View allAll Photos Tagged interactive
A helpfully annotated guide to various elements of the Passover seder. The photograph was taken during an excellent meal in Bristol.
At INTERACTIVE Pavilion we showcased a variety of the newest IT/technology related products from hardware and software to digital arts and sciences. People enjoyed experiencing and seeing the cutting-edge technology coming straight from Japan.
Photo by Alex Chan
interactive version of my former work. it's build with actionscript. you can play with it at blob.creanode.com/blob/eu2009/ if you want.
Mazda, a J-POP SUMMIT 2015 Presenting sponsor, showcased their all new CX-3 and MX-5! also, Kelvin Kazumi Hiraishi, a director of R&D Engineering from Mazda, had a special keynote session at Firehouse!
Photo by Kumi Yamauchi
CN Lulu Island Spur
Richmond, BC
Feb 8, 2013
Formerly an inactive spur, a new customer has moved into this warehouse and started receiving rail service to this spur again.
I humbly believe that the concept of "kidzania" is utterly brilliant. Engagement, interactivity and brand exposure at its best
A 3-D interactive tactile rendering of the painting, We Are Only Limited by Our Imagination by Gareth Hector, which depicts the Project AZORIAN operation. The tactile rendering allows visitors to experience the painting through touch.
The bunny slides down the hill! Lawn Fawn Joy to the Woods, Winter Bunny, Stitched Hillside Borders stamps&dies, twine. Simon Says Stamp Falling Snow stencil, fog cardstock. Copic markers. Wendy Vecchi embossing paste, Fancy Pants sequins.
The butterfly is adhered to the card with a little spiral so that it can wiggle.
Please visit my blog for more details : www.stampingmariette.blogspot.com
At INTERACTIVE Pavilion we showcased a variety of the newest IT/technology related products from hardware and software to digital arts and sciences. People enjoyed experiencing and seeing the cutting-edge technology coming straight from Japan.
Photo by Shuntaro Ogata
I love interactive kids books and this mechanism is one my son loves to do. Turn the circle and the greeting cycles through the window on the front of the card. It says "have a happy day from us"
HA happy day animals.
Street performers, from 'Paperwork Theatre', outside John Lewis Department Store, Liverpool ONE - Queen's Platinum Jubilee Weekend.
Paperwork Theatre create bold theatrical events, staged in traditional theatres, unusual places, and community owned spaces. Based in the North West of England, where they champion artistic excellence, working with established and emerging artists from across the UK.
Their work is delivered across 3 core strands - Theatre, Community & Artistic Opportunities.
N.B. Lady on 2nd left is not one of the cast and was enjoying the interactive experience.
The tri-fold card open....
(A card for the interactive challenge on Hero Arts blog. I copied the tri-fold from a store bought card my husband gave me for my birthday last week. I used my new background stamp (from Hero ARts of course) and an old HA daisy and butterfly that I had. Colored everything with chalks and added a little glitter.) Thanks for looking!
200m2 is one of the UK's leading exhibition stand companies. Some of the biggest brands rely on us to create display walls for their global exhibitions programme. Find out more abour our products at 200m2.co.uk
At RMIT we pride ourselves on taking a hands on approach to learning. We believe you learn better when you try things for yourself, not just hear about it from someone else!
RMIT Việt Nam tin rằng cách học tập tốt nhất là Nhìn tận mắt – Làm tận tay. Sinh viên sẽ học được nhiều hơn khi tự mình đào sâu nghiên cứu kiến thức và ứng dụng những kiến thức đó vào thực tiễn.
Edited European Southern Observatory image of the interacting galaxies NGC 2207 and IC 2163.
Original caption: In this image, two spiral galaxies, similar in looks to the Milky Way, are participating in a cosmic ballet, which, in a few billion years, will end up in a complete galactic merger — the two galaxies will become a single, bigger one. Located about 150 million light-years away in the constellation of Canis Major (the Great Dog), NGC 2207 — the larger of the two — and its companion, IC 2163, form a magnificent pair. English astronomer John Herschel discovered them in 1835. The fatal gravitational attraction of NGC 2207 is already wreaking havoc throughout its smaller partner, distorting IC 2163’s shape and flinging out stars and gas into long streamers that extend over 100,000 light-years. The space between the individual stars in a galaxy is so vast, however, that when these galaxies collide, virtually none of the stars in them will actually physically smash into each other. This image was captured with the ESO Faint Object Spectrograph and Camera (EFOSC2) through three wide band filters (B, V, R). EFOSC2 has a 4.1 x 4.1 arcminute field of view and is attached to the 3.6-metre telescope at ESO’s La Silla Observatory in Chile.
This fully interactive online application simulates the function of a phoropter, which is used for subjective refraction procedures (eye exams). It is designed to give optical students a chance to get familiar with the instrument prior to lab exercises. The exercise has ten patients. The sight of the first five is hard coded and the last five are randomly generated.
The simulation is designed so a student can follow the normal eye exam procedure and determine a prescription for eyeglasses or contact lenses. For example, the student can test the vision of the patient by clicking “better 1”, making a small change in sphere power and then clicking “better 2” and deciding where to adjust further to get closer to the correct result. Once the best spherical power is achieved, cylindrical power and its axis rotation value can be tested. The eye chart is programmed to blur based on the patient’s eyesight and the instrument settings accounting for both spherical and cylindrical power. In the case of a large spherical defect, the blur will skew along the rotational axis of the defect. Once the chart is crisp and sharp, the refraction procedure is done and the patient can see!
I had to build custom blurring algorithms to visualize the effects of stigmatism ... essentially blurring it along an axis (the Flash blur effect API does not support a rotational property to a blur). The effect is pretty subtle unless you get the sphere power correction bang on.
See it in action:
(www.nait.ca/d3/phoroptor/phoroptor.html) UPDATE this url is closed.
Visual design and development by Randy Troppmann.
Awards:
CNIE (Canadian Network for Innovation in Education) Award of Merit - Excellence and Innovation in the Use of Technology for Learning and Teaching. May 13, 2009
Edited European Southern Observatory image of two interacting galaxies.
Original caption: Two galaxies, about 50 million light-years away, are locked in a galactic embrace — literally. The Seyfert galaxy NGC 1097, in the constellation of Fornax (The Furnace), is seen in this image taken with the VIMOS instrument on ESO’s Very Large Telescope (VLT). A comparatively tiny elliptical companion galaxy, NGC 1097A, is also visible in the top left. There is evidence that NGC 1097 and NGC 1097A have been interacting in the recent past. Although NGC 1097 seems to be wrapping its companion in its spiral arms, this is no gentle motherly giant. The larger galaxy also has four faint jets — too extended and faint to be seen in this image — that emerge from its centre, forming an X-shaped pattern, and which are the longest visible-wavelength jets of any known galaxy. The jets are thought to be the remnants of a dwarf galaxy that was disrupted and cannibalised by the much larger NGC 1097 up to a few billion years ago. These unusual jets are not the galaxy’s only intriguing feature. As previously mentioned, NGC 1097 is a Seyfert galaxy, meaning that it contains a supermassive black hole in its centre. However, the core of NGC 1097 is relatively faint, suggesting that the central black hole is not currently swallowing large quantities of gas and stars. Instead, the most striking feature of the galaxy’s centre is the ring of bright knots surrounding the nucleus. These knots are thought to be large bubbles of glowing hydrogen gas about 750–2500 light-years across, ionised by the intense ultraviolet light of young stars, and they indicate that the ring is a site of vigorous star formation With this distinctive central star-forming ring, and the addition of numerous bluish clusters of hot, young stars dotted through its spiral arms, NGC 1097 makes a stunning visual object. The data were originally taken in 2004 (see eso0438) with the VIMOS instrument on the VLT, and additional colour information from an image taken by amateur astronomer Robert Gendler has been superimposed. The VLT data were taken through three visible-light filters: R (at a wavelength of 652 nanometres, and shown here in red), V (a wavelength of 540 nanometres, shown in green), and B (456 nanometres, shown in blue). The image covers a region of approximately 7.7 x 6.6 arcminutes on the sky.