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STANDARD - Survey Instrument Antique Center!

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81<br />

Transit Solar Attachment.<br />

For running Meridian or other lines by the Sun.<br />

Written for tnis catalogue with special reference to the wants of Public Land <strong>Survey</strong>ors, for both common and<br />

mineral lands, by J. B. DAVIS, Assistant Professor of Civil Engineering,<br />

University of Michigan.<br />

1. Remarks. The attachment herein referred to is the Davis and Berger<br />

solar screen, prism, and colored shade glass, used for direct solar observation.<br />

These inventions have been devised by the Mr. Berger, of the firm of C. L. Berger<br />

& Sons, and by the writer. They are simply for the purpose of enabling one<br />

to make an observation directly upon the sun's centre. This observation being<br />

secured by readings of the horizontal and vertical circles, is reduced so as to<br />

give the direction of the line of sight of the transit at the instant of the observation.<br />

Thus knowing the direction of the line of sight at a given instant it becomes<br />

simply necessary to turn off the angle which this line of sight makes with the<br />

meridian, to ascertain the position of the meridian. This angle is what is obtained<br />

by reducing the observation, as above mentioned. A brief reference to the history<br />

of these devices will best explain them. It occurred to the writer to see if an image<br />

of the sun could be formed behind the eye-piece of a telescope at the same time<br />

an image of the cross-wires was, and the latter image be made to quarter the<br />

former, by allowing the sun to shine into the object end of the telescope and thence<br />

directly through it. The experiment was made by holding a piece of white paper<br />

behind the eye-piece, and adjusting the focus of the eye-piece and object glass.<br />

The very first trial was readily successful. The next thing was to see if the position<br />

of the instrument could be located by this means as near as the circles would<br />

read. By the same simple means it was soon found that a motion given to the<br />

telescope by either tangent screw might be so slight that the eye could not detect<br />

it upon the circles, but evidence of it would be apparent in the position of the images<br />

with reference to each other. This fact at once settled the question of whether<br />

this would be a sufficiently delicate means of observation. It showed that the<br />

observations would be closer than the circles would read. After some trials and<br />

some months rest these facts were brought to the notice of others, and finally were<br />

submitted to Mr. Berger for his opinion. He made a screen \vhich the writer<br />

exhibited at the first annual convention of the association of Michigan Engineers<br />

and <strong>Survey</strong>ors at Lansing. The matter was further studied by Mr. Berger. The<br />

screen was much improved, and the mechanical construction of it brought to<br />

the standard of the work done by this firm. Mr. Berger soon conceived the<br />

idea of making the screen of ground white glass in a brass frame, as shown in<br />

figs. 1 and 2,*so one might observe the position of the images directly upon it,<br />

and thus secure not only the comfort of an easy position in observing, but the<br />

consequent accompanying accuracy. The arm of attachment was perfected from<br />

time to time. The screen of ground glass is mounted upon an arm that admits of<br />

all adjustments of position, and is so attached to the side of the telescope tube that<br />

it can be turned up out of the way when not needed. The reflecting prism<br />

can be screwed on to the eye-piece cap for observing at high altitudes. This also is<br />

adjustable so as to look in any desired direction from the telescope tube. The<br />

diagonal eye-piece also has its movable colored shade glass<br />

as above stated. With<br />

these attachments observations on the sun at all altitudes may be made in two<br />

ways. By looking directly at it through the simple colored glass for low altitudes,<br />

or through the prism and its shade glass for high altitudes. The other way is to<br />

receive on the screen the images of the cross-wires and the sun and make the image<br />

of the cross-wires just quarter the image of the sun by means of the slow motion<br />

screws to the circles of the instrument. For this method the colored shade glasses<br />

are not to be used. With this complete outfit one may work whichever way seems<br />

bwst.<br />

* For Figures 1, 2, 3, 4, 5, 6 and 7 see page 175.

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