Lunt LS80THA solar scope.

The Lunt LS80THA on top of the C11 EdgeHD.
Figure 1: The Lunt LS80THA on top of the C11 EdgeHD.
Piggy-back on the Celestron C11 XLT EdgeHD rides a Lunt LS80THA pressure tuned single stack etalon solar telescope. The Lunt is used both for visual observations using the standard Lunt zoom-eyepiece and for solar imaging (for examples see the Solar system (Main) page of this website).
In basic principle the etalon consists of two parallel glass plates with a small air gap in between. By changing this air gap one can influence which wavelengths are being cancelled out or magnified. For this there are two methods available: tilting and pressure tuning. When tilting the gap changes width in direction the light passes through it. Using a pressure tuner, like on my Lunt LS80THA, the gap is changed by increasing the pressure in the gap between the glass plates. As a result the gap widens, affecting other frequencies.
Over time this pressure leaks away, but by turning the pressuriser until it detaches the pressure can be reset and the etalon pressurised again.


The Lunt LS80THA ready for imaging with a 4x barlow and monochrome camera.
Figure 2: The Lunt LS80THA ready for imaging with a 4x barlow and monochrome camera.
At the observer end of the telescope a star diagonal contains a B1200 blocking filter. When imaging I use a TeleVue 2″ 4x PowerMate Barlow to image details of the sun. To be able to focus, the Barlow must come after the blocking filter. Lunt supplies straight-through housing blocking filters that allow to have the Barlow and camera in line with the telescope, but it is expected that most users will use a diagonal blocking filter just like I have. Adding a Barlow and camera to the diagonal looks a bit funny, but works just fine.
In order to connect a Barlow to the diagonal, Lunt supplies a special adapter ring that can be threaded onto the blocking filter, a much more affordable solution than a second straight-through blocking filter. The adapter is attached by unscrewing the 1.25″ eyepiece holder is first, after which the 2" Barlow adapter ring can be mounted. Once it is in place, the Barlow is inserted and, using a 2″ to 1.25″ adapter, the camera (I use a ZWO ASI174MM for the purpose) is inserted into it.


If you have any questions and/or remarks please let me know.


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