Mcanique Cleste volume 2
Mcanique Cleste volume 2
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S' nearly, we have -4' — ^ = — ^ [2733/]. The mean of [2760a] these two values, using [2578a, &€. ], is 4, ' — ^ = ^ . Tv A cos. S' -j ;- i = tv=:the mean synodical motion. [27606] Therefore if we take as many tides in the equinoxes as in the solstices, we may suppose the mean synodical motion, after the maximum. , to be 4^' — 4'j and before it, 4-' — 4'; so that 2 . (4'' — -4) is nearly equal to the synodical motion, in the whole interval [2761]. [2760c] 764 THEORY OF THE TIDES COMPARED WITH T...HE [Mcc. C^l.
the middle of the interval comprised between these observations ; therefore [2761] we may suppose 2. (V — J. ) to be equal to the sjnodical motion of the moon during this interval [2760c]. Moreover, the hour of the greatest tide [2762] is determined by the equation* w ^ -f -. — — x := [2479c] ; therefore [2762'] 2. (nt'-^r - — ^ — ^) is the retardation of the tide, in the interval comprised between the observations. This retardation, estimated in degrees, supposing the whole circumference 400° to correspond to one day, being put equal to fA, we shall have, t Ratio of the lunar Xv and solar — -tj- forces.
What to read after Mcanique Cleste volume 2?
You can find similar books in the "Read Also" column, or choose other free books by Pierre Simon Laplace to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
S' nearly, we have -4' — ^ = — ^ [2733/]. The mean of [2760a] these two values, using [2578a, &€. ], is 4, ' — ^ = ^ . Tv A cos. S' -j ;- i = tv=:the mean synodical motion. [27606] Therefore if we take as many tides in the equinoxes as in the solstices, we may suppose the mean synodical motion, after the maximum. , to be 4^' — 4'j and before it, 4-' — 4'; so that 2 . (4'' — -4) is nearly equal to the synodical motion, in the whole interval [2761]. [2760c] 764 THEORY OF THE TIDES COMPARED WITH T...HE [Mcc. C^l.
the middle of the interval comprised between these observations ; therefore [2761] we may suppose 2. (V — J. ) to be equal to the sjnodical motion of the moon during this interval [2760c]. Moreover, the hour of the greatest tide [2762] is determined by the equation* w ^ -f -. — — x := [2479c] ; therefore [2762'] 2. (nt'-^r - — ^ — ^) is the retardation of the tide, in the interval comprised between the observations. This retardation, estimated in degrees, supposing the whole circumference 400° to correspond to one day, being put equal to fA, we shall have, t Ratio of the lunar Xv and solar — -tj- forces.
What to read after Mcanique Cleste volume 2?
You can find similar books in the "Read Also" column, or choose other free books by Pierre Simon Laplace to read onlineMoreLess
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