Mathematical Tracts on the Lunar and Planetary Theories, the Figure of the Earth, Precession and Nutation, the Calculus of Variations, and the Undulatory Theory of Optics: Designed for the Use of Students in the UniversityMacmillan and Company, 1858 - 400 sider |
Inni boken
Resultat 1-5 av 47
Side 30
... { ( 2 — 2m ) 2 — 1 } Or , taking the last term to the second order only , u = 3k'a m'a'3 cos 2 ( 0 ― y ) k'a α - 4 2h2a3 + ae cos ( 0 - a ) - m'a's + has cos ( ( 2-2m ) 0 — 2ß } . - m ' To take away we observe that a ' 30 LUNAR THEORY .
... { ( 2 — 2m ) 2 — 1 } Or , taking the last term to the second order only , u = 3k'a m'a'3 cos 2 ( 0 ― y ) k'a α - 4 2h2a3 + ae cos ( 0 - a ) - m'a's + has cos ( ( 2-2m ) 0 — 2ß } . - m ' To take away we observe that a ' 30 LUNAR THEORY .
Side 31
... observe that a ' and a are nearly the h2 27 reciprocals of ' and p , which occur in ( 38 ) : and , since m ' 2 3 - m2.5 = P 37 m'a'3 we have m'a'3 = m2 . μ . a3 ; 13 = h2a3 - m2 . H = m2a . Thus , the value of u becomes a [ 1-9 32 - m2 ...
... observe that a ' and a are nearly the h2 27 reciprocals of ' and p , which occur in ( 38 ) : and , since m ' 2 3 - m2.5 = P 37 m'a'3 we have m'a'3 = m2 . μ . a3 ; 13 = h2a3 - m2 . H = m2a . Thus , the value of u becomes a [ 1-9 32 - m2 ...
Side 43
... observed , will be approximately repre- sented by k sin ( gey ) , where g differs little from 1 ; the differ- ence , which is caused entirely by the disturbing force , being of the second order . d's do2 Hence , + s , or k ( 1 − g3 ) ...
... observed , will be approximately repre- sented by k sin ( gey ) , where g differs little from 1 ; the differ- ence , which is caused entirely by the disturbing force , being of the second order . d's do2 Hence , + s , or k ( 1 − g3 ) ...
Side 49
... observe that { ( 1 - m ) 0 - ẞ } ( Article 48 ) is nearly the dif ference of longitude of the Sun and Moon , and consequently , cos { ( 2-2m ) 0-2ẞ } is greatest , when the Moon is in syzygies , and least ( or has its greatest negative ...
... observe that { ( 1 - m ) 0 - ẞ } ( Article 48 ) is nearly the dif ference of longitude of the Sun and Moon , and consequently , cos { ( 2-2m ) 0-2ẞ } is greatest , when the Moon is in syzygies , and least ( or has its greatest negative ...
Side 57
... observed ( amounting , at its maximum , to 122 " ) with its computed value , gives us the means a ' / M of determining being known pretty exactly , and therefore , a E E - M E - M or μ E + M wn ) , being known ) , that is , the ratio of ...
... observed ( amounting , at its maximum , to 122 " ) with its computed value , gives us the means a ' / M of determining being known pretty exactly , and therefore , a E E - M E - M or μ E + M wn ) , being known ) , that is , the ratio of ...
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Mathematical Tracts on the Lunar and Planetary Theories, the Figure of the ... George Biddell Airy Uten tilgangsbegrensning - 1858 |
Mathematical Tracts on the Lunar and Planetary Theories, the Figure of the ... George Biddell Airy Uten tilgangsbegrensning - 1858 |
Mathematical Tracts on the Lunar and Planetary Theories: The Figure of the ... George Biddell Airy, Sir Ingen forhåndsvisning tilgjengelig - 2016 |
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