USING CCD CAMERAS

                         
                         


     Connections & Interfacing

     Video out is generally BNC with cased cameras. Use only 75 ohm cable and 
   make sure equipment to interface with takes 1V p-p neg sync video. Note 
   that unless otherwise specified, a camera supplies only baseband video 
   and audio. You CANNOT connect the camera directly to the cable input or
   antenna terminals of a TV set and expect a picture. A VIDEO INPUT jack is
   required as well as an AUDIO INPUT jack. Many TV sets have these inputs, 
   as do VCRs and Camcorders. They are usually standard RCA type jacks. A
   shielded cable with RCA male connectors can be used for audio, but the
   video will need a BNC male (UG88) at one end and an RCA male at the other
   end. For short runs <10 ft. you can use shielded audio cable with two
   male RCA plugs and a BNC-RCA adapter but 75 ohm coax is to be preferred for
   longer runs. The video cable should be matched to avoid reflections
   and ghosting. DC is 12-14 volts CLEAN with little ripple and noise. Case 
   is generally negative and center pin is positive.

     Board cameras usually come with flying color coded leads with connectors
   to mate with the PC board. Follow wiring diagrams exactly.

   Precautions: Cased cameras and board cameras

    If your camera uses it, USE ONLY supplied wall transformer, NO OTHER, or 
   the camera may be damaged. Many wall transformers are poorly regulated and 
   produce 50% to 75% more voltage under light load conditions. This may 
   destroy your camera instantly beyond repair.

     A battery pack may be used if an fuse is installed in series with the 
   hot (generally positive or +) supply lead. Fuse should be rated no more 
   than twice the camera current drain. A protection diode such as a 1N4007
   should be installed in series with the battery supply to guard against 
   accidental reverse polarity due to incorrect wiring or transients from 
   other devices sharing the supply.

   DO NOT reverse supply leads even momentarily as this will destroy the cir-
   cuitry in the camera. 
   
   AVOID strong RF fields and static electricity. If used with a transmitter
   bypass all leads and keep camera away from antenna. Ferrite beads and a
   few 100 pf or 0.001 mfd disc capacitors can be used. Remember that the 
   video output impedance is 75 ohms and that a 470 pf disc capacitor will
   have about this much reactance at 4.5 MHz, so keep video bypasses less
   than about 220 pf. Also watch out for ferrite beads causing excessive loss
   at higher video frequencies. Cameras can be enclosed in shields made from
   cardboard or heavy paper covered with adhesive backed .0015" copper foil 
   if weight is a problem. This can be found at craft and hobby shops.

   DO NOT point camera at very bright lights or the sun. Keep lens covered 
   when camera is not being used.

   NEVER, NEVER attempt to clean CCD device or touch it with finger. It is
   static sensitive. Keep body cap on lens opening when no lens is installed.

   For cased cameras, DO NOT force lens threads as the aluminum housing has 
   a fine thread that strips very easily. Check for dirt or burrs before 
   installing lens. If resistance is encountered find out why. Again the lens 
   should turn effortlessly, DO NOT FORCE it, or you may jam the lens or strip 
   the threads. Treat the camera as you would a fine photographic camera and 
   you should have few if any problems.

   Board cameras should be mounted with small hardware and should not have any 
   strain on the circuit board. Use nylon hardware if possible or use fiber 
   washers with metal hardware as a strain relief.

   CCD camers using fixed lenses may be focused if necessary by using a fine 
   jewelers screwdriver to loosen the lens mounting screws, then sliding the 
   lens as needed, while monitoring the video on a monitor or oscilloscope, 
   adjusting lens for maximum detail(preferred method) or high frequency 
   content as seen on an oscilloscope. In most cases, CCD board cameras are 
   focused at the factory and need no adjustment.
                                                             

    Applications and hints for CCD cameras

   Standard Wratten photo filters may be used over the lens for effects

   B/W cameras have infrared sensitivity and a Wratten #87 filter can be used 
   to allow only infrared radiation to pass. Sensitivity is near IR region 
   out to about 1050-1100 nanometers. 

   A cyan or green filter will correct excessive red sensitivity to yield a
   more "natural" tonal scale as the human eye would see. A Wratten #11, 
   #38, #58, or #61 filter can be obtained from a dealer in photographic 
   supplies, or a piece of transparent green plastic can be used, if it 
   is optically suitable. Optical suitability can be determined as follows
   If it does not distort your vision in any way, and moving the plastic or
   glass filter in front of the eye causes no movement, blurring, or any
   distortion of an image to be noticed, it is probably OK for use. A #11 
   filter is a very common item and is recommended for general use. A coated 
   filter is best if available as it helps to reduce reflections. Tiffen
   or B+W brands are recommended.

     Color cameras have built in filtering to correct the high red and IR 
   sensitivity and therefore will show much less sensitivity to IR. This is
   a necessary compromise for correct color rendition. B/W cameras are 
   therefore best for IR and low light work.

   A standard camera tripod may be used as a mount. For cased cameras, thread 
   1/4-20 screw NO MORE than four threads (0.200 inches) into the camera body.
   
       Light source can be anything handy, or available daylight. Flourescent 
   tends to be red light deficient and has little IR component, and may not be 
   as good in low light situations (<1 lux) as tungsten light. A standard 10 
   to 100 watt clear or frosted bulb is an excellent source for this camera. 
   For battery powered applications a 12V tungsten or quartz halogen lamp 
   can be used. Avoid contrasty situations for best results.

     Cased cameras many times use C or CS mount lenses much like a 35 mm SLR
   camera. This permits use of various lenses for different applications.
   To adjust infinity focus for a lens, mount lens to be used. Connect up a 
   monitor and set up the camera to point at a distant object (> 20 ft). 
   Set the lens to infinity focus, with iris wide open (if applicable). On
   back of camera typically there is a slotted shaft, knob, or other arrange-
   ment. Turn with fine tip screwdriver or other suitable tool as needed until
   image on monitor is sharpest with lens set at infinity. Check at near
   distances to make sure near focus is OK. If needed, you can set this for
   close focusing if infinity focus is not necessary. With short focus lenses
   (4 or 6 mm) depth of field is tremendous, a few inches to infinity. 
     A T to C adapter can be used to mount other lenses. Also, a 1.25" adapter 
   can be used to connect this camera to an astronomical telescope. 
   
      Video Astronomy with CCD cameras

      A CCD camera can be mounted at the prime focus of a telescope, either a 
   refractor or a reflector. A C mount to 1.25 inch adapter can be used with 
   cased cameras. For board cameras, the camera could be mounted in a housing 
   so that the assembly slips into the focusing tube in place of the eyepiece
   and arranged so the CCD sensor is placed at the focal plane. The moon  
   shows up very well and depending on the telescope aperture, many stars can 
   be seen. The camera is quite sensitive and is useable for some video observations. 
   The same setup can be used for terrestrial observation and nature
   studies or surveillance applications. A VCR, VTR, or camcorder may be used 
   to directly record observations if desired. Note that the image of a star
   in a good telescope will be a fine point of light, and since a star cannot
   be resolved into a disc, the optical quality, seeing conditions, and aperture 
   of the scope determine the size of the point. Better scopes produce smaller
   points of light with little light present in the diffraction rings that 
   surround the star image. In this case, the amount of light picked up is
   proportional to the aperture of the scope. It is possible that this point of 
   light could fall between pixels on the CCD sensor. This is not a problem 
   with finite size images as is the usual case, so do not expect the CCD to 
   perform as well with stars as with planetary or lunar images. Also keep in 
   mind the inherent red and IR sensitivity of the CCD. Still, excellent 
   astronomical views may still be had with appropriate optics.

   If a TV set with no video input is all that is available, use a video modulator
   such as cat # MODU between camera and set. The video and audio are
   fed to the modulator and the modulator output connected to the ANTENNA
   terminals of the TV set. The video will appear on VHF CH3 or CH4. Note that 
   the modulator needs DC power, typically 9V at 50 mA.

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