以下是引用huangwy在2007-10-4 5:19:05的发言:I was using a monochrome camera. I think i was unable to see the details because the sunspot was quite small.  
reviously, when I take images of other larger sunspots, the details could be seen quite clearly. Note: the image below was taken with a DSLR using the baader herschel wedge.

This gives the explanation!
I am also using Baader Herschel solar wedge prism for white light observation and photography, it gives the best detail image of photosphere.
For hydrogen alpha observation in the chromosphere, I also use Coronado's double stack etalon. I am using one SolarMax 90 at the front and one etalon at the back of the telescope to obtain <0.5A performance. Both etalons were matched by Coronado in order to achieve the specification (both etalons offset a little bit for peak center frequency performance). This configuration has advantage of better weight balance as SM90 is very heavy and will affect balance when both is attached to the front of the telescope. Besides, this configuration also has better control of internal reflection as the etalon are widely separated. However, the disadvantage is a specific cocentric optics has to be tailor made by Coronado for the telescope (in my case Takahashi SKY90) such that rays pass through the second etalon perpendicularly.
I understand you are using BF10 blocking filter. Have you ask Coronado to modify it for photographic use. The standard BF10 has the band selection filter installed at the nose piece and the infra-red rejection filter at the eyepiece end of the diagonal. I am using both BF15 and BF30, the BF15 have a diagonal and consume a lot of back focus which would affect use of DSLR. Coronado provides a custom solution of installing both band selection and infra-red rejection filters at the nosepiece such that it can mount to a T2 adapter for DSLR.
For the calcium K-line observation at the inner chromospere, I am using Coronado CaK 70 telescope.
[此贴子已经被作者于2007-10-4 13:14:48编辑过]