Andy Resnick said:
That's correct- atmospheric turbulence can be modeled as a slowly-varying (in time & space) phase-only object, over the timescales and length scales of most imaging systems (thin screen model). Long exposures tend to show uniform blurring, while shorter exposures become sharper.
Borek said:
As explained earlier - it doesn't have to be camera motion.
It won't hurt to check how the lens performs in good light and with short times - at 300 mm rule of thumb says to use time 1/300 sec. Make it 1/500 (300 mm * 1.6 = 480 mm) and try to shot some distant object. Take a look at 1:1 crop then.
For whatever reason, I spent the past hour banging my head against my desk trying to generate some numbers. Here's what I came up with:
First, using focal lengths of 300mm, 1000mm, and 1500mm on an APS-C sensor gives equivalent focal lengths of 480 mm, 1600mm, and 2400 mm, corresponding to magnifications of 9.6, 32, and 48 (assuming the back focal length of a Rebel T2i is the 35mm film standard).
I chose an f/# of 8, corresponding to an aperture diameter D of 0.125*(focal length). The angular resolution is given as sin(theta) = 1.22 l/D, where l is the wavelength. Choosing green light (0.5 micron), the angular resolution of the lenses is:
480mm -> 0.34 arcmin
1600 mm -> 0.1 arcmin
2400 mm -> 0.07 arcmin
(the human eye can distinguish about 1 arcmin at best).
Ok- now the effect of turbulence. Using a model for 'Good seeing conditions' gives a spatial correlation time of 10 ms and a correlation length of 7.7 cm. That is, exposures longer than the correlation time give time-averaged effects, while short exposures do not.
The long-time effect is fairly straightforward to calculate- the effect is to blur the image. Given the correlation length of 7.7 cm as compared to aperture diameters of 0.125*F decreases the cutoff frequency f as:
480 mm -> f' = 0.8 f
1600mm -> f' = 0.5 f
2400mm -> f' = 0.3 f
This means that taking into account the atmospheric effects, the angular resolution has been decreased to 0.43 arcmin, 0.2 arcmin, and 0.2 arcmin: going from a 1000mm to a 1500mm lens will not increase the resolvable information.
This is for 'good seeing'- calm weather. The HV-54 model (Hufnagel-Valley model with a 54 mph upper atmospheric wind) gives a correlation length of 4.2 cm, which will degrade the image a lot more than you expect: the resolution limits are now 0.5 arcmin, 0.4 arcmin, and 0.5 arcmin- empty magnification kicks in at the 300mm lens (and possibly at shorter lenses).
Short time effects are considerably more complicated, but involve 'speckle imaging'. Exposures must be very short- 1 ms or less- for this to be seen.