CHAPTER V

ENLARGING BY ARTIFICIAL LIGHT

The apparatus for enlarging with artificial light is, as has been stated,

more expensive than that for use with daylight. The negative box and

screen, however, remain as given. But we need in addition two extra

pieces, a light-box and a pair of condensing lenses.

The form of light-box presupposes the choice of illuminant, and in this

there is a wide range. Suffice it to say that a kerosene lamp with one or

more one-and-a-half inch burners will be found suitable for very small

work or weak negatives. For larger work or stronger negatives a stronger

light will be needed.

Of these, the first in point of strength is the arc-light, which is too

strong for ordinary negatives to be enlarged not more than fourfold on

ordinary bromide paper. Used with any of the slower papers it will be

found very serviceable and satisfactory. Next comes the lime-light, which

has pretty much the same advantages and disadvantages. After these come

acetylene, a gas giving an intense light of high actinic power. This is

within the reach of nearly all, as a first-class generator costs only

about twelve dollars, and the uses of the gas are manifold. The same

generators and burners can be used with a projecting lantern and will be

found far more satisfactory than oil. Acetylene burners can be had in

various sizes, ranging in power from thirty to several hundred

candle-power. The carbide from which the gas is generated is not expensive

and costs only a few cents each time the machine is loaded. By an

adjustment attached to the generator the gas is kept at a constant

pressure, and hence the light is unusually steady. All in all this light

has many advantages. After it in strength comes the Welsbach burner,

suitable for those having gas in the house. After this comes the ordinary

gas-burner, and then oil. The reader, knowing now what will be required of

his light, can take his choice.

Perhaps the simplest form of light-box is where the light is placed in one

room and the enlarging done in an adjoining one, the light being admitted

through a suitable opening. This prevents the possibility of stray light

reaching the paper and is productive of no additional heat in a room

presumably already hot enough.

If this is not feasible a light-box must be constructed. As these vary so

much in material and design, and must be altered with different forms of

light in use, I will merely state the requirements. First of these is that

it must be light-tight, and second, that it must have adequate ventilation

and be fire-proof. Following these in importance, there should be a simple

arrangement for looking at the light from time to time to see that it is

burning properly and some means for readily attending to it if it is not.

Having the light-box, the burners must be placed in it properly. Here the

shortest way out of the difficulty is to go to an expert. If electricity

is used go to an electrical supply house; if gas, go to a gas-fitter. As

will be seen later the flame itself must be placed in a certain relation

to other portions of the apparatus, and provision must be made

accordingly.

In looking over the magazines and annuals we will now and then see some

new method given for illuminating evenly the back of a negative in

enlarging or reduction. The most of these the writer has tried, but he has

never found one of them which could be relied upon to give even reasonable

satisfaction. If the light is apparently evenly diffused it is too weak.

If strong enough it is not evenly diffused. Hence I will recommend nothing

short of a pair of condensing lenses, as these have been proved by

experience to be satisfactory in every respect if properly handled and

cared for. The diameter of these must be slightly greater than the

diagonal of the largest negative from which enlargements are to be made.

These can be bought in pairs, mounted or unmounted, at about the following

prices:

---------+-----------------+----------------+------------------

Diameter | Focus | Pair of Lenses | Per Single Lens

Inches | Inches | Mounted | Unmounted

---------+-----------------+----------------+------------------

4 | 5-1/2 or 6-1/2 | $ 4.00 | $ 1.25

4-1/2 | 5-1/2 or 6-1/2 | 6.00 | 1.50

5 | 6-1/2 | 7.50 | 1.75

6 | 8 | 12.00 | 3.00

8 | 12 | 32.00 | 7.50

9 | 14 | 40.00 | 10.00

---------+-----------------+----------------+------------------

The prices asked for condensers vary considerably in different

price-lists. They can often be had at second-hand at a decided saving of

expense.

If it is desired to save the additional cost of the mounted condensing

lenses, they can be comparatively easily mounted by anyone at all familiar

with tools in the following manner:

A piece of quarter-inch pine or poplar is cut to a square about an inch

larger than the diameter of the lenses. In the center of this is sawed out

a circular opening the exact size of the lens. In another board of the

same dimensions is cut a circle a quarter of an inch less in diameter.

These boards are placed together with the grain running in opposite

directions, to prevent warping, and the lens kept in place by a wire bent

in a circle and clamped in place so as to hold the lens, or other similar

arrangement. See Fig. 8. The other lens is mounted in the same way. The

two are mounted with their convex sides facing each other and a slight

distance apart. It is better to place between them a thin sheet of finely

ground glass, as this overcomes the bad effects of slight flaws in the

lenses, which are not uncommon. The combination is then boxed up.

[Illustration: Fig. 8]

Having now our light-box, condensers, negative box, camera and screen,

they are next arranged in the order shown by Fig. 9. A long table

especially constructed for the purpose makes the best base for this

purpose.

In putting the apparatus together there are several points to be noticed.

First, the planes of the lenses, negative, projecting lenses and screen

must all be parallel; second, the centers of all these should be in a

single straight line, and third, either the light or the condensers should

be so mounted as to easily slide backward or forward, since every time the

projecting lens is racked backward or forward it necessitates a

corresponding motion of the condensers to or from the light.

[Illustration: Fig. 9]

In constructing the apparatus, for use with condensers and artificial

light, the same provision should be made in the negative box for inserting

a piece of colored or ground glass as was made in the daylight apparatus.

When the diameter of the condensers is but little greater than the

diagonal of the negative it will be necessary to have the latter quite

close to the former, as the cone of light from the condensers has its apex

at the lens, and hence if the negative in such a case is at a distance

from the condensers the corners will receive no light. Reference to Fig. 9

will show this plainly. For this and other reasons it is always best to

have the condensers of ample size for a given negative. In fact, before

beginning to make enlargements the worker should work with one good

negative until he finds out exactly what light-intensity is best suited to

it. This will then serve as a standard for all other negatives of the same

general grade, and variations of the light can be made as required for

particular negatives, or where the extent of enlargement is materially

changed for various purposes.

In using the daylight apparatus, which we will now consider, the negative

is placed in the holder opposite the center of the ground-glass, upside

down and facing into the work room. The room is darkened and lens

uncapped. An image more or less blurred will appear on the screen. If the

enlarged picture is to be only slightly larger than the negative, the lens

must be racked out until its distance from the negative is but little less

than its distance from the screen. To make the enlargement greater we

simply rack back the lens and move the screen further off. There are

tables which show exactly the distance which the lens must be from the

negative and screen in order to get an enlargement of a given size: The

table here inserted covers the ordinary requirements and may be of service

in constructing the apparatus:

TIMES OF ENLARGEMENT

Total distances from the negative, in inches.

-------------+---------------+-----------------+-----------------+-----------------

Times of | 2 | 3 | 4 | 6

Enlargement | | | |

-------------+-------+-------+--------+--------+--------+--------+--------+--------

Focus of | To | To | To | To | To | To | To | To

Lens | Easel | Lens | Easel | Lens | Easel | Lens | Easel | Lens

-------------+-------+-------+--------+--------+--------+--------+--------+--------

6 inches | 27 | 9 | 32 | 8 | 37-1/2 | 7-1/2 | 49 | 7

8 " | 36 | 12 | 42-2/3 | 10-2/3 | 50 | 10 | 65-1/3 | 9-1/3

10 " | 45 | 15 | 53-1/3 | 13-1/3 | 62-1/2 | 12-1/2 | 81-2/3 | 11-2/3

12 " | 54 | 18 | 64 | 16 | 75 | 15 | 98 | 14

-------------+-------+-------+--------+--------+--------+--------+--------+--------

A table for enlargements of from one to twenty-five times, with lenses

varying in focal length from three to nine inches is here given.

ENLARGEMENTS

_From the British Journal of Photography Almanac._

+----------+-----------------------------------------------------------------------+

| Focus of | |

| Lens | Times of Enlargement and Reduction |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| Inches | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 |

| | inch | inches | inches | inches | inches | inches | inches | inches |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 3 | 6 | 9 | 12 | 15 | 18 | 21 | 24 | 27 |

| | 6 | 4-1/2 | 4 | 3-3/4 | 3-3/5 | 3-1/2 | 3-3/7 | 3-3/8 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 3-1/2 | 7 | 10-1/2 | 14 | 17-1/2 | 21 | 24-1/2 | 28 | 31-1/2 |

| | 7 | 5-1/4 | 4-2/3 | 4-3/4 | 4-1/5 | 4-1/12 | 4 | 3-9/10 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 4 | 8 | 12 | 16 | 20 | 24 | 28 | 32 | 36 |

| | 8 | 6 | 5-1/3 | 5 | 4-4/5 | 4-2/3 | 4-4/7 | 4-1/2 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 4-1/2 | 9 | 13-1/2 | 18 | 22-1/2 | 27 | 31-1/2 | 36 | 40-1/2 |

| | 9 | 6-3/4 | 6 | 5-3/5 | 5-2/5 | 5-1/4 | 5-1/7 | 5-1/16 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 5 | 10 | 15 | 20 | 25 | 30 | 35 | 40 | 45 |

| | 10 | 7-1/2 | 6-2/3 | 6-1/4 | 6 | 5-5/6 | 5-5/7 | 5-5/8 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 5-1/2 | 11 | 16-1/2 | 22 | 27-1/2 | 33 | 38-1/2 | 44 | 49-1/2 |

| | 11 | 8-1/4 | 7-1/3 | 6-4/5 | 6-1/2 | 6-5/12 | 6-2/7 | 6-3/10 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 6 | 12 | 18 | 24 | 30 | 36 | 42 | 48 | 54 |

| | 12 | 9 | 8 | 7-1/2 | 7-1/5 | 7 | 6-6/7 | 6-3/4 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 7 | 14 | 21 | 28 | 35 | 42 | 49 | 56 | 63 |

| | 14 | 10-1/2 | 9-1/3 | 8-3/4 | 8-2/5 | 8-1/6 | 8 | 7-7/8 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 8 | 16 | 24 | 32 | 40 | 48 | 56 | 64 | 72 |

| | 16 | 12 | 10-2/3 | 10 | 9-3/5 | 9-1/3 | 9-1/7 | 9 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

| 9 | 18 | 27 | 36 | 45 | 54 | 63 | 72 | 81 |

| | 18 | 13-1/2 | 12 | 11-1/4 | 10-4/5 | 10-1/2 | 10-2/7 | 10-1/8 |

+----------+------+--------+--------+--------+--------+---------+--------+---------+

The object of this table is to enable any manipulator who is about

to enlarge (or reduce) a copy any given number of times to do so

without troublesome calculation. It is assumed that the photographer

knows exactly what the focus of his lens is, and that he is able to

measure accurately from its optical center. The use of the table

will be seen from the following illustration: A photographer has a

_carte_ to enlarge to four times its size, and the lens he intends

employing is one of 6 inches equivalent focus. He must therefore

look for 4 on the upper horizontal line and for 6 in the first

vertical column, and carry his eye to where these two join, which

will be at 30-7-1/2. The greater of these is the distance the

sensitive plate must be from the center of the lens; and the lesser,

the distance of the picture to be copied.

In practice it is convenient, after having once found the focus for a

given enlargement from a given negative with the lens in use, to mark on

the base of the apparatus the point to which the lens has been extended.

Then in making future enlargements of the same size, it is only necessary

to set the lens at that point and move the easel backward or forward until

an approximate focus is obtained, when the image will be of the proper

size on the screen.

As an approximate guide it is sufficient to know that the nearer the lens

is to the negative the greater will be the enlargement, as may be seen in

Fig. 7. If a piece of thin cardboard, or a sheet of paper cut to the exact

size of the enlargement desired, is placed upon the easel-screen, little

difficulty will be experienced in getting an enlarged image of the proper

size and correctly focused.

It is advisable to focus the enlargement with the largest aperture of the

lens. If the lens, when working at its largest aperture, covers the plate

from which the enlargement is being made, it will give proper definition

over the enlargement. With a lens of the better sort, of course, the

definition will be equally good whether a large or small aperture is used;

but with a low-priced lens it is better to stop down to No. 8 (f/11.3) or

No. 16 (f/16), to avoid spherical aberration. Stopping the lens down

increases the time of exposure, and enables one to have greater control

over the operation of exposing the paper, permitting time to shade or

locally increase the exposure at any portion of the image. This is

sometimes useful, but as a general thing stopping the lens down is not

advisable, as interfering with one's judgment in calculating exposures for

various negatives. Having secured the image correct in size and focus,

place thumb-tacks at all four sides of the sheet of paper or card used to

focus the image. These will serve as a guide to the placing of the

sensitive paper. Adjust the lens stop as desired and cap the lens, leaving

the room totally dark save for such safe light as we may have for working.

Place the bromide paper on the screen, using the thumb-tacks as a guide to

the correct position in this.

In making his first enlargements, the beginner should avail himself of the

help of test-strips. These should be about one inch wide and the length of

the paper. The exposure depends on a number of factors, among which are

light, negative, focal length of lens, size of enlargement, stops,

sensitiveness of paper, developer, temperature of developer, and length of

development. The first experiment had best, therefore, be made on a purely

arbitrary basis, for which we will take ten seconds.

Pinning a test-strip on the screen, we uncap the lens and with a piece of

cardboard shade two-thirds of the strip during five seconds; move the

cardboard, and give the next section five seconds making ten for the

first; then remove the cardboard entirely and give five seconds more,

making fifteen for the first, ten for the second, and five for the third.

Now develop the strip. If the fifteen seconds portion finishes development

in less than one minute, and the ten takes approximately a minute, we will

know that our basis was correct. But if all three were over-exposed or

under-exposed, as shown by one minute's development, we can expose the

next test-strip accordingly.

In determining the correct exposure, the method already set forth for

contact exposures is a reasonably good one. If the paper with a given

exposure takes half the proper time to develop, halve the next exposure;

if double the time, or more, double it. More could be said on the subject

of exposure, and possibly to advantage; for instance, there are tables

showing the exact relation of exposure to the number of times of

enlargement, but complicated calculations in the dark-room are troublesome

and a test-strip is simpler. After a while one gets the ability to

determine the approximate exposure required by looking at the enlarged

image on the screen, correcting slight errors by length of development,

and greater ones by modifying the developer by diluting or strengthening.

It should be remembered, however, that in judging exposure by reference to

the screen, we must consider the high lights, as well as the shadows. It

is in the high lights that we need the detail if we are to have soft

pictures. If this detail in the high lights is plentiful and clear we may

know that our light is strong enough for a very short exposure. If it is

very faint, we will have to give a long exposure and use diluted developer

to save the over-exposed shadows. On the other hand, if the image on the

screen is a flat one, we may know that our light is too strong for the

negative, and it must be modified by removing the reflector or by

interposing ground or yellow glass; and if neither of these suffice, we

can simply lay the negative aside for a dark day when the light will be

very much weaker. Frequently all necessary contrasts can be obtained by

the use of the _hard_ paper before referred to. As under-exposure tends to

increase contrasts, we should also give the minimum exposure in the case

of flat negatives, abandoning for a time our standard one-minute

development. As will be seen by this time, there are many wrinkles about

using bromide paper, and it will be found that new ones appear at every

_seance_ in the enlarging room.

But why is it that so many of our enlargements are black in the shadows

and chalky in the high lights? Why, simply because our light is too weak

for our negative. We forget that if we cannot modify our negative we must

modify our light. It is this characteristic of the bromide enlargement

which has prevented the process from enjoying the popularity it deserves.

And I sometimes wonder whether this chalkiness is due to the use of the

north light!

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