Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
lighter_than_air [2014-09-27 00:34] – cocky | lighter_than_air [2014-09-27 17:27] (current) – cocky | ||
---|---|---|---|
Line 35: | Line 35: | ||
- | {{:graham_stevensthumb.jpg?300}}\\ | + | {{:desert-cloud-installation-1972.jpg?500}}\\ |
http:// | http:// | ||
- | Atmosfields 1971 Dessert Cloud 1974, Graham Stevens works in Centre Pompidou in Paris 2008. | + | Graham Stevens work rejects the idea of architecture as something static and explores the interaction between human and the invisible environments surrounds them daily.Atmosfields 1971, Dessert Cloud 1974. |
- | Research of the topic: Art and Levitation | + | http:// |
- | http:// | + | watch this movie at !!! http:// |
- | http:// | + | |
\\ | \\ | ||
- | {{: | + | {{: |
Breitling Orbiter, photographed by Jeremy l. Hinton, 1973\\ | Breitling Orbiter, photographed by Jeremy l. Hinton, 1973\\ | ||
Breitling Orbiter 3 was the first balloon to fly around the world non-stop, piloted by Bertrand Piccard and Brian Jones. Designed and built by Cameron Balloons, of Bristol, England, Breitling Orbiter 3 stood 55 m (180 ft) tall when fully inflated. The propane gas that fueled the six burners was contained in 28 titanium cylinders mounted in two rows along the sides of the gondola. Concerned about fuel consumption, | Breitling Orbiter 3 was the first balloon to fly around the world non-stop, piloted by Bertrand Piccard and Brian Jones. Designed and built by Cameron Balloons, of Bristol, England, Breitling Orbiter 3 stood 55 m (180 ft) tall when fully inflated. The propane gas that fueled the six burners was contained in 28 titanium cylinders mounted in two rows along the sides of the gondola. Concerned about fuel consumption, | ||
\\ | \\ | ||
- | {{tophat_launch_72.jpg? | + | {{tophat_launch_72.jpg? |
" | " | ||
Such measurements have become increasingly important for providing information on the initial conditions from which the large-scale structure of the Universe has evolved. The detailed measurement phase promises quantitative answers to some of the fundamental questions of structure evolution in our Universe: How did matter first distribute itself to eventually form the bubbles, voids and galaxy clusters that we observe? What is the amplitude of the quantum fluctuations which existed before the Universe entered the `inflationary' | Such measurements have become increasingly important for providing information on the initial conditions from which the large-scale structure of the Universe has evolved. The detailed measurement phase promises quantitative answers to some of the fundamental questions of structure evolution in our Universe: How did matter first distribute itself to eventually form the bubbles, voids and galaxy clusters that we observe? What is the amplitude of the quantum fluctuations which existed before the Universe entered the `inflationary' |