Clavius, Christoph
,
In Sphaeram Ioannis de Sacro Bosco commentarius
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Comment. in II. Cap. Sphæræ
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lis in Ecliptica ad diem propoſitum, eiusq́. </
s
>
<
s
xml:id
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echoid-s11722
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xml:space
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">declinationẽ ex tabula ſuprap oſita.
<
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</
s
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<
s
xml:id
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echoid-s11723
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xml:space
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">Nám Solis declinatio, ſi fuerit Borealis, vt quando Sol in ſignis Borealibus
<
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♈, ♉, ♊, ♋, ♌, & </
s
>
<
s
xml:id
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xml:space
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">♍, exiſtit, detrahenda erit ab altitudine meridiana Solis,
<
lb
/>
vt habeatur altitudo A equatoris, ſeu@ (quod idẽ eſt) altitudo meridiana Solis,
<
lb
/>
quam haberet in æquinoctijs: </
s
>
<
s
xml:id
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echoid-s11725
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xml:space
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">Hac enim dempta ex 90. </
s
>
<
s
xml:id
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echoid-s11726
"
xml:space
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">grad. </
s
>
<
s
xml:id
="
echoid-s11727
"
xml:space
="
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">relinquetur eleuæ
<
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tio poli. </
s
>
<
s
xml:id
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echoid-s11728
"
xml:space
="
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">Vt Romæ anno M D L X I X. </
s
>
<
s
xml:id
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echoid-s11729
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xml:space
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">& </
s
>
<
s
xml:id
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echoid-s11730
"
xml:space
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">die XX. </
s
>
<
s
xml:id
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echoid-s11731
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xml:space
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">Iulij, exiſtente Sole in grad. </
s
>
<
s
xml:id
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echoid-s11732
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xml:space
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<
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/>
6. </
s
>
<
s
xml:id
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echoid-s11733
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xml:space
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">min. </
s
>
<
s
xml:id
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echoid-s11734
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xml:space
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">40. </
s
>
<
s
xml:id
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echoid-s11735
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xml:space
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">♌, quæ quidem declinant in Boream ab Aequatore grad. </
s
>
<
s
xml:id
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echoid-s11736
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xml:space
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">18. </
s
>
<
s
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xml:space
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">min. </
s
>
<
s
xml:id
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echoid-s11738
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">
<
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39. </
s
>
<
s
xml:id
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echoid-s11739
"
xml:space
="
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">ut ex tabula declinationum cõ@tat; </
s
>
<
s
xml:id
="
echoid-s11740
"
xml:space
="
preserve
">inueni in meridie altitudinem Solis cõ
<
lb
/>
tinere grad. </
s
>
<
s
xml:id
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echoid-s11741
"
xml:space
="
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">66. </
s
>
<
s
xml:id
="
echoid-s11742
"
xml:space
="
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">min. </
s
>
<
s
xml:id
="
echoid-s11743
"
xml:space
="
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">39. </
s
>
<
s
xml:id
="
echoid-s11744
"
xml:space
="
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">De traho ex hac declinationem, nempe gr. </
s
>
<
s
xml:id
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echoid-s11745
"
xml:space
="
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">18. </
s
>
<
s
xml:id
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echoid-s11746
"
xml:space
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">min. </
s
>
<
s
xml:id
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echoid-s11747
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xml:space
="
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">39. </
s
>
<
s
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echoid-s11748
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">
<
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remanent 48. </
s
>
<
s
xml:id
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echoid-s11749
"
xml:space
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">gr. </
s
>
<
s
xml:id
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echoid-s11750
"
xml:space
="
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">pro altitudine Aequatoris, qua ablata ex 90. </
s
>
<
s
xml:id
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echoid-s11751
"
xml:space
="
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">grad. </
s
>
<
s
xml:id
="
echoid-s11752
"
xml:space
="
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">relinquitur
<
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/>
altitudo poli gr. </
s
>
<
s
xml:id
="
echoid-s11753
"
xml:space
="
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">42. </
s
>
<
s
xml:id
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echoid-s11754
"
xml:space
="
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">Si vero declinatio Solis fuerit Auſtralis, ut quando Sol
<
lb
/>
ſigna Auſtralia ♎, ♏, ♐, ♑, ♒, & </
s
>
<
s
xml:id
="
echoid-s11755
"
xml:space
="
preserve
">♓, percurrit, eritea adijcienda altitudini
<
lb
/>
Solis meridianæ, ut inueniatur altitudo Aequatoris; </
s
>
<
s
xml:id
="
echoid-s11756
"
xml:space
="
preserve
">Nam hac ablata ex 90. </
s
>
<
s
xml:id
="
echoid-s11757
"
xml:space
="
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">
<
lb
/>
grad. </
s
>
<
s
xml:id
="
echoid-s11758
"
xml:space
="
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">remanebit eleuatio poli, ut prius. </
s
>
<
s
xml:id
="
echoid-s11759
"
xml:space
="
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">Vt Romæ eadem anno M D L X I X. </
s
>
<
s
xml:id
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echoid-s11760
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xml:space
="
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">ac
<
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die XXI. </
s
>
<
s
xml:id
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xml:space
="
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">Nouembris, Sole commorante in grad. </
s
>
<
s
xml:id
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xml:space
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">9. </
s
>
<
s
xml:id
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xml:space
="
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">& </
s
>
<
s
xml:id
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xml:space
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">min. </
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>
<
s
xml:id
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"
xml:space
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">20. </
s
>
<
s
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xml:space
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">♐, quæ diſcedunt
<
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ab Aequatore in Auſtrum, ut docet tabula declinationum, gr. </
s
>
<
s
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xml:space
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">21. </
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<
s
xml:id
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">min. </
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>
<
s
xml:id
="
echoid-s11769
"
xml:space
="
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">54. </
s
>
<
s
xml:id
="
echoid-s11770
"
xml:space
="
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">de-
<
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/>
prehendi altitudinem Solis meridianam grad. </
s
>
<
s
xml:id
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echoid-s11771
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xml:space
="
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">26. </
s
>
<
s
xml:id
="
echoid-s11772
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xml:space
="
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">min. </
s
>
<
s
xml:id
="
echoid-s11773
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xml:space
="
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">6. </
s
>
<
s
xml:id
="
echoid-s11774
"
xml:space
="
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">cui ſi addatur declinæ
<
lb
/>
tio, puta grad. </
s
>
<
s
xml:id
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echoid-s11775
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xml:space
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">21. </
s
>
<
s
xml:id
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xml:space
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">min. </
s
>
<
s
xml:id
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echoid-s11777
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xml:space
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">54. </
s
>
<
s
xml:id
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xml:space
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">colligetur altitudo Aequatoris grad. </
s
>
<
s
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echoid-s11779
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xml:space
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">48. </
s
>
<
s
xml:id
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echoid-s11780
"
xml:space
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">ex qua iterũ
<
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inuenitur ele@a tio poli 42. </
s
>
<
s
xml:id
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echoid-s11781
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xml:space
="
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">grad. </
s
>
<
s
xml:id
="
echoid-s11782
"
xml:space
="
preserve
">Aliam rationem inueniendæ altitudinis poli
<
lb
/>
ex Analemmate quolibet die, etiamſi declinatio Solis ignota ſit, tradidi in ſe-
<
lb
/>
cundo ſcholio. </
s
>
<
s
xml:id
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echoid-s11783
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xml:space
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">propoſ. </
s
>
<
s
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xml:space
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">28. </
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<
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xml:id
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echoid-s11785
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xml:space
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">lib. </
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<
s
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xml:space
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">1. </
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<
s
xml:id
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xml:space
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">Gnomonices.</
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<
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</
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<
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<
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<
emph
style
="
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">Qvoniam</
emph
>
vero, ut recte inueniatur altitudo poli, præciſe in puncto
<
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<
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xlink:label
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note-316-01
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xlink:href
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note-316-01a
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xml:space
="
preserve
">Meridiana
<
lb
/>
linea, qua
<
lb
/>
arte inue
<
lb
/>
niat@r.</
note
>
meridiei accipienda eſt altitudo Solis, quòd tum demum fiet, cum umbra
<
lb
/>
gnomonis præciſe in lineam meridianam proijcietur, nõ abs re fuerit, paucis
<
lb
/>
indicare, qua arte linea meridiana indagari debeat: </
s
>
<
s
xml:id
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xml:space
="
preserve
">quoniam ad multas obſer-
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lb
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uationes Aſtronomorum neceſſaria eſt. </
s
>
<
s
xml:id
="
echoid-s11791
"
xml:space
="
preserve
">In plano igitur ad libellam cõſtructo,
<
lb
/>
quod nimirum Horizonti ſit parallelum, deſcribantur plurimi circuli ex eo-
<
lb
/>
dem cẽtro E, in quo erigatur ſtylus, ſeu gnomon E F, ad angulos rectos, quod
<
lb
/>
tum fiet, quando eius cacumen F, æqualiter remotum fuerit à circunferentia
<
lb
/>
cuiuslibet circuli in plano propoſito ex centro E, deſcripti. </
s
>
<
s
xml:id
="
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xml:space
="
preserve
">Erit aurem æqua-
<
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liter remotũ, ſi à tribus ſaltem punctis circumferentiæ æqualiter diſtiterit, ut
<
lb
/>
lib. </
s
>
<
s
xml:id
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xml:space
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">4. </
s
>
<
s
xml:id
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xml:space
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">Gnomonices propoſ. </
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<
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xml:space
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">12. </
s
>
<
s
xml:id
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xml:space
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">demonſtrauimus. </
s
>
<
s
xml:id
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"
xml:space
="
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">Deinde ante meridiem obſer-
<
lb
/>
uetur extremitas umbræ, donec ad amuſſim circumferentiam alicuius circuli
<
lb
/>
tãgat, qualis eſt umbra E G, cuius extremitas præciſe in circumferentiam ter-
<
lb
/>
tij circuli cadit. </
s
>
<
s
xml:id
="
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xml:space
="
preserve
">Rurſus poſt meridiem notetur umbræ extremitas, donec in
<
lb
/>
circumferentiam eiuſdem circuli cadat præciſe, cuiuſmodi eſt umbra E H.
<
lb
/>
</
s
>
<
s
xml:id
="
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"
xml:space
="
preserve
">Vt autem ſcias, qua hora poſt meridiem umbræ extremitas circumferentiam
<
lb
/>
eiuſdem circuli @angere poſſit, (ne fruſtra ad Solem accedas) obſeruandæ
<
lb
/>
erunttot horæ poſt meridiem, quot horis ante meridiem umbram notaſti. </
s
>
<
s
xml:id
="
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"
xml:space
="
preserve
">Nã
<
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/>
@i v. </
s
>
<
s
xml:id
="
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xml:space
="
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">g. </
s
>
<
s
xml:id
="
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"
xml:space
="
preserve
">tertia hora ante meridiem extremitas umbræ tang it pręciſe circunferẽ-
<
lb
/>
tiã alicuius circuli, neceſſe eſt, ut tertia hora poſt meridiem eiuſdem circuli
<
lb
/>
circumferentiã contingat umbræ extremitas. </
s
>
<
s
xml:id
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echoid-s11803
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xml:space
="
preserve
">Quod quidẽ multo certius ſcies
<
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/>
hac ratione. </
s
>
<
s
xml:id
="
echoid-s11804
"
xml:space
="
preserve
">Quãdo umbræ extremum cadit ante meridiẽ præciſe in circum-
<
lb
/>
ferentiam alicuius circuli, inueſtigetur aliquo inſtrumento altitudo Solis@ quę
<
lb
/>
diligenter notata, quando poſt meridiem eandem Sol obtinebit altitudinem,
<
lb
/>
certiſſime tibi perſuadeas, tunc umbrã extremã eiuſdem circuli circumferen-
<
lb
/>
tiam attingere: </
s
>
<
s
xml:id
="
echoid-s11805
"
xml:space
="
preserve
">Quoniam eadem proportione poſt meridiem altitudo Solis di
<
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/>
minuitur, qua accreſcit ante meridiẽ, & </
s
>
<
s
xml:id
="
echoid-s11806
"
xml:space
="
preserve
">idcirco qua proportione umbra </
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>
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