Astromania 1.25" Astrophotography Flip Mirror - The flip Mirror for Precise Focusing

£94.995
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Astromania 1.25" Astrophotography Flip Mirror - The flip Mirror for Precise Focusing

Astromania 1.25" Astrophotography Flip Mirror - The flip Mirror for Precise Focusing

RRP: £189.99
Price: £94.995
£94.995 FREE Shipping

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Now, during the global pandemic, when everyone wears a face mask, the online mirror can help you a lot. In situations where you do not have a real mirror, the online mirror helps you to properly arrange the protective mask, carefully covering your mouth and nose. Use our online mirror, arrange your face mask, to be comfortable, but at the same time to be fixed correctly. Wear a protective mask correctly and be healthy! So if anyone can help me and suggest way's for the flip mirror to fit on my scope, If would of great help. The dimensions of the mirror are such that 36x24mm is reflected. That's quit small to cover the inner 38mm of the 42mm tube system. I now think I have it worked out, although I need some clear skies to test my theory. The key is the two sets of 3 hex screws on the top of the body, just above the mirror arm pivot points. T-2 Fine-Adjustment rings (0,3 / 0,5 / 1 mm) - Aluminium ( #2457910, € 14,63) (also available separately) for eyepieces with the field stop inside of the nose piece

Dark frames are very easy to take by just flipping the mirror to the eyepiece. In fact, I usually take darks, while doing the fine centering of the object in the ep. Quantum mechanics is a fundamental theory in physics that describes the behavior of nature at the scale of atoms and subatomic particles.[2]: 1.1 It is the foundation of all quantum physics including quantum chemistry, quantum field theory, quantum technology, and quantum information science.Please note that the upper port is restricted by the T-2-thread and the diameter of the diagonal. The usable field is 32mm, equal to our 32mm T-2 prism diagonals. The distances vary, depending on nosepiece and focus of the guiding camera – it may as well work without a 1.25"-extension. Please note that the upper port is limited by the diameter of the T-2-thread, so it is a little bit less than 40mm, and there will be some vignetting with 2"-eyepieces with long focal lengths. Finally, I’m going to cover what might be considered the most important part – the mirror itself. I must admit to being no real expert in how to judge a flat mirror, but it seems to have an even surface with no blemishes. Star images both in and out of focus were as I’d expect and didn’t show any unusual problems. With 2 strips of double-sided adhesive tape of 2-3mm wide, this cover plate can be fixed without damaging the original rear mirror.

The field stop of the eyepiece and the camera sensor should each be in the same distance from the Flip Mirror. Our video flipper lets users set the preferred file format. It can be MP4, MOV, MKV. This way, you can use this tool not only to mirror videos but also to convert your files into different formats.BTW, I just got my first view on M74 from the side of my house on a really busy main street in the red zone of long beach california. The image doesn't look impressive,actually it's terrible =), but I found it thanks to the platesolving. I've been trying to research if there is a good resource for calculations to model the light angles before I start throwing money at it but I haven't found too much, does anyone have any resource recommendations? You will also see some more values such as Astigmatism and Coma. Again, these are measured by the interferometer when we take measurements of the optical surface after adjustment. These are values which ideally would be at 0 but as our test optics are all curved lenses, there will always be astigmatism and coma present. The lower the number, the less of these aberations you will effectively see but with most refractors, you can buy field flatteners which will compensate for the coma anyway. The astigmatisms value is explaining the error between the symmetrical curvature of the lens. Basically, no lens will be perfectly symmetrical, the lower the astigmatism, the more symmetrical the lens surface is.

Javier Moreno about his product: "A mirror fulfils its function, but I wanted to create a mirror with more to offer than that. Usually, the last glimpse of everyone before leaving the house is the one in the mirror. So why don't dropping all the small necessary things we need before we leave the house there?" The T-2 flange focal distance is standardized – even a mirrorless camera needs 55mm with a standard T-ring. We'd recommend to use these two clamps and to determine the focus position of the eyepiece. You shouldn't need to insert it completely into upper port, as that clamp is shorter. If desired, you can add T-2-extensions later to get to the right distance. Or you focus your telescope now with the cameras to find out how much the focus differs between eyepiece and cameras, then you can determine the required T-2-extensions in advance. The problem is that the focus point of a cross hair eyepiece is often different to that of a standard 1.25" eyepiece.

The Flip Mirror itself has got T-2-threads on both ends. For use with Barlow and ADC, it is probably the best if you use T-2-eyepiece clamps on both ports. There are several clamps available: https://www.baader-planetarium.com/en/accessories/adapters-imaging-accessories/eyepiece-clamps.html?filter_threads_lenssided=536 As the position of the ADC should be orientated on the horizon, it is better to use a clamp than to screw it directly onto the FlipMirror without an option to rotate it.



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