IV—Winds, Currents and Sailing Routes

1977 ◽  
Vol 30 (2) ◽  
pp. 182-184
Author(s):  
Charles H. Cotter

The pattern of surface winds on an ideal non-rotating uniform Earth would be related to the distribution of surface temperatures. This would lead to atmospheric pressure gradients which, in turn, would produce surface winds. The effect of the Earth's rotation produces the so-called ‘Planetary Wind System’, and the actual pattern of surface winds is often considered to be a modification of this. But many factors influence the global wind system to such an extent that the explanation of any part of the system at any given time is a matter of considerable complexity. Moreover, experience has amply demonstrated that despite the close attention of physicists the accurate forecasting of winds for more than a day or so ahead has not met with hoped-for success.

1966 ◽  
Vol 25 ◽  
pp. 323-325 ◽  
Author(s):  
B. Garfinkel

The paper extends the known solution of the Main Problem to include the effects of the higher spherical harmonics of the geopotential. The von Zeipel method is used to calculate the secular variations of orderJmand the long-periodic variations of ordersJm/J2andnJm,λ/ω. HereJmandJm,λare the coefficients of the zonal and the tesseral harmonics respectively, withJm,0=Jm, andωis the angular velocity of the Earth's rotation. With the aid of the theory of spherical harmonics the results are expressed in a most compact form.


1992 ◽  
Vol 30 (4) ◽  
pp. 196-196
Author(s):  
Robert Lanni

Peritia ◽  
1997 ◽  
Vol 11 ◽  
pp. 378-381
Author(s):  
D. P. McCarthy

Science ◽  
1943 ◽  
Vol 97 (2510) ◽  
pp. 138-138
Author(s):  
P. KIRKPATRICK

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