Stereoscopic Glasses If i would buy an ordinary 120 Hz LCD TV , would i be able to play 3d games?
I was wondering if i would buy an ordinary 120 Hz LCD TV that doesn't specify whether or not it supports stereoscopic 3d, could i play 3d games on it (on my PS3)? And also, what type of 3d glasses would i need?
No.
Sony is currently working out on packaging an add-on unit for retro-fitting non-3D TVs into 3D TVs. When they release that (should be this summer), then you could get that and make your TV into a 3D TV.
The glasses aren't out yet, but just go to a TV store and they'll have them for you. You won't be using those junk paper things. You'll be using the hard plastic style at like theaters (Shutter glasses). Pricing hasn't been announced, but the expectation is anywhere from $100 - $300 per pair (with the expectation that a 3D TV will come included with at least 1 pair).
How can I create an animation for viewing with 3d glasses?
I have 3ds max and Adobe After effects. Is is possible for me to render the stereoscopic footage and composite for viewing on a 3d monitor (Nvidia one maybe with 3d shutter glasses?)
Well, take the picture and duplicate it.
Put them side by side and put your glasses on and then.
Ta da
28 July 2005
These images, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, show a patch of water ice sitting on the floor of an unnamed crater near the Martian north pole.
Map showing crater in context
The HRSC obtained these images during orbit 1343 with a ground resolution of approximately 15 metres per pixel. The unnamed impact crater is located on Vastitas Borealis, a broad plain that covers much of Mars's far northern latitudes, at approximately 70.5° North and 103° East.
The crater is 35 kilometres wide and has a maximum depth of approximately 2 kilometres beneath the crater rim. The circular patch of bright material located at the centre of the crater is residual water ice.
Colour view of crater with water ice
This white patch is present all year round, as the temperature and pressure conditions do not favour the sublimation of water ice.
It cannot be frozen carbon dioxide since carbon dioxide ice had already disappeared from the north polar cap at the time the image was taken (late summer in the Martian northern hemisphere).
Black and white view of crater with water ice
There is a height difference of 200 metres between the crater floor and the surface of this bright material, which cannot be attributed solely to water ice.
It is probably mostly due to a large dune field lying beneath this ice layer. Indeed, some of these dunes are exposed at the easternmost edge of the ice.
Faint traces of water ice are also visible along the rim of the crater and on the crater walls. The absence of ice along the north-west rim and walls may occur because this area receives more sunlight due to the Sun’s orientation, as highlighted in the perspective view.
3D anaglyph view of crater with water ice
The colour images were processed using the HRSC nadir (vertical view) and three colour channels. The perspective views were calculated from the digital terrain model derived from the stereo channels.
The 3D anaglyph images were created from the nadir channel and one of the stereo channels. Stereoscopic glasses are needed to view the 3D images Image resolution has been decreased for use on the internet.
For more information on Mars Express HRSC images, you might like to read our updated 'Frequently Asked Questions'.
Wait until the glasses are able to dynamically adjust the focus of specific points on the screen. Problem fixed! Or maybe something cool like this: Or maybe any technology that doesn’t require all of the following: 2D screen, stereoscopic glasses to mimic convergence, source image coming from a 2D layer, or multiple people to see the same image.
2 Comments
28 July 2005
These images, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, show a patch of water ice sitting on the floor of an unnamed crater near the Martian north pole.
Map showing crater in context
The HRSC obtained these images during orbit 1343 with a ground resolution of approximately 15 metres per pixel. The unnamed impact crater is located on Vastitas Borealis, a broad plain that covers much of Mars's far northern latitudes, at approximately 70.5° North and 103° East.
The crater is 35 kilometres wide and has a maximum depth of approximately 2 kilometres beneath the crater rim. The circular patch of bright material located at the centre of the crater is residual water ice.
Colour view of crater with water ice
This white patch is present all year round, as the temperature and pressure conditions do not favour the sublimation of water ice.
It cannot be frozen carbon dioxide since carbon dioxide ice had already disappeared from the north polar cap at the time the image was taken (late summer in the Martian northern hemisphere).
Black and white view of crater with water ice
There is a height difference of 200 metres between the crater floor and the surface of this bright material, which cannot be attributed solely to water ice.
It is probably mostly due to a large dune field lying beneath this ice layer. Indeed, some of these dunes are exposed at the easternmost edge of the ice.
Faint traces of water ice are also visible along the rim of the crater and on the crater walls. The absence of ice along the north-west rim and walls may occur because this area receives more sunlight due to the Sun’s orientation, as highlighted in the perspective view.
3D anaglyph view of crater with water ice
The colour images were processed using the HRSC nadir (vertical view) and three colour channels. The perspective views were calculated from the digital terrain model derived from the stereo channels.
The 3D anaglyph images were created from the nadir channel and one of the stereo channels. Stereoscopic glasses are needed to view the 3D images Image resolution has been decreased for use on the internet.
For more information on Mars Express HRSC images, you might like to read our updated 'Frequently Asked Questions'.
Wait until the glasses are able to dynamically adjust the focus of specific points on the screen. Problem fixed! Or maybe something cool like this: Or maybe any technology that doesn’t require all of the following: 2D screen, stereoscopic glasses to mimic convergence, source image coming from a 2D layer, or multiple people to see the same image.