Bernoulli, Daniel
,
Hydrodynamica, sive De viribus et motibus fluidorum commentarii
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SECTIO DECIMA.
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ertiæ quæ globo ineſt: </
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<
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">vi iſtius hypotheſeos avolabit aura per utramque aper-
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turam eadem velocitate, cum alias poſita velocitate in lumine accenſorio
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= √ A, & </
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<
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xml:space
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">velocitate globi = v, velocitas auræ in hiatu a
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globo ad ſuperfi-
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ciem animæ relicto dicenda eſſet = √ A - v. </
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<
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<
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xml:space
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">(VI) Primo notandum eſt, ſi elaſticitates auræ cenſeantur denſitatibus
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proportionales, fore ut aura
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conſtanter eadem velocitate per utramque
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aperturam avolet, uti vidimus in problemate §. </
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<
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<
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xml:space
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">iſtaque velocitas no-
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minatim talis erit, quæ generetur ab altitudine auræ homogeneæ, cu-
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jus pondus auram captam coërcere poſſit, ne ſe expandat. </
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<
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xml:space
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minabitur dicta velocitas hoc modo: </
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<
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xml:space
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">ſit gravitas globi = 1, elaſticitas
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ſeu pondus quod auram pulveris modo inflammati A C D B in illo com-
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preſſionis ſtatu coërcere poſſit = P: </
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<
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xml:space
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">pondus pulveris adhibiti = p;
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</
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<
s
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xml:space
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">erit pondus auræ pulveris modo inflammati etiam = p: </
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<
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xml:space
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">ſique lon-
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gitudo A C ponitur = b, patet altitudinem auræ homogeneæ, quæ pondus
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P habeat, fore = {P/p} b; </
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<
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xml:space
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">Igitur velocitas quacum aura recens nata per lumen
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accenſorium avolat eſt = √({P/p} b), eademque velocitate durante tota ex-
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ploſione ejicietur, idque non ſolum per lumen accenſorium, ſed & </
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<
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per hiatum inter globum & </
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<
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<
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</
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<
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<
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xml:space
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">(VII) Sit nunc porro amplitudo animæ = F; </
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<
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">hiatus interceptus inter
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globum & </
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<
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xml:space
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">animam = f: </
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<
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">amplitudo luminis accenſorii = Φ: </
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<
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xml:space
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">longitudo ani-
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mæ = a, quantitas auræ ab initio exploſionis = g. </
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<
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xml:space
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">Intelligatur deinde glo-
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bus perveniſſe ex E in e, dicaturque A C = x: </
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">quantitas auræ eo temporis
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puncto in tormento reſidua = z: </
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<
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">velocitas globi in iſto ſitu = v, reliquæ de-
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nominationes fuerunt jam antea explicatæ.</
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</
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<
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<
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xml:space
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">Quoniam elaſticitas per hypotheſin eſt directe ut quantitas & </
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<
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xml:space
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ce ut ſpatium, erit elaſticitas auræ in A c d B reſiduæ = {zb/gx} P: </
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<
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">quæ quidem
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non tota in propellendum globum impenditur, ſed tantum pars ejus, quæ
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ſe habeat ad totam ut F - f ad f. </
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">Eſt itaque poſito d t pro elemento temporis
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dv = {F - f/F} X {zb/gx} P X dt.
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</
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<
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">Per methodum autem §. </
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<
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effluens ſpecifice definita fuit, </
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