspective of what is happening in and around the center of the Milky Way. It shows the effects of dozens of massive stellar giants with fierce winds blowing off their surfaces in the region a few light years away from the supermassive black hole known as Sagittarius A* (Sgr A* for short).
These winds provide a buffet of material for the supermassive black hole to potentially feed upon. As in a previous visualization, the viewer can observe dense clumps of material streaming toward Sgr A*. These clumps formed when winds from the massive stars near Sgr A* collide. Along with watching the motion of these clumps, viewers can watch as relatively low-density gas falls toward Sgr A*. In this new visualization, the blue and cyan colors represent X-ray emission from hot gas, with temperatures of tens of millions of degrees; red shows moderately dense regions of cooler gas, with temperatures of tens of thousands of degrees; and yellow shows of the cooler gas with the highest densities.
A collection of X-ray-emitting gas is seen to move slowly when it is far away from Sgr A*, and then pick up speed and whip around the viewer as it comes inwards. Sometimes clumps of gas will collide with gas ejected by other stars, resulting in a flash of X-rays when the gas is heated up, and then it quickly cools down. Farther away from the viewer, the movie also shows collisions of fast stellar winds producing X-rays. These collisions are thought to provide the dominant source of hot gas that is seen by Chandra.
When an outburst occurs from gas very near the black hole, the ejected gas collides with material flowing away from the massive stars in winds, pushing this material backwards and causing it to glow in X-rays. When the outburst dies down the winds return to normal and the X-rays fade.
The 360-degree video of the Galactic Center is ideally viewed through virtual reality (VR) goggles, such as Samsung Gear VR or Google Cardboard. The video can also be viewed on smartphones using the YouTube app. Moving the phone around reveals a different portion of the movie, mimicking the effect in the VR goggles. Finally, most browsers on a computer also allow 360-degree videos to be shown on YouTube. To look around, either click and drag the video, or click the direction pad in the corner.
Dr. Christopher Russell of the Pontificia Universidad Católica de Chile (Pontifical Catholic University) presented the new visualization at the 17th meeting of the High-Energy Astrophysics (HEAD) of the American Astronomical Society held in Monterey, Calif. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.
Here's a quick and dirty attempt to automatically determine arterial streets without any prior knowledge about the arterial status of a street. The idea is: a shortest path tree is taken for a bunch of random points, and the trunkyness of each branch was determined. The trunkynesses of the roads are summed, and this is the resulting map. It sort of works.
June 18, 2013 - NREL Senior Scientists Ross Larsen and Travis Kemper examine a molecular model of Polymeric organic nitroxide radical (PTMA) film for battery applications using a 3D model at the Insight Collaboration Laboratory during a tour of the Energy Systems Integration Facility (ESIF) at the National Renewable Energy Laboratory (NREL) in Golden, Colorado. (Photo by Dennis Schroeder / NREL)
I'm playing with a new theme for my blog, and wanted a better way to let people quickly scan for how many posts I had. So I used a background image of black, offset with background-position in css to let a graph "show through" to show the count.
I've also posted the PHP and CSS code for WordPress to make this work: http://gist.github.com/304290
It looks better larger: http://www.flickr.com/photos/artlung/4356884087/sizes/o/
The Taj Mahal located in the white spot of a heatmap of compass data taken from public Flickr photos.
See the related Flickr Blog post.
visualization in-progress - this is a dataset of twitter messages taken from the #140conf that jeff pulver organized in Tel Aviv last December.
In its 2006 Gallery, the journal Nature chose an image that spatially lays out different areas of science in a plane. It is a reduction of a large-format (42" x 43") paper print.
The map was constructed by sorting roughly 800,000 scientific papers (shown as white dots) into 776 different scientific paradigms (red circular nodes) based on how often the papers were cited together by authors of other papers. Links (curved lines) were made between the paradigms that shared common members, then treated as rubber bands, holding similar paradigms nearer one another when a physical simulation had every paradigm repel every other: thus the layout derives directly from the data. Larger paradigms have more papers. Labels list common words unique to each paradigm.
This work was commissioned and partially supported by Katy Borner and the Places and Spaces: Mapping Science exhibition.
www.visualcomplexity.com/vc/project_details.cfm?id=421&am...
Mike Moradi, Founder and Chief Executive Officer, Sensulin, USA; Young Global Leader capture during the Session: "Visualizing Disease" at the World Economic Forum - Annual Meeting of the New Champions in Dalian, People's Republic of China 2017. Copyright by World Economic Forum / Sikarin Fon Thanachaiary
I made myself a goal to walk 3000 miles (4828 km) in 2014 (and my stretch goal is to cover 5000 km = 3106 miles). Getting behind happens one day at a time, as you can see in this graph, which plots how far behind (or ahead) I am each day.
As you can see, I was 161 miles behind on 6 June, which is day 157, so I the slope is about -1 mile per day. As summer has appeared in Seattle, I am catching up by averaging about 9 miles per day. I am hoping to boost that again when summer school is over and I can get in some long days of hiking.
I find this graph a pretty good motivator to get me to cover miles each day, I think it might be possible to get to 3000 miles (on other words, delta = 0 on 31 December.
Fit20140808Delta