What's the main difference between the LS60MT and LS50THa?
The LS60MT has a larger 60mm aperture for higher resolution and is a modular system that can be converted for nighttime use. The LS50THa is a dedicated 50mm solar telescope. Both use an internal pressure-tuned etalon.
Do I really need a double-stack filter?
For the highest-contrast views of solar surface detail, yes. A single-stack system is excellent for prominences on the Sun's edge, but a double-stack dramatically enhances the visibility of filaments and plage on the disk itself by narrowing the bandpass.
Why choose the B1200 blocking filter over the B600?
The B1200 provides a larger, fully illuminated field of view. This is important for imagers using cameras with larger sensors to avoid vignetting, and it provides a more comfortable visual experience with low-power, wide-field eyepieces.
What kind of mount do I need for the Lunt LS60MT?
A lightweight, stable alt-azimuth mount like the Sky-Watcher AZ-GTe or a small equatorial mount is sufficient. The telescope is relatively light, but a solid platform is crucial for the fine focusing and tracking needed for solar observation.
Can I use my regular nighttime eyepieces with this telescope?
Yes. In solar mode the B1200 blocking filter, in a 1.25" diagonal housing, takes standard 1.25" eyepieces. At night the 2" focuser has a 2" compression ring and an included 1.25" adapter, so it accepts both 2" and 1.25" eyepieces. The included zoom eyepiece is a versatile starting point, but high-quality planetary or wide-field eyepieces can enhance the view further.
Is pressure tuning better than tilt tuning?
Pressure tuning provides a more uniform view across the entire field because it doesn't tilt the etalon. This avoids creating an off-band gradient from one side of the image to the other. It is generally considered a more advanced and consistent tuning method.