Computer
Objective: Use of Software Adobe Premiere Cs3
Skills: is the creation of video footage and live audio using the software time adobe Cs3
Incorporation from other software.
transcision Creation of audio effects and video, credits Gc.
Generation of compressed files (mpg,. Mov, AVI) in a final dvd
digitizing devices using video cameras. Activity
1 .- Find and post on his blog: "A tutorial
premiere CS3 software (Video) (PDF)
Work-group max 4 persons
-build and create a video of a minimum of 40 seconds and a maximum of 3 minutes.
must-have titles and captions input or output Gc
-transition effects and audio video music should have. Free-Topic
and respect the times.
-The working group delivered the final work on a DVD.
Thursday, April 23, 2009
Tuesday, April 7, 2009
Do Male Or Females Get Cystic Fibrosis
Example color calibration of large-scale processing (wavelets)
What I show below is a simple way to process large-scale structures from the brainchild of Carlos Milovic (PTeam).
This sample processing large scale is made on an image of the Milky Way centered on the constellation of Cygnus. This is a single 30 minute exposure Fuji film Provia 400F chemistry through a standard lens 50mm F4 closed, taken in August 2004 under clear skies and dark (Ordesa).
This image is an excellent test which enhance large-scale structures. The picture is processed entirely in PixInsight Core. The adjustments include color calibration, correction of the backlight (ABE) by a division based on prior data linearization (Divide), histograms, curves and noise reduction for luminance (ACDNR).
In this photograph, to process large-scale structures a problem occurs. The stars, especially the brightest, for reflections in the upper layers of wavelets. This means that increasing the weight in layers where the stars are not present, they also exert some influence, creating strange halos.
You must then add the result to the image of small-scale objects (mainly stars), this time Rescaling.
enhanced
What I show below is a simple way to process large-scale structures from the brainchild of Carlos Milovic (PTeam).
This sample processing large scale is made on an image of the Milky Way centered on the constellation of Cygnus. This is a single 30 minute exposure Fuji film Provia 400F chemistry through a standard lens 50mm F4 closed, taken in August 2004 under clear skies and dark (Ordesa).
This image is an excellent test which enhance large-scale structures. The picture is processed entirely in PixInsight Core. The adjustments include color calibration, correction of the backlight (ABE) by a division based on prior data linearization (Divide), histograms, curves and noise reduction for luminance (ACDNR).
In this photograph, to process large-scale structures a problem occurs. The stars, especially the brightest, for reflections in the upper layers of wavelets. This means that increasing the weight in layers where the stars are not present, they also exert some influence, creating strange halos.

The solution here is basically subtract the stars, to isolate them. It is not possible to simply disable the wavelets the lower layers (small scale) because the halos dark adversely affect the outcome. We must do the opposite: to duplicate the image (in this case the luminance) and her first disable all layers above 64 pixels. Then, it maximizes deringing parameter in the layers survivors and applied. This generates an image with the stars alone, without his halo negative.

then subtract the result (without climbing) and you get a picture without the small-scale components (smaller than 64 pixels).
This is usually enough to enhance large-scale structures by changing the weight of the upper layers of wavelets. However, if only enhance dark detail, bright structures dilute the effect. The solution is to invert the image with no stars, before and after processing the dark structures.
This is usually enough to enhance large-scale structures by changing the weight of the upper layers of wavelets. However, if only enhance dark detail, bright structures dilute the effect. The solution is to invert the image with no stars, before and after processing the dark structures.

You must then add the result to the image of small-scale objects (mainly stars), this time Rescaling.

enhanced
Once large-scale structures, we combine the processed luminance original RGB image.
Here we have used the LRGBCombination process for several reasons. First, we import the luminance changing their relative weight with respect to the RGB data, on the other hand, we also avoid the loss of color saturation by light transfer function halftones on the channel C, while reduce the noise in the chrominance.

Make Your Own Portable Dvd Player Car Strap
The Backbone of Night
The most successful work has been the most brilliant science writer, Cosmos Carl Sagan, the author relates:
\u0026lt;\u0026lt;"the Backbone of Night", as if the sky was a large animal in which we live ... The Kung believe that the Milky Way holds the night, but for the Milky Way, dark pieces fall, breaking at our feet. It's a smart idea>>
The following image is inspired by the paintings of Jon Lomberg, published in that book, which describes a metaphor about the nature of the Milky Way told Kung people of the Republic of Botswana. I recommend you view the image at a minimum distance of 1.5-2 meters above the monitor:
More information on how we obtained the final result can be found at: http://www
.astrosurf.com/astro35mm/articulos/procesamiento/procesamiento2/procesamiento2.htm
Well, even so, there are several reasons why the stars do not appear at the end of processing as bright as in the raw image. First, there are several processing techniques with multi-scale wavelet tend to produce that effect. Fortunately it is something that has easy solution, because usually only a matter of giving more or less emphasis on small-scale components, which normally are present most stars. Second, this effect can be caused also by the use of filters at least, and if not handled carefully, the stars tend to leave "dull", which again they lose some of their role. And finally, this aspect can be generated simply by the desire of the author.
When running a portrait photographer for instance, always seeks to highlight the subject from the background, blurring it and preventing any other element can distract the viewer's attention. When photographing deep sky same thing happens, there is a subject and a background. The subject here is the Milky Way and the rest is the background of the sky and many stars in the field. Therefore, if you want your taxable gain greater prominence on the scene, need to reduce the visual impact generated by the stars.
Speaking of pictures, than the mere physical identification (photo ID card, for example), the portrait is intended to reveal the character, feelings, moods, etc ... However, if our intention is to reveal all these features at once, most likely the subject will not be too encouraged. Of course the Milky Cap is not an animate subject and lack of character, or mood. But we do know one very own, such as its dimensions. The Milky Way is a galaxy that is presented before our eyes like an unusually large structure. Therefore, it is in the larger scales where it can be useful to have a more in our processing, it is a quality we want to highlight of our subject, and because our intention is not just a mere physical identification of the object.
On the other hand, there are many forms and ways to process an image. We can be proud to have flexible tools that allow us to express ourselves freely and be creative. Of course, the most important part of processing this image of the Milky Way with a 50mm lens, are the last two steps, in which one tries to enhance both the dark structures of small and medium scale, such as large-scale bright . Logically explain this requires an extensive article with step by step examples. What I think I have already commented here about this type of image processing, is that when processing the images with the wavelets, and try to give more importance or weight to the upper layers (large scale), you just realizing that problem is that stars, especially the brightest, for reflections in the upper layers of wavelets. This means that if you increase the bias in layers where there are no stars, they also exert some influence, creating strange halos. This effect is caused by the fact that the scaling function in wavelet can not completely isolate the stars in certain layers. Fortunately there is an easy solution: subtract the stars, to isolate. You simply can not disable the lower layers wavelet (small scale) because the dark halos affect the result. We must do the opposite: duplicate the image and her first disable all the upper layers, for example, 32 pixels. Then, it maximizes the layers survivors deringing and applied. This will generate an image with the stars alone, without the negative halo. Then you must subtract this image without scaling and then re-add, this time Rescaling. In between subtraction and addition is introduced all the processes to apply to the picture without stars.
In most cases this is usually sufficient to enhance the bright structures. But what about the dark structures? In that case we need to invest the image with no stars before and after processing structures, so that as in the image do not have stars, or their presence is minimal, increasing the influence deringing now avoid generating bright structures.
must be remembered also, for example, that if you want only to isolate the components of small or large, should be applied to image simultaneously the wavelets on the luminance and chrominance, except when they want to enhance details or structures should then be applied only on luminance and then combine the result with the color data (RGB). Finally, the masks play a role. Actually are you at all times to control which areas or components of the image are processed and which not. In the end, the further away you get, the more sophisticated end up being the masks. Trying this picture of the Milky Way at times I found the need to combine several masks at the same time in order to protect small-scale components present in highly lit areas, while protecting against the sky while enhancing high-level details.
Be happy,
The most successful work has been the most brilliant science writer, Cosmos Carl Sagan, the author relates:
\u0026lt;\u0026lt;"the Backbone of Night", as if the sky was a large animal in which we live ... The Kung believe that the Milky Way holds the night, but for the Milky Way, dark pieces fall, breaking at our feet. It's a smart idea>>
The following image is inspired by the paintings of Jon Lomberg, published in that book, which describes a metaphor about the nature of the Milky Way told Kung people of the Republic of Botswana. I recommend you view the image at a minimum distance of 1.5-2 meters above the monitor:

More information on how we obtained the final result can be found at: http://www
.astrosurf.com/astro35mm/articulos/procesamiento/procesamiento2/procesamiento2.htm
Well, even so, there are several reasons why the stars do not appear at the end of processing as bright as in the raw image. First, there are several processing techniques with multi-scale wavelet tend to produce that effect. Fortunately it is something that has easy solution, because usually only a matter of giving more or less emphasis on small-scale components, which normally are present most stars. Second, this effect can be caused also by the use of filters at least, and if not handled carefully, the stars tend to leave "dull", which again they lose some of their role. And finally, this aspect can be generated simply by the desire of the author.
When running a portrait photographer for instance, always seeks to highlight the subject from the background, blurring it and preventing any other element can distract the viewer's attention. When photographing deep sky same thing happens, there is a subject and a background. The subject here is the Milky Way and the rest is the background of the sky and many stars in the field. Therefore, if you want your taxable gain greater prominence on the scene, need to reduce the visual impact generated by the stars.
Speaking of pictures, than the mere physical identification (photo ID card, for example), the portrait is intended to reveal the character, feelings, moods, etc ... However, if our intention is to reveal all these features at once, most likely the subject will not be too encouraged. Of course the Milky Cap is not an animate subject and lack of character, or mood. But we do know one very own, such as its dimensions. The Milky Way is a galaxy that is presented before our eyes like an unusually large structure. Therefore, it is in the larger scales where it can be useful to have a more in our processing, it is a quality we want to highlight of our subject, and because our intention is not just a mere physical identification of the object.
On the other hand, there are many forms and ways to process an image. We can be proud to have flexible tools that allow us to express ourselves freely and be creative. Of course, the most important part of processing this image of the Milky Way with a 50mm lens, are the last two steps, in which one tries to enhance both the dark structures of small and medium scale, such as large-scale bright . Logically explain this requires an extensive article with step by step examples. What I think I have already commented here about this type of image processing, is that when processing the images with the wavelets, and try to give more importance or weight to the upper layers (large scale), you just realizing that problem is that stars, especially the brightest, for reflections in the upper layers of wavelets. This means that if you increase the bias in layers where there are no stars, they also exert some influence, creating strange halos. This effect is caused by the fact that the scaling function in wavelet can not completely isolate the stars in certain layers. Fortunately there is an easy solution: subtract the stars, to isolate. You simply can not disable the lower layers wavelet (small scale) because the dark halos affect the result. We must do the opposite: duplicate the image and her first disable all the upper layers, for example, 32 pixels. Then, it maximizes the layers survivors deringing and applied. This will generate an image with the stars alone, without the negative halo. Then you must subtract this image without scaling and then re-add, this time Rescaling. In between subtraction and addition is introduced all the processes to apply to the picture without stars.
In most cases this is usually sufficient to enhance the bright structures. But what about the dark structures? In that case we need to invest the image with no stars before and after processing structures, so that as in the image do not have stars, or their presence is minimal, increasing the influence deringing now avoid generating bright structures.
must be remembered also, for example, that if you want only to isolate the components of small or large, should be applied to image simultaneously the wavelets on the luminance and chrominance, except when they want to enhance details or structures should then be applied only on luminance and then combine the result with the color data (RGB). Finally, the masks play a role. Actually are you at all times to control which areas or components of the image are processed and which not. In the end, the further away you get, the more sophisticated end up being the masks. Trying this picture of the Milky Way at times I found the need to combine several masks at the same time in order to protect small-scale components present in highly lit areas, while protecting against the sky while enhancing high-level details.
Be happy,
Monday, April 6, 2009
Swing Set For Sale Calgary
Images
lists already are running five wide-field images with old film. I need to remove the scratches and make updates to publish to web.
lists already are running five wide-field images with old film. I need to remove the scratches and make updates to publish to web.
Sunday, April 5, 2009
Where To Buy Bracelet Ring
reprocessed old Thor's helmet Jim Misti
Well, Jim Misti recently published new data to process:
http://www.mistisoftware.com/Astronomy/index_fits.htm
Among the nine new pictures published I selected the NGC 2359 (Thor's Helmet). The data contains ten shots stacked five minutes for the luminance (unbinned) and five of five minutes for each RGB channel (3x3 binning). All through the RC telescope of 32 ":
There is a higher resolution version available at the following link:
http://www.wrunch.com/viewer.php?id=bwy1238864343l . jpg
And for comparison, here are the same data processed by Robert Gendler:
http://www.robgendlerastropics.com/NGC2359JM.html
Well, Jim Misti recently published new data to process:
http://www.mistisoftware.com/Astronomy/index_fits.htm
Among the nine new pictures published I selected the NGC 2359 (Thor's Helmet). The data contains ten shots stacked five minutes for the luminance (unbinned) and five of five minutes for each RGB channel (3x3 binning). All through the RC telescope of 32 ":
There is a higher resolution version available at the following link:
http://www.wrunch.com/viewer.php?id=bwy1238864343l . jpg
And for comparison, here are the same data processed by Robert Gendler:
http://www.robgendlerastropics.com/NGC2359JM.html
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