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LRGB filter set Diam. 50.8mm Series

LRGB filter set Diam. 50.8mm Series

Set Filters Lrgb Diam. 50mm Unmounted Series For Kodak Sensors Blu-Enhanced Ccd Type And Sxv-H9.

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LRGB filter set Diam. 50.8mm Series



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Set Filters Lrgb Diam. 50mm Unmounted Series For Kodak Sensors Blu-Enhanced Ccd Type And Sxv-H9.

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"The spectrum preliminary filter Tru-Balance E series is shown in the figure: the emission lines of H-Alpha and dell'OIII near 656 and 500 nm are shown. The SII emits at 672.4nm, lengths d ' wave slightly higher H-Alpha. The SII is also an emission line that is part of the transmission curve of the red filter a set of RGB.
Note the amplitude of the curve of the blue filter: this compensates for the lack of sensitivity in blue Kodak sensor full frame in comparison to that in the green and red. This blue filter has an efficiency of 50% higher than that of the blue filter of Custom Scientific, 30% higher than the blue filter 2C dell'Astronomik, taking realize that the Astronomik RGB filters produces the best in amateur.
This means that with the blue filter Astrodon will immediately notice an increase in the signal / noise ratio and the details in the images of the blue channel already upon download image rough.
This also means avoid losing the guide star when using the blue filter with integrated CCD autoguiding.
The gray curve in figure is that of the filter Luminance (L) with block-infrared (NIR).
This filter is designed to combine with the spectral amplitudes of the RGB filters, adapting like a glove in order to ensure the best chromatic yield in the images obtained with LRGB.
A filter type Clear (C) without block infrared can be used in place of the filter L. The filter C has a transmission greater than 97% in the spectral region, that transmission drops to 95% at 400nm in the blue. Filter C allows you to increase by 45% the luminance signal with sensors Kodak spacing but may not offer a perfect coupling to the set as is possible with the RGB filter L.
Finally you notice in the picture the interval between filter curve green and red filter. This feature helps to minimize the negative effects of light pollution of high-pressure sodium lamps. These sources of light pollution are usually at 580nm, the spectral region in which these green and red filters let through only 15% of light. Therefore the filters series E have an anti-light pollution built.

All filters are parfocal Astrodon:
most frustration nell'astrofotografia with CCD is that of having to find the correct position fire with the filter H-alpha filters narrowband keep out much light so you must use a very bright star to perfect focus. All filters Astrodon Tru-Balance L, C, R, G, B, H-Alfa, OIII and SII are parfocal on optics with focal ratio less than f / 4. Login This means you can adjust the focus by using a filter C or G, install a filter H-Alpha and immediately proceed with the acquisition. This is one of the key advantages of the Tru-Balance filters Astrodon that made them so popular in a short time.
The thickness of the filter determines how it can be parafocality: Tru-Balance filters are dichroic filters with very resistant treatments deposited on a single glass substrate of high quality. The reduced thickness (3mm) of this substrate is controlled accurately with error +/- 0.05mm. The change from lot to lot is less than 0.1mm, measuring slightly less than the critical areas of focus of a system f / 5. On request it is possible to select within various batches filters with less variation and then get a set of filters that have the exact same thickness (prices on request).

balance corrected blue-green OIII: < / b>
when applying the same weight to the three colors (1: 1: 1) for the point of the white balance, the next step is to obtain a correct blue-green color corresponding to the issuance OIII in the region Central of planetary nebulae. Login This it requires that the emission line OIII has a component equal both in the green channel than in the blue, AFTER you apply the weights G2V for correct color balance of the stars and therefore white. < br> This is what is meant by "" œParadosso RGB color "": when applied weights G2V-color to your camera and filters, the proper balancing of the emission line OIII for the final images in the blue and green it is impossible. There is little to do but slightly alter the weight-color G2V. This is the problem in "" œmescolare "" in astrophotography emissions in narrow bands (eg. OIII) with colors in wide stripes (RGB). This problem does not affect the emission lines H-Alpha and SII because both fall in the curve of the red filter. The problem is characteristic of the emission line dell'OIII close to 500nm which falls between the curve of the blue filter and that of the green filter. The problem is even more evident when using photometric filters UVBRI as the blue photometric filter has a very low transmission nell'OIII.
Note however high and similar transmission filters green and blue Astrodon level of emission line OIII : from the time that the weights applied are 1: 1: 1, the transmission nell'OIII must be the same for both the green filter for the blue one. This not only allows to obtain a correct blue-green color for the OIII but does so with a high efficiency. The speech is valid for both the series and that for that I. In other words you will eventually get such a M27 with the right color. The Astrodon Tru-Balance filters provide color nebulae OIII requiring a balance by up to 10%, no other filter on the market has such efficiency.

The figure shows will follow what you mean by image "" œtroppo green "" or "" œtroppo blue "" in comparison with well-balanced image.
The last image shows the planetary nebula M27 taken with a CCD sensor and a KAF3200ME C14: color combination 1: 1: 1, exposure of 10min for R, G and B using the filters Astrodon Tru -BALANCE series E. Note the details that have emerged despite a total exposure time of 30 min reduced and how the color of the nebula is well balanced, neither too green or too blue. "

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