Dear Raymond,
If your TEC-140 refractor already have had a "curved" field, then a true flat field eyepiece is not the solution. What you need is an optical device that has an "opposite" curvature to offset the TEC defects. It is hard to tell specifically what is this optical device, since we do not know the magnitude and orientation of the curvature (positively or negatively curved, and by how much?). The best way is by "try and error" until you feel comfortable with the trial.
I recall that years ago before film technology declined, Pentax produced the "XP" series flat-field projection eyepiece. This, of course, assumed the preceding optics before XP is ideal. I still got a sample XP (3.8 mm), but I think it is not suitable for a trial with TEC now.
My preference is to use the Powermate Barlow instead of an eyepiece. Powermate has wider lens aperture than the typical short focal length eyepiece, hence less risk of curved field and dark frame corners. If 4X Barlow is not enough, you can cascade like 3X + 2X for 6X, or add an extension tube between Barlow & CCD. I sometimes do this way. However, there are always two limitations:
1. Seeing --- You may get even worse result if seeing is not supportive.
2. Nyquist sampling theory --- It says that the optimum sampling is obtained when a lunar feature of angular size equal to your telescope resolution (~0.8 arcsecond for TEC-140) just covers 2 pixels of your CCD. So be careful that the EFL (effective focal length) of your telescope is controlled below a value in order to fit Nyquist. By my experience, EFL = f/30 is probably approaching the Nyquist threshold, assuming best seeing. Perhaps you could use f/35 at most. At less favorable seeing, EFL better kept below f/20 ~f/30. I am not sure the size of one pixel in Canon 5D, so no exact mathematics can tell now. Best is experiment on your own.
My 2 cents. Please take above as reference only, as one's medicine could turn out to be another man's poison.
AC
[ 本帖最後由 mca 於 2009-6-11 23:18 編輯 ] |