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Reblogged from cjwho  835 notas

cjwho:

The Naked House by Marc Gerritsen

"The main thing about this location is the expanse of the surroundings and the quietness. Life in Taipei is very hectic, and I needed a place to escape. I really wanted a quiet area and a fantastic view. Having an open plan living room, with doors that can totally slide away, which looks out at the pool and the ocean – that’s something I’d been thinking about for a long time. With this plot, I was able to put the pieces of the puzzle together. The house was a return to the basic values in life: good clean air, wide open space, quiet solitude. With these basic values you can be in a space that is uncluttered, and your mind can become still. That’s also the reason behind the very basic materials that I have used: concrete, wood, steel and glass. There are no embellishments. The focus is on the space rather than the materials.

I originally planned three stories: two bedrooms on the bottom; the pool, living area and kitchen on the middle level; and an office on top. But I’ve added a bathroom on the living room level, a laundry room and pantry. I wanted a simple kitchen, with no overhead cupboards or tall fridge, so the pantry is good for storage. I added a freestanding open-air bathroom, as the top room became a magnificent master bedroom which needed an en-suite. The tank and plant room became a large open room with a swing bed, underneath the deck I added a steam room, and the space below the bedrooms now houses an office and maid’s room. So it ended up being five stories – the result of a work in progress”, said Gerritsen.

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thedemon-hauntedworld:

Radio Occultation: Unraveling Saturn’s Rings Specially designed Cassini orbits place Earth and Cassini on opposite sides of Saturn’s rings, a geometry known as occultation. Cassini conducted the first radio occultation observation of Saturn’s rings on May 3, 2005. Three simultaneous radio signals of 0.94, 3.6, and 13 centimeter wavelength (Ka-, X-, and S-bands) were sent from Cassini through the rings to Earth. The observed change of each signal as Cassini moved behind the rings provided a profile of the distribution of ring material as a function of distance from Saturn, or an optical depth profile. This simulated image was constructed from the measured optical depth profiles. It depicts the observed ring structure at about 10 kilometers (6 miles) in resolution. Color is used to represent information about ring particle sizes in different regions based on the measured effects of the three radio signals. Purple color indicates regions where there is a lack of particles of size less than 5 centimeters (about 2 inches). Green and blue shades indicate regions where there are particles smaller than 5 centimeters (2 inches) and 1 centimeter (less than one third of one inch). The saturated broad white band near the middle of ring B is the densest region of ring B, over which two of the three radio signals were blocked at 10-kilometer (6-mile) resolution, preventing accurate color representation over this band. From other evidence in the radio observations, all ring regions appear to be populated by a broad range particle size distribution that extends to boulder sizes (several to many meters across). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The radio science team is based at JPL.

thedemon-hauntedworld:

Radio Occultation: Unraveling Saturn’s Rings
Specially designed Cassini orbits place Earth and Cassini on opposite sides of Saturn’s rings, a geometry known as occultation. Cassini conducted the first radio occultation observation of Saturn’s rings on May 3, 2005.
Three simultaneous radio signals of 0.94, 3.6, and 13 centimeter wavelength (Ka-, X-, and S-bands) were sent from Cassini through the rings to Earth. The observed change of each signal as Cassini moved behind the rings provided a profile of the distribution of ring material as a function of distance from Saturn, or an optical depth profile.
This simulated image was constructed from the measured optical depth profiles. It depicts the observed ring structure at about 10 kilometers (6 miles) in resolution. Color is used to represent information about ring particle sizes in different regions based on the measured effects of the three radio signals.
Purple color indicates regions where there is a lack of particles of size less than 5 centimeters (about 2 inches). Green and blue shades indicate regions where there are particles smaller than 5 centimeters (2 inches) and 1 centimeter (less than one third of one inch). The saturated broad white band near the middle of ring B is the densest region of ring B, over which two of the three radio signals were blocked at 10-kilometer (6-mile) resolution, preventing accurate color representation over this band. From other evidence in the radio observations, all ring regions appear to be populated by a broad range particle size distribution that extends to boulder sizes (several to many meters across).
The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The radio science team is based at JPL.