Transactions of the Cambridge Philosophical Society, المجلد 22University Press, 1923 |
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الصفحة
... Molecules from an Atmosphere , with special reference to the Boundary of a Gaseous Star . By E. A. MILNE , M.A. , Trinity College , Cambridge 483 XXVII . Some Problems of Diophantine Approximation : The Analytic Properties of Certain ...
... Molecules from an Atmosphere , with special reference to the Boundary of a Gaseous Star . By E. A. MILNE , M.A. , Trinity College , Cambridge 483 XXVII . Some Problems of Diophantine Approximation : The Analytic Properties of Certain ...
الصفحة 482
... MOLECULES FROM AN ATMOSPHERE , WITH SPECIAL REFERENCE TO THE BOUNDARY OF A GASEOUS STAR BY E. A. MILNE , M.A. , TRINITY COLLEGE , CAMBRIDGE CAMBRIDGE AT THE UNIVERSITY PRESS M.DCCCC.XXIII ADVERTISEMENT THE SOCIETY as a body is not to be ...
... MOLECULES FROM AN ATMOSPHERE , WITH SPECIAL REFERENCE TO THE BOUNDARY OF A GASEOUS STAR BY E. A. MILNE , M.A. , TRINITY COLLEGE , CAMBRIDGE CAMBRIDGE AT THE UNIVERSITY PRESS M.DCCCC.XXIII ADVERTISEMENT THE SOCIETY as a body is not to be ...
الصفحة 482
... acknowledgments to the SYNDICS of the University Press for their liberality in taking upon themselves the expense of printing this Volume of the Transactions . PRINTED IN GREAT BRITAIN XXVI . The Escape of Molecules from an Atmosphere ,
... acknowledgments to the SYNDICS of the University Press for their liberality in taking upon themselves the expense of printing this Volume of the Transactions . PRINTED IN GREAT BRITAIN XXVI . The Escape of Molecules from an Atmosphere ,
الصفحة 483
... molecules . The gravitational potential falls off only as the inverse first power of the distance , and it is easily calculated that for a Orionis , in spite of its large radius and consequently low surface value of gravity , the ...
... molecules . The gravitational potential falls off only as the inverse first power of the distance , and it is easily calculated that for a Orionis , in spite of its large radius and consequently low surface value of gravity , the ...
الصفحة 484
... molecules possessing sufficient velocities at that level are free to escape . It will appear that by this means a direct rough evaluation of the density and height of the escape layer is possible , and that the formula for the rate of ...
... molecules possessing sufficient velocities at that level are free to escape . It will appear that by this means a direct rough evaluation of the density and height of the escape layer is possible , and that the formula for the rate of ...
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a₁ angle approximately asymptotic expansion atmosphere Axiom of Archimedes axis b₁ c₁ calculated coefficients considered constant convergent convex set cordon corresponding cos² curve d₁ definition denote density determined differential equations disturbance diurnal diurnal variations dyadic earth equal escape expression factor finite follows formula free path function G. H. Hardy giant star given h₂ Hence integral equation invariant Jacobian k₁ k₂ magnitude molecules obtained orbit paper parameters partitions plane positive potential Primitive Roots ratio relation respectively result rotation scalar shew shewn sin² solar solid angle solutions substitution suppose surface t₁ theorem theory v₁ values vector velocity w₁ X₁ XXII zero Σ Σ дх