Bernoulli, Daniel
,
Hydrodynamica, sive De viribus et motibus fluidorum commentarii
Text
Text Image
Image
XML
Thumbnail overview
Document information
None
Concordance
Notes
Handwritten
Figures
Content
Thumbnails
Table of Notes
<
1 - 3
[out of range]
>
[Note]
Page: 204
[Note]
Page: 207
[Note]
Page: 210
[Note]
Page: 214
[Note]
Page: 218
[Note]
Page: 220
[Note]
Page: 227
[Note]
Page: 229
[Note]
Page: 234
[Note]
Page: 235
[Note]
Page: 236
[Note]
Page: 243
[Note]
Page: 247
[Note]
Page: 248
[Note]
Page: 250
[Note]
Page: 251
[Note]
Page: 258
[Note]
Page: 258
[Note]
Page: 266
[Note]
Page: 267
[Note]
Page: 268
[Note]
Page: 268
[Note]
Page: 272
[Note]
Page: 277
[Note]
Page: 279
[Note]
Page: 279
[Note]
Page: 287
[Note]
Page: 289
[Note]
Page: 290
[Note]
Page: 293
<
1 - 3
[out of range]
>
page
|<
<
(238)
of 361
>
>|
<
echo
version
="
1.0RC
">
<
text
xml:lang
="
la
"
type
="
free
">
<
div
xml:id
="
echoid-div252
"
type
="
section
"
level
="
1
"
n
="
194
">
<
pb
o
="
238
"
file
="
0252
"
n
="
252
"
rhead
="
HYDRODYNAMICÆ
"/>
<
p
>
<
s
xml:id
="
echoid-s7027
"
xml:space
="
preserve
">(IV) Quod maximam oſtendit auræ elaſticitatem eſt experimentum ter-
<
lb
/>
tium cum tormento nondum decurtato ſumtum, quod indicat aſcendere
<
lb
/>
potuiſſe globum accepto impetu ad altitudinem α = 58750 ped. </
s
>
<
s
xml:id
="
echoid-s7028
"
xml:space
="
preserve
">Angl. </
s
>
<
s
xml:id
="
echoid-s7029
"
xml:space
="
preserve
">Erat
<
lb
/>
autem longitudo animæ A G ſeu a = 7, 7: </
s
>
<
s
xml:id
="
echoid-s7030
"
xml:space
="
preserve
">longitudo A C (quantum ex
<
lb
/>
amplitudine animæ & </
s
>
<
s
xml:id
="
echoid-s7031
"
xml:space
="
preserve
">gravitate pulveris pyrii conjicio) erat = 0, 08. </
s
>
<
s
xml:id
="
echoid-s7032
"
xml:space
="
preserve
">De-
<
lb
/>
nique valor ipſius P (ſeu ponderis columnæ mercurialis, cujus baſis ſit cir-
<
lb
/>
culus maximus globi & </
s
>
<
s
xml:id
="
echoid-s7033
"
xml:space
="
preserve
">cujus altitudo ſit 30. </
s
>
<
s
xml:id
="
echoid-s7034
"
xml:space
="
preserve
">poll. </
s
>
<
s
xml:id
="
echoid-s7035
"
xml:space
="
preserve
">Angl. </
s
>
<
s
xml:id
="
echoid-s7036
"
xml:space
="
preserve
">ratione ponderis glo-
<
lb
/>
bi ferri deſignati per unitatem) invenitur poſita gravitate ſpecifica inter mer-
<
lb
/>
curium & </
s
>
<
s
xml:id
="
echoid-s7037
"
xml:space
="
preserve
">ferrum ut 17 ad 10 = 26, 8: </
s
>
<
s
xml:id
="
echoid-s7038
"
xml:space
="
preserve
">Et cum per §. </
s
>
<
s
xml:id
="
echoid-s7039
"
xml:space
="
preserve
">III. </
s
>
<
s
xml:id
="
echoid-s7040
"
xml:space
="
preserve
">ſit proxime n =
<
lb
/>
α: </
s
>
<
s
xml:id
="
echoid-s7041
"
xml:space
="
preserve
">(b P log {a/b}) erit n = 6004. </
s
>
<
s
xml:id
="
echoid-s7042
"
xml:space
="
preserve
">Unde ſequitur, ſi aura pulveris pyrii inflamma-
<
lb
/>
ti elaſticitatem habeat ſuæ denſitati proportionalem, eſſe illius maximam ela-
<
lb
/>
ſticitatem minimum ſexies millies majorem elaſticitate aëris ordinarii.</
s
>
<
s
xml:id
="
echoid-s7043
"
xml:space
="
preserve
"/>
</
p
>
<
p
>
<
s
xml:id
="
echoid-s7044
"
xml:space
="
preserve
">(V) At vero ſi jam conſideremus partem auræ inutilem, quæ avolat per
<
lb
/>
lumen accenſorium & </
s
>
<
s
xml:id
="
echoid-s7045
"
xml:space
="
preserve
">hiatum à globo relictum, majorem elaſticitatem inve-
<
lb
/>
niemus: </
s
>
<
s
xml:id
="
echoid-s7046
"
xml:space
="
preserve
">Calculus qui ad hanc quæſtionem ſolvendam requiritur, cum non
<
lb
/>
parum prolixus atque intricatus ſit, non hæſitavi hypotheſes adhibere paul-
<
lb
/>
lo liberiores, quibus admodum facilitatur: </
s
>
<
s
xml:id
="
echoid-s7047
"
xml:space
="
preserve
">quamvis ipſæ hypotheſes non
<
lb
/>
ſint omni rigore veræ, errorem tamen notabilem producere non poſſunt.
<
lb
/>
</
s
>
<
s
xml:id
="
echoid-s7048
"
xml:space
="
preserve
">Primo ponam utramque aperturam, per quam aura evolare poſſit, eſſe ve-
<
lb
/>
luti infinite parvam ratione animæ amplitudinis; </
s
>
<
s
xml:id
="
echoid-s7049
"
xml:space
="
preserve
">hoc poſito poterit ſingulis
<
lb
/>
momentis velocitas, cum qua aura avolat, æſtimari immediate ex preſſione
<
lb
/>
ſola: </
s
>
<
s
xml:id
="
echoid-s7050
"
xml:space
="
preserve
">hujusmodi autem hypotheſin ſine ullo ſenſibili errore fieri poſſe pro
<
lb
/>
omni fluido, tunc etiam cum foramina non ſunt admodum exigua, paſſim
<
lb
/>
ut corollarium ex theoria noſtra deduximus, & </
s
>
<
s
xml:id
="
echoid-s7051
"
xml:space
="
preserve
">multo facilius aſſumi poſſe in
<
lb
/>
fluido valde elaſtico facile quisque videbit ex eo, quod incrementum aſcen-
<
lb
/>
ſus potentialis ratione motus interni longe minus eſt ratione aſcenſus potentialis
<
lb
/>
particulæ per foramen exilientis in fluido, quod à propria elaſticitate ex-
<
lb
/>
pellitur, quam quod gravitatis vi ejicitur: </
s
>
<
s
xml:id
="
echoid-s7052
"
xml:space
="
preserve
">in priori enim minor eſt motus
<
lb
/>
localis internus quam in altero. </
s
>
<
s
xml:id
="
echoid-s7053
"
xml:space
="
preserve
">Secundo auræ pulveris pyrii inflammati vim
<
lb
/>
elaſticam tantam eſſe, ut niſus atmoſphæræ contrarius attendi non mereatur: </
s
>
<
s
xml:id
="
echoid-s7054
"
xml:space
="
preserve
">
<
lb
/>
tertio velocitatem globi in tormento utut permagnam, tamen minimam cen-
<
lb
/>
ſeri poſſe ratione velocitatis, qua aura per hiatum utrumque avolat, quia
<
lb
/>
nempe inertia iſtius auræ non poteſt non admodum eſſe exigua ratione </
s
>
</
p
>
</
div
>
</
text
>
</
echo
>