Scientific American Supplement, No. 358, November 11, 1882Various
Science
Scientific American Supplement, No. 358, November 11, 1882
Various
Science -- Periodicals
With regard to the time of exposure: we must again impress upon the
student the necessity for placing the sitter as close to the window
as can be conveniently done, for then he will receive the strongest
illumination; and, no matter how strong the shadows which may be
produced, they can always be modified sufficiently by the judicious use
of the reflector. Of course, in practice there is a limit as to the
closeness the sitter can be placed, inasmuch as if too near there will
not be room enough for the background. As we have before said, the
effective light falling upon the sitter is governed by the amount of
direct skylight to which he is exposed. For experiment, let any one seat
himself, say, one foot from the window and sideways to it, and note the
amount of sky that can be seen from this position, then take a seat six
feet within the room, and note it from thence. The difference will be
very marked indeed, and it will fully account for the long exposure that
some have found imperative.
In our previous articles we directed special attention to the advantage
accruing from arranging the sitter in such a position that he received
as much direct light as possible, so that it practically helps to soften
the shadows; hence the sitter should be placed so that he is turned as
little away from the source of light as will enable the desired view of
the face being obtained. That this may the more advantageously be done
the camera should always be placed as close as possible to the side
wall in which the window is situated. As an experiment illustrating the
advantage of this: let a camera be placed close to the wall, then the
sitter arranged so that from that point of view a three-quarter face is
obtained, and it will be noticed that there is very little need of the
reflector at all. Let a negative now be taken, and the camera brought,
say, five feet into the room, and the sitter, without changing his seat,
turned round until a similar view of the face is obtained from that
point. It will now be seen that the shadows are very much deeper than
before, and the reflector will have to be brought pretty close in order
to overcome them; nevertheless they may be obtained quite as soft and
harmonious as in the former case. Let a second negative now be taken,
giving the same exposure as before, and it will be found that if
the first one were correctly timed the second will be considerably
under-exposed. Yet the sitter was at the same distance from the window
in each case.
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