Making a light box became a necessity when I began subtracting dark frames
from my images and then, on
careful examination, could still spot other
marks that only flat field frames could remove.
I searched the internet but few sites mentioned how they had made their light
boxes. Other alternatives to produce a flat frame did not seem appropriate for
my use, i.e. dome, twilight or sky flats.
Don Goldman at Astrodon.com
gives instructions and a plan for the light box he had made - mine is a near copy
of Don's. The light box is a 14" cube for my Meade LX200GPS - note
that the OTA for the 10" telescope has a diameter of 12".
I obtained three sheets of foam-board from my local artists shop but could not find a supplier for the translucent plastic until I suddenly realised that most shop-front signs have acres of the stuff - a local sign maker cut me two off-cuts to size for £1 each.
The image to the left shows an edge-on picture of the foam board.
The
design puts two squares of white translucent plastic, separated by about
4", at the telescope end of the light box. Cutting the board with
craft knife was easy: the most difficult operation was making the round hole to
fit the dew shield which is permanently mounted onto my telescope. I sealed the
exposed edges of this aperture with a coating of glue to stop any foam
fragments landing on the objective when the light box is used.
The
sides of the box were secured with white 'gaffer' tape; separators and locating
supports within the box were glued to the sides to secure the plastic sheets in
place.
As you can see from the work-in-progress shots, I left the green protection covers on the plastic sheets till the last moment of assembly.
I adapted the corner templates from the plan in Don's drawing: the angle
between the equal sides of equilateral triangle I made between 45o -
60o.
Two corner deflectors were glued in place to give the box some rigidity and then the control box was glued to the outside and the cables to the LEDs routed around the outside of the box to their respective corners.
The LEDs were glued through holes to small foam board squares glued below the corner deflectors.
The
electronic control box was made from similar parts to that defined by Don on his
site, Astrodon.com.
I mounted the lot in a plastic box and used telephone cable for the runs to the
LEDs. The parts were available in the UK from Maplin
Electronics.
I bought a rotary potentiometer with an on/off switch to save a installing separate on/off switch.
The parts list from Maplin Electronics included the following parts:
| Maplin Code # | |
| FW41 | Sw Pot Lin 4k7 |
| CK65 | PP3 Batt Box |
| D120R | 2W Res 120R |
| FP18 | 100pk TieWrp 203/2.5 |
| HF28 | PP3 Clip |
| JP42 | Small PSU Grommet |
| NR73 | 5mm White 1800mcd -----------LEDs |
| RX01 | Knob NK2 |
| UK14 | LED Clip Convex 5mm |
| YA12 | Duracell Ultra PP3 |
| LH20W | ABS Box MB1 |
When the
light box interior was complete and the LEDs proved to be functioning correctly,
the green protective light plastic sheet was removed from the translucent
plastic sheet and the box top was secured in place with white gaffer tape.
Effort was made to ensure the box was sealed to prevent dust and dirt from
entering.
The box was then mounted
onto the telescope - I have secured the light box to
the telescope when it is used by a couple of heavy elastic bands from two small
coat hooks glued to the top corners of the box to two of the plastic screws used
to secure the dew shield to OTA. A further elastic band secures the lower side
to the third screw on the dew shield.
Following the instructions in The
Handbook of Astronomical Image Processing by Berry & Burnell, I adjusted
the potentiometer to half-fill the photosites on my CCD with a 10 second
exposure. I have marked this position on the control box and use it as the
standard for my flat field exposures.
An
early attempt to use the light box for flat field production showed the
tell-tale dirt 'doughnuts'.
I found that exposing for 10 seconds and using 30% of the potentiometer
resistance gave me the required 50% photosite saturation levels.