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e 29 I<br />

firft ill a ads PoGtion to it, that it might a.gairI<br />

r&a& the beam of the Sun’s Light which came<br />

to it through the firit Prifrn. In the firit Prifrn<br />

this beam was refratted UPWS~S, and in the<br />

fecond meways. And I found that by the H$efsatlion<br />

of thc’kcond Prifnl the breadth of the<br />

Image was not increafcd, but its fuperior part<br />

which in the firii: Priftn MTered the greater<br />

RefracGon and appeared violet and blue, did<br />

again jn the fecond Priiin fuEer 8. greater RefraAion<br />

than its inferior part, which appeared<br />

red and yellow, and this without any Dilatation<br />

of the Image in breadth.<br />

lhjhz~io~~. Let S [in Fz$. p.s.1 reprefent<br />

the Sun, F the hole in the “WmdoWY AI3C the<br />

firfi Priiin, D .H the fecoud Prifm, ‘1’ the round<br />

Image of the Sun made by a direct beam of<br />

Light wheu the Prifms are taken air-ay3 PT<br />

the oblong Image of the Sun made by that beam<br />

paihng through the firit Prifin alone when the<br />

fecond Prifin is taken away, and p t the Image<br />

made by the crofs RefraAions of both Prilixs<br />

together. Now if the Rays which tend towards<br />

the feveral Points of the round ImageY<br />

were dilated and fpread by the Refra&ion c$<br />

.the firit Psih, fo that they ihsuld not any lon-<br />

\ ger go in iingle Lines to fingle Points, but that<br />

,cvery Ray being @lit, fhattered, and changed<br />

from a Linear Ray to a Superficies of Rays diverging<br />

from the Poiuk of Refraction,’ and lying<br />

in the P!.nnc of the Angles of Incidence and<br />

Kefra&ion, they fhould go in thofe Planes to<br />

fo many Lines reaching alrnoik from one end of<br />

the Image PT to the other, and if that Image<br />

dllOUlCj#

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