The Crystelliptometer An Instrument for the Polariscopic Analysis of Very Slend
The Crystelliptometer An Instrument for the Polariscopic Analysis of Very Slend
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In our eReader you can find the full English version of the book. Read The Crystelliptometer An Instrument for the Polariscopic Analysis of Very Slend Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book The Crystelliptometer An Instrument for the Polariscopic Analysis of Very Slend
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& R. S. I. , VI and rows +2, 1, etc. , the other way, through a certain amount a, so that now the coordinates of S are x a, y = -fa (a being neg- ative). These changes are shown in Fig. 9. 12 Introducing the above values of s, q, x, and y into (13), and resuming m = tan 0, we get [~\ r T r~ n 45+ -180 cos -360 +cos 45 -f -180 5 J La J L 8 _r [a "1 fa ~| 45 + - 180 sin -360, 1 Fa T ' (18) L = sin 45 + - 180 sin ^360, L 5 J Id J P = sin|45 H-^ 180 |cosfo60] -tan (9 cos|45H-- 180 1. L d J La J L S... J While the attention is, indeed, fixed on one particular spot 5, 5 Fig. 9, whose coordinates are a and -fa, yet in actual practice it is expedient to make measurements on a number of spots, usually twenty or more, and deduce the position of S from them. Refer- ring to Fig. 9, it is clear that the abscissa of any spot in the nth vertical column (numbered along the bottom of the figure) is d (19) which gives n By measuring the abscissas of several spots in different rows, thus varying x and n, we obta'n as many independent observa- tions upon a.
What to read after The Crystelliptometer An Instrument for the Polariscopic Analysis of Very Slend?
You can find similar books in the "Read Also" column, or choose other free books by Le Roy D Le Roy Dougherty Weld to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
& R. S. I. , VI and rows +2, 1, etc. , the other way, through a certain amount a, so that now the coordinates of S are x a, y = -fa (a being neg- ative). These changes are shown in Fig. 9. 12 Introducing the above values of s, q, x, and y into (13), and resuming m = tan 0, we get [~\ r T r~ n 45+ -180 cos -360 +cos 45 -f -180 5 J La J L 8 _r [a "1 fa ~| 45 + - 180 sin -360, 1 Fa T ' (18) L = sin 45 + - 180 sin ^360, L 5 J Id J P = sin|45 H-^ 180 |cosfo60] -tan (9 cos|45H-- 180 1. L d J La J L S... J While the attention is, indeed, fixed on one particular spot 5, 5 Fig. 9, whose coordinates are a and -fa, yet in actual practice it is expedient to make measurements on a number of spots, usually twenty or more, and deduce the position of S from them. Refer- ring to Fig. 9, it is clear that the abscissa of any spot in the nth vertical column (numbered along the bottom of the figure) is d (19) which gives n By measuring the abscissas of several spots in different rows, thus varying x and n, we obta'n as many independent observa- tions upon a.
What to read after The Crystelliptometer An Instrument for the Polariscopic Analysis of Very Slend?
You can find similar books in the "Read Also" column, or choose other free books by Le Roy D Le Roy Dougherty Weld to read onlineMoreLess
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