Tuesday, April 7, 2009

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,

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.

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

Saturday, March 14, 2009

What Does Light Do To Things



do you think about how it is leaving the matter? I need a perspective back outside to see if I'm on the right track, so you can leave your comments here.

The following link is the starting image:
http://pteam.pixinsight.com/sonnenstein/sagitario_raw.jpg

As I mentioned, the processing of this image was made using a criterion rather than the other images that I processed these days.

And in this other link shows the result after processing:
http://pteam.pixinsight.com/sonnenstein/sagitario_test.jpg


The first step, first of all consists of a single halftone setting really aggressive in the channel RGB / K combined (0.00001). This setting delivers pixel values \u200b\u200bin the entire image around 0.9995!

then adjust the dynamic range ( autoclip in the shadows and lights) the sky background starts to have values \u200b\u200baround 0.4 to 0.6, as shown in the following video:


This first adjustment is not always the work on CCD images, because the raw data and tend to occupy the entire available dynamic range, but yes, very compressed in the shadows. So adjust the dynamic range after applying this transfer function as aggressive halftone not affect the outcome. However, for disponéis still images taken with film, this method will allow you to take a much more linear aspect to the whole image, so I think that can be approximated quite what you get in peak condition with a DSLR and a single dose of 10-15 minutes.

Well then, in this early stage of processing, I think a good time to make a noise reduction, for two reasons:

- Apply a transfer function as aggressive tones media has left the bell-shaped histogram saw. That is, the noise is now everywhere distributed throughout the tonal range of the image.


- The algorithm for noise reduction and edge protection ACDNR adapts much more easily when the sky background values \u200b\u200bfound in this case in a higher range.

Fortunately, the read noise generated by the film scanner is relatively easy to remove by ATWT, as this type of noise is usually distributed at high spatial frequencies. So I just eliminated the first layer of wavelets, choosing a scaling function and a Gaussian kernel 3x3.


If however the noise generated by the film grain and is 'another story'. Here I had to apply two noise reduction:

- The first reduction includes a standard deviation value around 1.8 in 2.5 in the luminance and chrominance, using symmetrical threshold values \u200b\u200bfor edge protection. It is obvious that in these cases, a luminance mask inverted wavelets and curves adjusted, it always helps to define a much more controlled areas of the image where you must act more or less noise reduction.

- The second reduction is only for luminance, using a higher filter value (StdDev = 6.5). Also chose symmetrical values \u200b\u200bfor the protection of borders, but with much lower thresholds. Finally readjusted again the dynamic range, because as you know, the filter function in ACDNR tends to slightly reduce the contrast, especially in the areas of signal to noise ratio poorest, where the mask allows the filter to a greater extent .

Here is a good idea to also reduce chroma noise with SCNR in the green channel. Nothing new here to tell, except that in this case it worked better the method Maximum .

Now is the time neutralizes the sky. In this picture there are few regions can be defined strictly as a background, so I had to rely on running DBE interpolation after putting some samples at the top of the image. As simpre that successfully neutralizes the sky background, the left side of the hood of the histogram is more straight and steep, so that makes us free to leave a small portion of dynamic range in the shadows. So with HistogramTransformation again give him a light push on image contrast.

now the image is very far from showing a color balance. However, it is not possible to have a linear image because of reciprocity failure suffered by the film, is relatively easy to calibrate the color modifying the midtones independently on each RGB channel.

Finally, the most fun was to maximize color saturation by MTF on channel C (CIE L * c * h *) from LRGBCombination before taking action with multiscale processing, separating small-scale structures and removing them from the larger scales, where structures appear better defined in the Milky Way. HDRWT applied on these structures using eight layers, one iteration. As you know, this action increases the overall contrast to the entire image within defined structures. Then reinsert the result together with small-scale image of the original. This operation sometimes causes a slight imbalance between small structures and the rest of the image. So I took the opportunity to add more weight on small structures, while iteratively applied morphological and wavelet filters to the stars.

It is now a good gigs with CloneStamp .