PST 加左價?!
- david_kmng
- 白矮星
- 文章: 960
- 註冊時間: 週五 11 7月, 2003 00:10
- 來自: 草根階層
Thanks!
Just know that narrower bandwidth will yield higher resolution for solar imaging...
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umm...
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then for DSO photography, will the imaging with the narrow band filter yield higher resolution when comparing the imaging from scope with same aperature boardband or no filter?
Or the light from DSO is already so narrow in bandwidth hence the difference between is not much...
However, for solar imaging then there are still a lot of area to explore with the narrow band filter!!!
Just know that narrower bandwidth will yield higher resolution for solar imaging...
......
...
umm...
...
then for DSO photography, will the imaging with the narrow band filter yield higher resolution when comparing the imaging from scope with same aperature boardband or no filter?
Or the light from DSO is already so narrow in bandwidth hence the difference between is not much...
However, for solar imaging then there are still a lot of area to explore with the narrow band filter!!!
- david_kmng
- 白矮星
- 文章: 960
- 註冊時間: 週五 11 7月, 2003 00:10
- 來自: 草根階層
For Ha solar viewing or imaging, the objective is to isolate the Ha from the continuous spectrum, so the narrower the bandwidth, the clearer you can see what's happening on the Chromosphere.
For DSO imaging, the need is on collecting enough photons with an adequate image scale. In most situations, the imaging scale is usually well below the diffraction limit. So, the resolution is mainly depending on the focal length of the optical system.
For DSO imaging, the need is on collecting enough photons with an adequate image scale. In most situations, the imaging scale is usually well below the diffraction limit. So, the resolution is mainly depending on the focal length of the optical system.
The reason why I think this is ...
Generally speaking, a telescope's resolution is governed by the diameter of the telescope. True for planets, DSOs.
However, for solar imaging seems there is also one important/dominate factor, that is the bandwidth filtering. The narrower the bandwidth, the higher the resolution, otherwise the details are SMEARED and even FLUSHED by the flood of the wide spectrum of white light.
Just wild guess... Can we also improve the resolution of planets, DSOs imaging by also using narrow bandwidth filter?
Are we using the highest res. capability of our scope already?
Generally speaking, a telescope's resolution is governed by the diameter of the telescope. True for planets, DSOs.
However, for solar imaging seems there is also one important/dominate factor, that is the bandwidth filtering. The narrower the bandwidth, the higher the resolution, otherwise the details are SMEARED and even FLUSHED by the flood of the wide spectrum of white light.
Just wild guess... Can we also improve the resolution of planets, DSOs imaging by also using narrow bandwidth filter?
Are we using the highest res. capability of our scope already?
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